Telescopes no longer in operations by CTIO or SMARTS.
The SMARTS 1.3 meter telescope has been close since late August 2019.
The SMARTS 1.3-meter telescope was previously the 2MASS southern telescope before SMARTS took over its operation. A permanently-mounted, dual-channel, optical-IR imager called ANDICAM takes simultaneous optical and infrared data on the telescope. The 1.3-m was operated entirely in service / queue mode.
ANDICAM started regular operations at the 1.3-m in February 2003 by the SMARTS Consortium. Previously, it had been operated in queue mode on the 1.0-m (YALO Consortium) with the optical detector since the 1998B semester. The IR array was installed in July 1999, enabling simultaneous optical and infrared imaging, including dithering in the IR channel while the optical channel integrates. ANDICAM was constructed by the Ohio State astronomical instrumentation group led by Darren DePoy and its construction was funded in part by the National Science Foundation.
ANDICAM takes simultaneous optical and infrared data by using a dichroic with a CCD and a HgCdTe array. A moveable mirror allows dithering in the IR while an optical exposure is going on. The primary purpose of the instrument is for microlensing event follow-up to look for the presence of planets and other anomalous behaviour. ANDICAM is operated by the Prospero control software. It also has a twin--DANDICAM (Dutch ANDICAM)--that is used on a 1m telescope in South Africa. With ANDICAM one can obtain UBVRIJHK photometry within a 6 arcmin (optical) or 1 arcmin (near-IR) field.
ANDICAM Resources
FILTER | Plot | Data file | |
CCD Filters | KPNO-B | kpno_b.pdf [4] | kpno_b.txt [5] |
KPNO-V | kpno_v.pdf [6] | kpno_v.txt [7] | |
KPNO-I | kpno_i.pdf [8] | kpno_i.txt [9] | |
Infrared Filers | J-band | andi_j.pdf [10] | j_andi.txt [11] |
H-band | andi_h.pdf [12] | h_andi.txt [13] | |
K-band | andi_k.pdf [14] | k_andi.txt [15] | |
Legacy Filters | YALO B | yalo_b.pdf [16] | b_yalo.txt [17] |
YALO wide R | yalo_r.pdf [18] | r_yalo.txt [19] |
Operational Information
Reports
General Information
1.3m Usage Summaries (2004-2006)
NOTE: The 1.3m has been removed from the CTIO exposure time calculator. The values obtained using this calculator were found to be too optimistic by several orders of magnitude. Please estimate you exposure times using the values found at the ANDICAM detector website.
Telescope Operator Instructions [21]
Optical Processing Procedure [35]
Reports and Logs
Nightly 1.3m Observing Log Archive [23]
1.3m Nightly Observer's Reports [24]
1.3m Telescope Trouble Reports [36]
Report Forms
Photometric Standards and Measurements Reports [37]
Nightly Observing Logs [38]
Nightly Observing Reports [21]
Daily Processing Reports [25]
delete this page.
delete this page.
March 2009
To assist you in reducing your infrared images, we are now providing combined infrared flat field images for each filter. These are created by combining all of the flat images that are taken at each dither position, producing one flat image for each filter. These can be downloaded from the ftp site in /home/ftp/pub/smarts13m/flatsir.
Separate flat field images (at each of the dither positions) will continue to be available from the same ftp directory as before (/home/ftp/pub/smarts13m/calibsir).
Please direct any questions to either Michelle Buxton or Suzanne Tourtellotte.
If you have to generate schedules for a telescope (or anything else) and are interested in streamlining the process, we recommend the software developed at NASA Goddard by the Science Goal Montior (SGM) group. The main website can be found here and you can download the specific software developed for SMARTS here. Email Michelle Buxton if you need help with creating the specific sun and moon files needed (this is currently done using another piece of software, XEphem).
The 1.3m/ANDICAM now has neutral-density filters installed for viewing bright sources in V, I, H, and narrowband He 1038nm. Tests with standard stars show that the V+ND combination has an attenuation of 4.6 (a factor of 39,000, or 11.5 magnitudes) over that of the V filter, and the I+ND combination an attentuation of 3.0 (1100, or 7.6 magnitudes).
The ANDICAM instrument has two optical neutral density filters, V+ND4 and I+ND4, and two infrared neutral density filters, H+ND4 and 10830+ND3. (The 10830+ND3 filter is a narrowband He filter.) The optical ND filters are 5-arcminute diameter round filters, and the IR ND filters are 2.4-arcmin square filters. According to the previous paragraph, the V+ND filter has an attenuation of 4.6 (a factor of 39,000, or 11.5 magnitudes) over that of the V filter, and the I+ND combination has an attenuation of 3.0 (1100, or 7.6 magnitudes).
From observations of Eta Car in the ND4 filters done by Alan Whiting, the FWHM generally ranges from 2.5 to 4.9 pixels in V. He also notes that flat fields taken through the attenuated filters have not been successful in calibrating the data. However, the flats from the unattenuated V, I, and H filters seem to work fine with ND filter observations.
We have spotted a peculiarity in observing the Landolt standard PG1323. It appears as though the light of a bright star (most likely Spica) outside the field of view is not properly baffled, causing the raised level of the background, as shown here:
In principle, this should not affect the count rate in the standard stars themselves, but, we do not recommend using this particular standard for your observations.
The 1.3m has been removed from the CTIO exposure time calculator. The values obtained using this calculator were found to be too optimistic by several orders of magnitude. Please estimate you exposure times using the values found at the ANDICAM detector website (http://www.astronomy.ohio-state.edu/ANDICAM/detectors.html#sens [39]).
PLEASE NOTE: The U filter is currently broken and unusable.
SMARTS optical images are processed with the IRAF task CCDPROC using a bias prepared with the IRAF task ZEROCOMBINE and a domeflat or skyflat prepared with the IRAF task FLATCOMBINE. As of November 1, 2006, the SMARTS optical images are processed slightly differently. In order to remove the low-level horizontal "banding" that we have seen at times during the last six months, the overscan is now fit with a cubic spline function of order 11. All other steps remain the same. The old processing parameters can be found here.
Modified 11/01/2006
===============================================================================
Ten biases are taken each night and are combined into a single
bias frame using the IRAF task ZEROCOMBINE.
The IRAF task ZEROCOMBINE parameters are set as follows:
I R A F Image Reduction and Analysis Facility |
|||
PACKAGE = ccdred | |||
TASK = zerocombine | |||
input = | List of zero level images to combine | ||
(output = | ZERO) | Output zero level name | |
(combine= | average) | Type of combine operation | |
(reject = | minmax) | Type of rejection | |
(ccdtype= | ) | CCD image type to combine | |
(process= | no) | Process images before combining? | |
(delete = | no) | Delete input images after combining? | |
(clobber= | no) | Clobber existing output image? | |
(scale = | none) | Image scaling | |
(statsec= | ) | Image section for computing statistics | |
(nlow = | 1) | minmax: Number of low pixels to reject | |
(nhigh = | 1) | minmax: Number of high pixels to reject | |
(nkeep = | 1) | Minimum to keep (pos) or maximum to reject(neg) | |
(mclip = | yes) | Use median in sigma clipping algorithms? | |
(lsigma = | 3.) | Lower sigma clipping factor | |
(hsigma = | 3.) | Upper sigma clipping factor | |
(rdnoise= | 0.) | ccdclip: CCD readout noise (electrons) | |
(gain = | 1.) | ccdclip: CCD gain (electrons/DN) | |
(snoise = | 0.) | ccdclip: Sensitivity noise (fraction) | |
(pclip = | -0.5) | pclip: Percentile clipping parameter | |
(blank = | 0.) | Value if there are no pixels | |
(mode = | ql) |
===============================================================================
VRI dome flats are observed every night, 10 exposures of each.
JHK dome flats are observed every third night in rotation. 10 exposures are taken at each of the 7 dither positions (dither throw = 40). 10 additional exposures at each dither position are then taken with the dome lamps off. The final flat at each dither position is the difference between the combined lamp-on flat minus the combined lamp-off flat.
B sky flats are taken due to undesirable artifacts present in the B domes. A minimum of 3 images are taken every night weather permitting. It is required that individual skyflats have different RA and
DEC values.
In all cases, the individual flats are processed first with CCDPROC for the overscan and zero corrections, then combined with FLATCOMBINE.
FLATCOMBINE parameters are set as follows for the SKY flats:
I R A F Image Reduction and Analysis Facility |
|||
PACKAGE = ccdred | |||
TASK = flatcombine | |||
input = | List of flat field images to combine | ||
(output = | FLAT) | Output flat field root name | |
(combine= | median) | Type of combine operation | |
(reject = | minmax) | Type of rejection | |
(ccdtype= | ) | CCD image type to combine | |
(process= | no) | Process images before combining? | |
(subsets= | no) | Combine images by subset parameter? | |
(delete = | no) | Delete input images after combining? | |
(clobber= | no) | Clobber existing output image? | |
(scale = | mode) | Image scaling | |
(statsec = | ) | Image section for computing statistics | |
(nlow = | 1) | minmax: Number of low pixels to reject | |
(nhigh = | 1) | minmax: Number of high pixels to reject | |
(nkeep = | 1) | Minimum to keep (pos) or maximum to reject(neg) | |
(mclip = | yes) | Use median in sigma clipping algorithms? | |
(lsigma = | 3.) | Lower sigma clipping factor | |
(hsigma = | 3.) | Upper sigma clipping factor | |
(rdnoise = | 0.) | ccdclip: CCD readout noise (electrons) | |
(gain = | 1.) | ccdclip: CCD gain (electrons/DN) | |
(snoise = | 0.) | ccdclip: Sensitivity noise (fraction) | |
(pclip = | -0.5) | pclip: Percentile clipping parameter | |
(blank = | 0.) | Value if there are no pixels | |
(mode = | ql) |
FLATCOMBINE parameters are set as follows for the DOME flats:
I R A F Image Reduction and Analysis Facility |
|||
PACKAGE = ccdred | |||
TASK = flatcombine | |||
input = | List of flat field images to combine | ||
(output = | FLAT) | Output flat field root name | |
(combine= | average) | Type of combine operation | |
(reject = | crreject) | Type of rejection | |
(ccdtype= | ) | CCD image type to combine | |
(process= | no) | Process images before combining? | |
(subsets= | no) | Combine images by subset parameter? | |
(delete = | no) | Delete input images after combining? | |
(clobber= | no) | Clobber existing output image? | |
(scale = | mode) | Image scaling | |
(statsec= | ) | Image section for computing statistics | |
(nlow = | 1) | minmax: Number of low pixels to reject | |
(nhigh = | 1) | minmax: Number of high pixels to reject | |
(nkeep = | 1) | Minimum to keep (pos) or maximum to reject(neg) | |
(mclip = | yes) | Use median in sigma clipping algorithms? | |
(lsigma = | 3.) | Lower sigma clipping factor | |
(hsigma = | 3.) | Upper sigma clipping factor | |
(rdnoise= | 6.5) | ccdclip: CCD readout noise (electrons) | |
(gain = | 2.3) | ccdclip: CCD gain (electrons/DN) | |
(snoise = | 0.) | ccdclip: Sensitivity noise (fraction) | |
(pclip = | -0.5) | pclip: Percentile clipping parameter | |
(blank = | 1.) | Value if there are no pixels | |
(mode = | ql) |
===============================================================================
Images are processed, one filter type at a time, with a bias and a skyflat of the corresponding filter type using the IRAF task CCDPROC. The result is a processed image, prefixed with the letter "r", that have been OZF'ed (overscanned, flattened and zeroed) but not T'ed (trimmed).
When biases are not taken for a given night, the ZEROCOMBINEd bias from the nearest available night is used instead. This bias will have already gone through CCDPROC with images of its same night. The bias section for use in overscanning was determined by IMPLOT to extend from less than 3 and more than 14, so [3:14,1:1024]) was chosen as the overscan strip image section.
When contemporaneous skyflats are not available, FLATCOMBINEd skyflats from previous nights are used instead. These skyflats will have already been processed using their own contemporaneous biases.
The IRAF task CCDPROC parameters are set as follows:
I R A F
Image Reduction and Analysis Facility
PACKAGE = ccdred
TASK = ccdproc
I R A F Image Reduction and Analysis Facility |
|||
PACKAGE = ccdred | |||
TASK = ccdproc | |||
images = | @in.(filtertype) ) | List of CCD images to correct | |
(output = | @out.(filtertype) ) | List of output CCD images | |
(ccdtype= | ) | CCD image type to correct | |
(max_cac= | 0) | Maximum image caching memory (in Mbytes) | |
(noproc = | no) | List processing steps only? | |
(fixpix = | no) | Fix bad CCD lines and columns? | |
(oversca= | yes) | Apply overscan strip correction? | |
(trim = | no) | Trim the image? | |
(zerocor= | yes) | Apply zero level correction? | |
(darkcor= | no) | Apply dark count correction? | |
(flatcor= | yes) | Apply flat field correction? | |
(illumco= | no) | Apply illumination correction? | |
(fringec= | no) | Apply fringe correction? | |
(readcor= | no) | Convert zero level image to readout correction? | |
(scancor= | no) | Convert flat field image to scan correction? | |
(readaxi= | line) | Read out axis (column|line) | |
(fixfile= | ) | File describing the bad lines and columns | |
(biassec= | [3:14,1:1024]) | Overscan strip image section | |
(trimsec= | ) | Trim data section | |
(zero = | ccd(night).bias) | Zero level calibration image | |
(dark = | ) | Dark count calibration image | |
(flat = | ccd(night).sky/domeflat(filter) ) | Flat field images | |
(illum = | ) | Illumination correction images | |
(fringe = | ) | Fringe correction images | |
(minrepl= | 1.) | Minimum flat field value | |
(scantyp= | shortscan) | Scan type (shortscan|longscan) | |
(nscan = | 1) | Number of short scan lines | |
(interac= | no) | Fit overscan interactively? | |
(functio= | spline3) | Fitting function | |
(order = | 11) | Number of polynomial terms or spline pieces | |
(sample = | *) | Sample points to fit | |
(naverag= | 1) | Number of sample points to combine | |
(niterat= | 1) | Number of rejection iterations | |
(low_rej= | 3.) | Low sigma rejection factor | |
(high_re= | 3.) | High sigma rejection factor | |
(grow = | 0.) | Rejection growing radius | |
(mode = | ql) |
General-purpose photometric standards are observed every photometric night on the 1.3m telescope.
The procedure is as follows:
Each photometric night, 1 Landolt field is observed ONCE in all optical filters. In addition, 2 IR standards (one blue and one red) are observed ONCE in all IR filters. Because extinction coefficients cannot be calculated on such nights, "default" values (see below)are used for calculations of zeropoints and color terms.
Periodically, more thorough observations of the same standards are performed, observing each of the 3 standard fields (1 Landolt, 2 IR fields) at 3 different airmasses in order to calculate extinction coefficients. The medians of these values, taken over many months, are the "default" extinction coefficients mentioned above.
Standard star images are available to all users and are not charged against their allocation. We do our best to choose those Landolt fields with at least 3 standard stars available in the field of view. If your program requires additional standard observations, please include them in your PhaseII submission. Additional observations are charged against your allocation.
Photometric Results | Optical [43] | Infrared [44] | |
Extinction Coefficients Values | Optical [45] | Infrared [46] | |
Description of Photometric Calculation Methods | Optical [47] | Infrared [48] |
SMARTS Consortium [49]
ANDICAM & CTIO 1.3m Telescope Contact Information
Program coordinators are responsible for the coordinating their institution's shares of the SMARTS telescope time. Members of the U.S. and Chilean astronomical communities granted time on SMARTS telescopes and instruments through the NOAO TAC should work with the AURA/NOAO coordinator.
These contacts are for both SMARTS in general and ANDICAM in particular:
SMARTS Operations:
Prof. Charles Bailyn (charles.bailyn@yale.edu [50])
SMARTS Consortium General Manager
Victoria Gardner (victoria.gardner@yale.edu [51])
SMARTS Administrative Coordinator
Ohio State University:
Prof. Darren DePoy (depoy@astronomy.ohio-state.edu [52])
Instrument configuration and future upgrades
Prof. Richard Pogge (pogge@astronomy.ohio-state.edu [53])
Data-Acquisition and Observing Preparation/Tracking Software
ANDICAM Observing Queue Manager:
Dr. Michelle Buxton (Yale) (michelle.buxton@yale.edu [54])
Data Processing and Archving Manager:
Dr. Suzanne Tourtellotte (Yale) (swt@astro.yale.edu [55])
ANDICAM Instrument Scientist:
Prof. Darren DePoy (OSU) (depoy@astronomy.ohio-state.edu [52])
CTIO Operations:
Dr. R. Chris Smith (CTIO) (csmith@noao.edu [56])
ANDICAM Web Pages & Observing Preparation Tools:
Prof. Richard Pogge (OSU) (pogge@astronomy.ohio-state.edu [53])
NOAO Observer Programs:
Dr. R. Chris Smith (CTIO) (csmith@noao.edu [56])
This page provides access to tools for preparing, submitting, and tracking the progress of "Phase II" observing programs approved for scheduling on the CTIO 1.3-meter [40] telescope and ANDICAM [57] .
Access to these tools is via a login screen [58]. If you have been granted time with ANDICAM [57] but not yet received a SMARTS Project ID code for your observing program, please contact your program coordinator [59].
Login to the ANDICAM Phase II Observing Pages [58]
Information:
Phase II Submission Instructions [60]
Observation Template (Obs File) Creation Form Instructions [61]
Multi-Observation Script Creation Form Instructions [62]
Phase II Observing Program Submission Form Instructions [63]
Once a project has been approved for observing with ANDICAM, the PI needs to submit a detailed "Phase II" observing plan to the queue manager. This plan consists of a set of observations to be carried out, each "unit" observation of which is described by one or more data-acquisition template files called "Observation Templates" or "obs files". A set of written instructions for how to use these obs files to execute your program observations rounds out the Phase II submission package. Other elements may be required for more complex programs or those with long target lists.
We have adopted a web-based electronic submission process built around a suite of simple web forms. The observing program submission procedure is analogous to "Phase II" observing preparation for Hubble Space Telescope, Gemini, WIYN, or the ESO NTT and VLT. Indeed, many ideas and examples from those systems were used in considering the development of these tools. The CTIO 1.3m has only one instrument with three well-defined observing modes, so it should be very straightforward to use efficiently, and the Phase II process is therefore proportionally simpler than these other observatories. Our highly successful experience with this observing mode at the Yale 1-meter telescope bears out this expectation.
ANDICAM observing programs generally come in three broad types: Synoptic, Survey, and Target-Of-Opportunity.
These are programs in which you wish to observe a relatively small number of variable targets many times over the course of an observing season. For these programs, you will generally create a small number of single-target obs files that will get executed many times.
In cases where each target requires either a large number of separate obs files (e.g., 5 obs files, one for each of the UBVRI filters), or a small number of obs files to be executed in a specific sequence with repeats (e.g., I+H and V+H dual-mode observations, executed in the sequence "VIIV"), you have the option of creating an additional multi-observation script that will define the observing sequence made up of particular obs files. For "complex" synoptic programs, use of multi-observation scripts can improve the efficiency of your program (there is less for the on-site observer to type).
These are programs in which you have a relatively large number of targets that you wish to observe only once, but in many filters. For example, a program to obtain UBVRI+JHK images of a sample of 100 cool subdwarf stars would require you to create nearly 500 separate obs files using only single-target files. This is clearly ridiculous.
To make execution of such programs easier, you would settle on some standarized set of exposure times (e.g., either one set for all in each filter, or divide your sample into long and short exposure time groups), and then create a small set of multi-target obs files for each generic set. These obs files have no target specifications (name and coordinates), only filter and exposure settings.
You would then create a multi-observation script to wrap around these generic obs files which would be executed by the on-site observer to take your observations. The script prompts the observer to enter the target name each time, ensuring that the correct object name makes it into the header. A complete target list with coordinates, specifying which are to be observed with which multi-observation script, rounds out your Phase II submission.
For our example of the 100 star UBVRI+JHK observing program, we might divide the sample into two exposure time sets (long and short), and create 5 multi-target obs files for each filter combination for each set. This would reduce the number of Phase II observing files needed to execute the program from 500 to 12: 6 files for each of the long and short sets, each of which consist of 5 multi-target obs files and 1 multi-observation script to execute them. The advantages of combining generic obs files with scripts is considerable.
These are one-time programs triggered by transient events like novae, supernovae, gamma-ray bursts, etc. TOO programs must be pre-approved (if NOAO time), or you must warn the queue management team in advance if you think you will be requesting TOO observations. Politics apply, so keep on top of the situation. In the event of super-rare events (e.g., a Galactic or LMC/SMC Supernova), we will coordinate all observations by the SMARTS consortium as a whole.
TOO programs will be treated like single-target synoptic programs. You will need to prepare single-target obs files (and any optional multi-observation scripts) in advance of calling in the TOO trigger, and submit a Phase II program using the regular forms.
Important! TOO programs requested after 3:30pm Eastern Time (1530 EST or EDT) will be executed that night at the discretion of the queue manager, otherwise they will be deferred to the next night. We remind all principal investigators that they are specifically forbidden to call up the on-site observers directly, and note that the on-site observers are empowered to hang up on you politely (in fact, they are instructed to ignore all such extraneous calls). Maintaining a clear, unambiguous "chain of command" is absolutely essential for smooth remote queue operations, so no matter how important it is, please work through the proper channels. Repeat offenders will have their observing programs terminated with extreme prejudice.
The Phase II submission process has 3 steps, as follows:
Projects awarded time with ANDICAM on the CTIO 1.3m Telescope (either via the SMARTS consortium or the NOAO TAC) are assigned a Project ID code their programs. This ID is your entry point into the observation preparation tools on this web server. Using these tools, you can create obs files for your observing program, and edit or delete existing obs files. The obs files reside on the server in separate directories assigned to each approved project.
If you do not find your project ID in the list, contact the SMARTS queue manager or NOAO SMARTS Program Coordinator [67] (as appropriate). Please do not appropriate someone else's project space.
Observation Template Files ("obs files" for short) are used by the ANDICAM data-taking system to execute your observations. A set of web forms are provided to help you create obs files that have the correct format (eliminating syntax errors if you try to make them by hand). In addition, these obs file creation tools provide estimates of the amount of time required to execute an observation, exclusive of target acquisition and setup time. These estimates will help you optimize the data-acquisition for your program, especially for those programs that will be acquiring simultaneous IR and CCD images. Instructions for the creation of obs files is described in the ANDICAM Observation Template Files document. Please read this document carefully.
If you are submitting a survey-type program, you also need to create a multi-observation script to execute your multi-target obs files. Programs that make use of multi-target obs files are required to submit valid multi-observation scripts with their Phase II program.
Similarly, if you have a complex synoptic program, you may wish to also prepare one or more optional multi-observation script to execute your single-target obs files in a particular sequence. These scripts are optional for single-target programs, and should only be done if necessary.
Once you have created a complete set of obs files for all targets in your program (or a set of multi-target obs files and associated multi-observation scripts), the Phase II Observing Program Submission Form is used to submit the obs files, multi-observation scripts, and your detailed narrative instructions to the ANDICAM queue manager for eventual scheduling and implementation. This form is accessed from the main observing preparation menu after you have logged in (see Step 1 above).
The Phase 2 submission form copies your observing files and the instructions (in an ASCII text file) to an ftp staging disk, and emails the instructions to the queue management team (via the andicam-submit mailing list). Once on the staging disk, the files will be downloaded by the queue manager or by the on-site observers (at the queue manager's instructions) to CTIO where they will be used to execute your program when it is scheduled. Click here for detailed instructions for using the Phase II program submission form.
In preparing your Phase II submission for execution, the queue management team, in consultation with the instrument scientists, may require changes in your program if the proposed observations present an unusually complicated execution problem, or present book-keeping or execution-time problems for the on-site observers. Programs that require excessive execution time may be sent back for reduction in scope.
In addition to submitting your Phase II observing program, these forms can be used to submit updates, corrections, and amendments to your program. The nature of the submission should be clearly spelled out at the top of the narrative instructions.
NOTE: Phase II files and instructions must be submitted by 3:30pm EST/EDT for the targets to be scheduled in that night's queue. Please contact the queue manager if this deadline presents a major problem to your program's feasibility.
Time with the ANDICAM is generally awarded as a given number of hours of observing time to be devoted to a project. "Observing" in this context includes not only the amount of time spent collecting photons, but also the target acquisition, setup, and system overheads. These overheads are included in your time allocation (same as they would be if you were awarded, for example, a night of observing or some number of HST orbits). How efficiently you can observe determines what fraction of your time allocation is spent collecting photons.
Each obs file you create includes an estimate of the execution time. This execution time only includes the operations that occur between the observer typing "GO" for that obs file and when the last image in the obs file has finished being readout. This overhead calculation includes detector setup and readout times, as well as the requested integration times. These times are all highly predictable. Separate estimates are given for the CCD and IR channels (as appropriate), to help you evaluate how much deadtime there will be (the execution time for an obs file is the longer of the two estimates). Details on how this estimate is computed is included in the ANDICAM Observation Template Files document.
This is not the whole story, however. The individual obsfile execution time estimates do not include the following unpredictable overheads:
1. Instrument configuration times, which typically run a 1-4 seconds per operation, and usually at most 10 seconds per obs file. These times are so short to be treated as "noise" in the process. For example, if the filter and exposure times from the previous obs file are the same as yours, there is no overhead, but if they must be changed, it takes 1 second to change the exptime and 1-4 seconds to change a filter (depending on the amount of motion required). Hence why we don't compute them since they depend unpredictably on what observations came before.
2. Telescope Pointing & Target Acquisition (TP&TA). This typically requires between 3 and 5 minutes per pointing, and includes such unpredictables as telescope slew time, target acquisition offsets (though the 1.3m points admirably well, sometimes your target may be hard to identify the first time), and guide star acquisition (time to select a suitable guide star and lock the guider). If your program is simple (point to a target and take a series of images using a set of obs file), this TP&TA overhead will have a minimal impact on your time allocation. However, if your program requires a lot of pointings or offsets at a particular location, it will cut into the observing efficiency because of the greater TP&TA requirements, ultimately reducing the amount of your time allocation that is actually spent collecting photons.
In estimating the amount of time your Phase II submission will require, the ANDICAM queue managers at Yale will factor in a nominal TP&TA overhead, and combine the overheads from your individual obs files. If the amount of time you request exceeds your allocation, or looks to present an unusually low-efficiency observation, you will be contacted by them and asked to revise your observing project so as to both meet your scientific needs and have a program that does not present execution problems for the 1.3m on-site observers.
Note that requests for additional calibration data (e.g., special flats other than the ones acquired generally for all projects, or special flux calibration targets) do count against your time allocation. These are handled on a case-by-case basis by the queue management team at Yale.
In general, you will be informed by email when observations for your program have been acquired and are ready for pickup from the FTP server at Yale. In between times, however, you can track the progress of your program electronically in a number of ways:
You can receive a copy of the nightly observing logs by subscribing to the andicam-logs mailing list. Instructions for subscribing and unsubscribing to this list may be found in the ANDICAM Mail Lists document.
When you login to the Phase II Observing Tools page for your project, a simple search tool is provided that will extract all observing log entries for your Project ID. You can also extract observing log entries for a restricted range of dates, or for which a particular keyword (e.g., a target name) matches. All searches on keywords are case-insensitive. This allows you to get to the info you need on your program's observations without having to wade through all of the others.
If you have problems using these web tools, or have comments that you think will improve their usefulness, please send your feedback to the Queue Management personnel at SMARTS2 at Yale (see the contact list for the current personnel).
Updated: 2006 May 11 [rwp/osu]
SMARTS Consortium
Creating ANDICAM Multi-Observation Scripts
Updated: 2003 March 1
Table of Contents:
* Overview
* How to Create Multi-Observation Scripts
o Step 1: Select Obs files to execute
o Step 2: Prompt for Target Name?
o Step 3: Enter the Script Filename
* Example Multi-Observation Scripts
Overview
The ANDICAM is a 2-channel instrument with separately configurable CCD and IR cameras fed by a dichroic beam splitter. To enable efficient queue scheduling of observations, all ANDICAM data are acquired by means of Observation Template Files (or "obs files" for short) prepared by the astronomer. Obs files define "unit observations", specifying the instrument, detector, and target parameters and configurations needed to acquire a single observation.
In addition, astronomers can create simple Multi-Observation Scripts that are used to execute a sequence of obs files for a single target. There are two basic uses of Multi-Observation Scripts:
Complex Synoptic Observations:
A "synoptic" program is here defined as one in which you wish to observe a relatively small number of targets many times over a long period of time. A "complex" synoptic program is one in which the target is to be observed through a number of different filters in a specific sequence. In this case, you would create separate single-target obs files for each exposure-time and filter combination required for a given target (and do so for each of your targets). After your obs files have been created, you make a set of multi-observation scripts that would be used to execute each of these obs files in the preferred sequence each time, including repeats, for each target. Examples are given below.
Note that for standard single-target obs files, multi-observation scripts are optional, and should only be done if the observations are of particular complexity (e.g., many different exposure/filter combinations that must be executed in a particular sequence or a pattern of repeat observations required in a single continguous sequence). Don't make and submit multi-observation scripts if you don't really need them, as they do complicate the Phase II submission process, and are inappropriate for execution of just 1 or 2 single-target obs files.
Survey Observations:
A "survey" project is broadly defined as one in which you wish to observe a number of targets in the same way in many filters only once (or at most a couple of times). In this case, having to create a number of separate single-target obs files for all of the targets quickly becomes a burden for both the astronomer (who has to create them all) and for the observers (who have to keep them organized). The "one obs file per observation per target" mode that works well for synoptic programs is clearly impractical for even medium-sized survey projects, especially if you want to observe each target in many filters.
A better solution is to create a small set of generic multi-target obs files that contain exposure and filter settings, but do not specify the targets or their coordinates. A multi-observation script would then be created to execute these generic obs files for all of your targets, and the script would include the option to prompt the observer to enter the target name. Thus a single multi-observation script and a small set of generic obs files stands in for many separate obs files. The trade-off is that you must standardize exposure times, or divide your program into "long" and "short" exposure sequences and provide sets of generic obs files and associated multi-osbservation scripts for each. The examples section below discusses some strategy issues (a simple observing program is more likely to get executed than a very complex one). A separate target list with coordinates would be submitted with the Phase II instructions to round out your program submission.
For submission of survey-style projects, use of multi-target obs files and multi-observation scripts is mandatory.
In general, multi-observation scripts are not useful if you have relatively simple programs (at most one or two obs files per target). The gain in using them comes with large numbers of targets, or large numbers of observations per target that must come in a specific sequence.
This document describes how to create multi-observation scripts for your observing program, and gives worked examples.
[Contents]
How to Create Multi-Observation Scripts
Multi-observation scripts are created using a webform accessed by logging into the Observing Preparation Tools pages (via the Phase II front page), and using the Project ID assigned to your project when it was approved for implementation and scheduling. Scripts are created after you have created the obs files for your program. Once you have made your multi-observation scripts, you will submit them along with your obs files as part of the Phase II Observing Program Submission.
There are two basic types of multi-observation script:
1. Single-Target Scripts that execute a set of single-target obs files in a particular sequence, including repeats.
2. Multi-Target Scripts that execute a set of generic multi-target obs files in a specific sequence for many different targets, each time prompting the observer to enter the target name.
Step 0: Create the set of observing template files
Multi-observation scripts are created after you create your basic set of observing template files for your program. If there are no obs files, the script creation form will not have anything to work with.
Step 1: Select obs files to execute
Each multi-observation script may execute up to 10 obs files in sequence. This includes repeat observations of a given obs file. the form presents you with a set of 10 pull-down boxes, the menu containing a list of all of the obs files you have currently in your project's working directory on this server.
The obs files you select will be executed in the order selected, top to bottom in the form. Blank selections are ignored). If you wish to execute a given obs file twice in sequence, it must be selected twice.
Step 2: Prompt for Target Name?
If the obs files selected above are generic multi-target obs files that do not contain target names or coordinates, then your script will need to prompt the observer to enter the target name before the obs files are executed. Check the box to create a prompt in the script. If you omit this, no object name will be put into the image headers or observing logs, making it impossible to know what was observed.
If instead your script is executing standard single-target obs files, leave this box unchecked. If you do check it, the observer will have to type something at the prompt, and then what is typed will be overridden by what is in the subsequent obs files.
Step 3: Enter the script filename
Finally, you need to provide a unique filename for your multi-observation script. It should be descriptive of the obs files it contains, and should be unique to your project insofar as possible, so generic names like "myscript" or "script1" are discouraged. Filenames that conflict with other programs will be renamed at the discretion of the queue manager.
The filename you give must not have a file extension appended. A file extension (.pro) will be automatically assigned by the system, and has a specific meaning to the data-taking system. Adding a file extension could result in a script that cannot execute.
Example Multi-Observation Scripts
Example 1: Multi-Filter Synpotic Observations
In this example, the program is to make nightly observations of the microlensing source OB03018. Two obs files have been prepared
ob03018ih
ob03018vh
and each night the target is to be observed in the sequence
I+H
V+H
I+H
Using the form you would make 3 obs file selections, in order
ob03018ih
ob03018vh
ob03018ih
and leave the other 7 entries blank.
Since this is a set of single-target observations, you would leave the "Prompt for Target Name?" check box blank, as having the observer type in the target name would be redundant and a waste of time, since the target name in the obs files proper would override whatever they type.
Since this script is for a specific target, you would select a simple filename, the target itself:
ob03018
Which choice keeps the book-keeping simple for all concerned.
Example 2: Stellar Photometry Survey
This program is to acquire UBVRI and JHK images of a set of 200 low-mass stars from the 2MASS catalog. Since all of the stars are of comparable brightness, the same exposure times can be used for each star for the various filters. Since the H and K observations will take longer than J, we will double them up, taking J only with the most efficient R filter. The resulting set of 5 multi-target obs files is:
2masslm_uk
2masslm_bk
2masslm_vh
2masslm_ih
2masslm_rj
Here we have used "2masslm" as the base name (for "2MASS Low Mass") and specified the filters used in each obs files.
Using the form you would make 5 obs file selections, in order
2mass_uk
2mass_bk
2mass_vh
2mass_rj
2mass_ih
so that the optical imaging is acquired in the order UBVRI, and leave the other 5 entries blank.
Since this is a set of multi-target obs files, you would check the "Prompt for Target Name?" box. The observer will be prompted to enter the target name each time he/she executes the script.
Because this script is for many targets, a generic but suggestive name would be:
2masslm
this choice is the same as the "root name" of the obs files, making the association between them, and the program proper, clear.
Example 3: Multiple Targets, but long & short exposures
In this example, you have a large number of quasars from the LBQS, but about half the targets require relatively long exposures (e.g., 300s at V) whiel the others are brighter targets that would saturate in this time and can be observed with shorter exposures (e.g., 120s at V).
To handle this situation, you would create two sets of obs files, first a set of "long" observations templates:
lbqs_l_vh
lbqs_l_rh
lbqs_l_ij
and a parallel set of "short" observation templates
lbsq_s_vh
lbsq_s_rh
lbsq_s_ij
You then divide your sample into "long" and "short" targets, and create two multi-object scripts:
lbqs_long
lbqs_short
to execute the long and short sequences, respectively. In both cases, you need to makes sure you check the "Prompt for Target Name?" box so that the quasar's name is correctly entered by the observer.
As a general point of strategy, fine-tuning exposure times is a waste of time. If you really think one object has to have 320s at V and another 280s, then you will have to create separate single-target obs files for them. Since this places a greater book-keeping burden on the observers, it will cut into the observing efficiency, and it will require you to create each of the individual obs files. The on-site observers will not fine-tune obs files, and they will not edit obs files on the fly. That cuts too deeply into the observing efficiency. Inefficient Phase II programs will be returned to the astronomer with instructions for revision if it is felt that they will have to high of an impact on observing efficiency.
[Contents]
If you came here from one of the entry forms, use the "BACK" button on your browser to return to the obs file generation form in progress.
Updated: 2003 March 1 [rwp/osu]
SMARTS Consortium
ANDICAM Observation Template (Obs) Files
Updated: 2003 August 6
The ANDICAM is a 2-channel instrument with separately configurable CCD and IR cameras behind a dichroic beam splitter that can acquire simultaneous CCD and IR images. To enable efficient queue scheduling of observations, all data with ANDICAM are acquired by means of Observation Template Files (or "obs files" for short).
Obs files define the target parameters and the instrument and exposure configuration of the smallest schedulable "unit observation" that can be acquired with the ANDICAM. A "unit observation" means that the choice of filters and the base integration times for each channel are fixed, but multiple images with those filters and integration times may be acquired. Similarly, IR channel observations can be dithered between images using internal tip/tilt mirror. If observations with different filters or exposure times are required, the astronomer must create a different obs file. Some examples are described below.
Each obs file consists of the following basic blocks:
Project ID Block:
SMARTS Project ID used to assign "ownership" of the data acquired to a particular project.
Target Block:
Contains the target name and coordinates (RA, Dec, and Equinox). In a generic multi-target observing template, the target name and coordinates will be omitted.
Observation Block:
Specifies the observing mode (DUAL, CCD-only, or IR-only), and the exposure parameters, as follows:
CCD Block with the CCD observing parameters (filter, exposure time, number of images to acquire, etc.), if required.
IR Block with the IR observing parameters (filter, exposure time, number of co-adds and sequential images, dithering parameters, etc.), if required.
While obs files have been primarily designed for efficient simultaneous CCD and IR imaging, they also provide a consistent and logical way to schedule single-channel observations (i.e., CCD-only or IR-only imaging) with ANDICAM. This allows us to simplify the suite of commands needed to take data in each of the ANDICAM's 3 modes, which in turn simplifies the work of the on-site observers and the queue manager. It also ensures that the unused detector channel is kept idle while the other is active.
A set of obs files for a given target can be executed in a specific sequence by creating an optional multi-observation script. This is most often done for complex multi-wavelength observations (e.g., UBVRI+JHK photometry), or for "survey" projects in which many targets are observed once in the same way using a set of pre-defined templates. A special web form is provided to help you create simple multi-observation scripts as part of the Phase II observing preparation process. Use of such scripts can greatly simplify the execution of your observations. Note that if you are creating multi-target obs files for survey-type projects, use of multi-observation scripts is required.
Once you have created all of the obs files (and any associated scripts) for your program, you need to submit them along with a set of detailed observing instructions to the queue manager for evaluation, scheduling, and implementation. This is done using a separate "Phase II Submission Form". See the Phase II Observing Program Electronic Submission Instructions for details [68].
Obs files are created in three steps using a multi-part web form. This form is accessed by logging into the Observing Preparation Tools pages (via the Phase II Front Page [69]) and using the Project ID assigned to your project when it was approved for implementation and scheduling.
The first step in creating a set of obs files for a target is to specify the information for the target proper. You have two basic options:
Single Target:
In which the obs file is to be used for a single, specific target. In this case you would enter the following information:
1. The name of the target.
2. The RA and Dec of the target, and the equinox of the coordinates.
3. Indicate whether the target is a solar system object (i.e., a moving target requiring ephemerides or other time-dependent sources of coordinates).
Multiple Targets:
In which the obs file is to be used as a generic observing template for many different targets that will share the same detectors, filters, and exposure times. In this case, no target information need be entered.
In addition, you need to also specify the imaging mode you wish to use, which is one of:
1. CCD-only (no IR imaging).
2. IR-only (no CCD imaging).
3. Dual CCD+IR Imaging (simultaneous imaging in both channels)
Once you have entered this information, hitting the "Next>" button on the form will pass you into the exposure parameter entry form.
After entering the target info, you will be given a blank form for entering the exposure parameters for the observations. As described above, obs files are used to perform unit observations with a given instrument configuration. These units can be combined into multi-part imaging "sequences" using Prospero scripts that execute each of the separate obs files in turn.
For example, to take BVI images of an object, you would create three separate obs files, one for each of the B, V, and I filters. You would then have the on-site observers execute the obs files one at a time by hand, or create a multi-observation script to execute them in a sequence (thus reducing three execution steps into one: executing the script).
Once you have entered the exposure parameters for a given configuration, hitting the "Next>" button will then validate and analyze the entries.
You will next be shown a summary of the observation parameters you entered on the previous form along with an execution time analysis. At this point you need to review the parameters for errors. The project PI's are responsible for making sure that everything is correct before submission. You can use the browser's "Back" button to return to the exposure parameter entry form, make changes, and iterate until everything is ready before submitting the final obs file.
The exposure parameters you entered on the previous form are analyzed to make an estimate of the total amount of time that will be required to execute the requested exposures sequence. This estimate includes the unit integration times in each channel, number of images to be acquired, detector reset and readout times, IR mirror dithering motion overheads, etc., as appropriate. In general, the estimates are good to about 5% or so. The estimates do not, however, include instrument configuration overheads (e.g., changing filters or entering user parameters like the object name and coordinates), telescope configuration, etc. These latter will add to the total time it takes to execute your observation program. In general, instrument-related overheads add only ~10 seconds for each target/instrument change.
The estimates provided by the execution time analysis are meant to serve two purposes:
1. To aid the proposer in optimizing 2-channel observation to minimize dead-time.
2. To provide guidance to the queue manager in scheduling the observations.
From the proposer's perspective, the first provides a way to make sure that time that could be spent collecting more photons is not wasted because the CCD and IR operations are mismatched. For example, you might find that your first choices of integration times leave 64s of "dead time" on the IR channel while the CCD is still integrating and reading out. The web tools provided allow you to assess the impact is of adding an extra 60-second IR image to the obs files to close the gap. The web tools have been designed to make this kind of optimization exercise straightforward.
If you need to adjust any of the exposure parameters, use the "Back" button on your browser to return to the exposure parameter entry form in Step 2, make the changes, and then repeat the validation step. You can iterate as often as you like until you get things the way you want them. This way you avoid making lots of intermediate files that pile up on the disk (you can always clean up later with the Obs File Manager, but why make extra work?
It bears repeating that the estimates of execution times do not include such factors as the time required to setup the observation (e.g., setting the filters, exposure times, object names, etc.), nor do they include the computer-to-disk data-transfer times. They only provide estimates of the time it takes to perform those operations that occur from the moment the first exposure in the sequence begins until the last image is readout. All of the other configuration and data-transfer overheads cannot be predicted with any precision, the former because it depends critically on the previous configurtion of the instrument, and the latter because the inter-machine data-transfer system has a roughly factor of 4 range of transfer speeds (roughly 1Mb/sec to 4Mb/sec) governed by such ineffibles as the disk caching, how busy the up/downstream machines are, etc. As such, the queue manager has to empirically estimate any additional overheads based on past experience, and the adjust the queue schedule accordingly on subsequent nights based on how long it takes the observers to execute the program in practice (e.g., using the times reported by the nightly data logs).
Telescope pointing, target acquisition, and guide-star acquisition/lock times are not known a priori, but in general, the official estimate is to allow 3 minutes per acquisition. This is a slight overestimate, but it works out in the final accounting, since it allows for greater or lesser degrees of difficulty that the observer will have pointing, focussing, setting guide stars, etc. This is the value the queue-scheduling team uses when working out the observing program for each night.
If your program requires a lot of additional operations, e.g., many offsets around the target position between observations, it will cost you in terms of total execution time. If your program proves to be excessively costly in additional overhead, the queue manager will contact you regarding how to modify your program to make it more efficient. Not surprisingly, difficult programs are also difficult to schedule and execute, and have higher overheads. Keeping it simple is a virtue.
If everything is satisfactory, you are then asked to give the obs file a name. Each project is assigned a unique working directory for its obs files, so there is little chance your files with collide with others, though care in choosing filenames is essential. Above all else, make filenames that are simple and descriptive.
By simple, we mean you must restrict yourself to letters and numbers; no ".", "_" or other special characters. Special characters (even those technically allowed by Unix) can cause problems with the data-taking system, and if your observation fails because it has an illegal filename syntax, the fault is yours not the systems!
Similarly, a filename should reflect as much as possible the contents of the file (without being so complicated as to be unusable). For example, if the obs file is to acquire simultaneous V and H band images of a star cluster named NGC007, you might name the obs file ngc007vh. Naming it "fred001" is not just perverse, it could potentially waste a lot of time, as who knows that "fred001" means "make V+H images of NGC007".
Remember that choosing simple, unique, descriptive names will help the on-site observers execute your program. If you make complicated names that are hard to type, it will slow down the process; please keep it simple (the filenames are ultimately for them, not you). The observing managers will ask observers to resubmit observation files with more meaningful names, or change names as required if they cause execution problems.
After selecting a name, save the final obs file to your project's working directory by hitting the "Save Obs File" button at the bottom of the form. The obs file is stored on disk where you can view it later with the Obs File Manager (which also provides tools for renaming and deleting files). You will also be shown a copy of the final, saved obs file on your browser screen. We recommend that you print out your browser screen with the final version for your records.
Safe Saving
To protect existing obs files for your project from accidental deletion, you are prevented from overwriting existing obs files with the form. If you try, the form will warn you and ask you to either (a) provide another, unique name and resubmit the form for processing, or (b) to go to the Obs File Manager and either delete or rename the existing file, and then resubmit the form again. Careful use of the "back" button on the browser lets you do this simply.
Making more than one obs file for a target
The multi-step process is designed to allow multiple iterations between any sets of forms, provided you take care to use the browser Back button and the various form buttons carefully. The target information (name and coordinates) are If you reload the form by following a link, bookmark, or other means, you will be given a blank form. By now simple web forms are familiar to most users, so this needs little detailed explanation.
Trouble? How to Get Help
No system is perfect. If you have problems using these forms please contact the SMARTS2 support personnel at Yale and describe your problem, the time it occurred, and any other info you think might help him debug things. The more feedback the better at this stage.
The following are descriptions of the entries in the obs file creation forms. These entries are accessible from within the forms themselves by clicking on the highlighted item. If you have come to this page from the web form, remember use the "Back" button on your browser to continue filling out the form in progress.
On logging into the Observing Preparation Tools pages, you need to provide your name and Project ID.
Your Name
To keep track of who created the obs files for a project, we ask you to enter your name in the box provided.
Project ID codes are assigned by the SMARTS scheduling committee when time is awarded on the SMARTS telescopes. Select your SMARTS Project ID from among the entries in the pull-down menu. If you don't know your ID number, or don't find it in the menu, contact the current queue manager or NOAO program coordinator (as appropriate) immediately.
The first form will ask you to enter the target name and coordinates, and the imaging mode to be used. Project PIs (or their CoIs) are responsible for entering the target name and coordinates correctly. Neither the queue manager nor the on-site observers will enter, validate or correct target names or coordinates. Although if there are problems with your coordinates, the queue manager will be in touch.
There are two types of observing template that can be created: single-target and multi-target.
If your obs file is to be used for one, specific target, you will be creating a "single-target obs file". In this case, check the "Single Target" box, and enter the Target Name and coordinates in the boxes provided, as follows:
Target Name
Enter the target name of the object you wish to observe. This is how the target name will appear in all observing logs and FITS image headers (the OBJECT keyword). The target name you enter in step 1 is carried forward through all subsequent obs file creation steps.
You can enter up target names up to 60 characters long (including spaces), but only the first 16 characters will appear in the observing logs (all 60 will appear in the image FITS headers).
Solar System Objects
If your target is a solar system object (i.e., a moving target), be sure to check the "Solar System Object" box. You will also need to provide both approximate coordinates for the object, as well as arranging to send the queue manager ephemerides for minor bodies (asteroids and moons) separately from this form.
Target RA, Dec, & Equinox
Enter the Right Ascension, Declination, and Equinox of the target. RA should be in hh:mm:ss.s format, and Declination in dd:mm:ss format. The sign of the declination goes in the first place, thus:
-00:00:32
+12:12:34
etc. are valid declinations. Please do not enter decimal coordinates.
The default equinox is J2000.0 coordinates, and we would prefer that you precess coordinates to J2000.0 before entering them here. If you cannot precess the coordinates, enter the Equinox in the box provided (e.g., 1950.0 for B1950.0 coordinates; omit the "J" or "B"). Use of non-2000 coordinates is greatly discouraged, as it could be overlooked by observers working through a long target list with 99% J2000 coordinates. Give them a break and precess them, please.
If your target is a solar system object, enter approximate coordinates for the observing season to assist in queue scheduling, and remember to check the "Solar System Object" box next to the Target Name. All of the planets are already in the 1.3m telescope's control system, but for minor planets or planetary moons you will have to provide the queue manager with an accurate ephemeris. Contact the queue manager [59] for instructions on how to submit ephemerides for solar system targets.
Note: There is apparently some confusion about the precise role of these coordinates in the data-taking process. They are not actually used by the data-taking system per-se (i.e., the data-taking system does not read the coordinates from the obs file and slew the telescope). Rather, they are there for two purposes: (1) to be used by the queue-management team as the "definitive" coordinates for your target, and (2) in cases of uncertainty at the telescope the observer will consult the obs file for a particular target to verify the coordinates against what is given on their nightly observing list. This sounds non-functional, but in fact it serves to "bind" the definitive coordinates to the observation template in an unambiguous fashion.
If your observing program requires multiple pointings within or around an object because it is larger than the ANDICAM field-of-view, the situation is more complicated. Such offset pointings must be treated as separate observations because the on-site observers must enter the new field coordinates by hand into the TCS, execute the telescope offset, and setup the autoguider separately for each subfield. None of these operations may be automated by way of obs files at the present time (and may not in fact be easy or possible in the future). There are a number of ways to go about doing this, so you will need to consult with ANDICAM core team members for recommendations as this is not a normal ANDICAM observing mode.
If you are creating a generic obs file to be used as a template for multiple targets that will share the same exposure times and filters, check this box to create a "multi-target obs file". No target name or coordinate info needs to be entered if this box is checked (and any entries you put into those boxes will be ignored by subsequent forms).
Multi-object observing template are most often used to take observations of many different targets in a "survey" style mode (see the Phase II Instructions [68] for a discussion). This is what you would use if you had a large list of objects that only need to be observed once (or only infrequently), but with different filter settings. A multi-observation script is then used to set the Target name separately, and you will be required to submit a separate coordinate list with your Phase II instructions.
Once you have selected single- or multiple-target mode, you must select the imaging mode for the observations. This is one of:
You may change the imaging mode used for a given template later by returning to Step 1 with the Back button on your browser. All of the stages in the form are designed to be as "re-entrant" as possible to make building sets of templates for the same object easier (no guarantees, it depends on which web browser you are using).
Having set the target parameters (single or multiple) and the base observing mode (CCD, IR, or Dual), the second form asks you to enter the CCD and/or IR imaging exposure parameters for your target for the imaging mode selected. This includes filter selection, and setting up the dithering parameters for IR imaging.
CCD Filter
Select a filter from the list provided. Only one CCD filter can be specified in a given obs file. To make a series of observations through more than one CCD filter, you need to create a separate obs file for each filter.
CCD Base Integration Time
Enter the integration time, in seconds, of a single CCD image. Integration times up to 1800s are allowed. You can integrate for longer than 1800s, but cosmic ray contamination becomes severe. There is no default integration time, and this field may not be left blank.
An integration time of 0 seconds will result in a "bias" or "zero" frame being acquired. If you do not wish to take CCD images with this obs file, back up to the target info form and select "IR-only Mode" as the Imaging Mode.
Number of CCD Images
Select the total number of CCD images to be acquired during this observation. Each CCD image will have the base integration time entered above. The total integration time will be the base CCD integration time multiplied by the number of CCD images. Default is 1 image. The total CCD integration time will be the number of CCD images times the base integration time.
NOTE: you cannot select 0 CCD images. If you do not wish to take CCD images with this obs file, back up to the target info form and select "IR-only Mode" as the Imaging Mode.
New to the 1.3m ANDICAM. The unbinned pixel scale at the CTIO 1.3m telescope is ~0.18 arcsec/pixel, necessitating that we bin the detector 2x2 pixels on-chip to get a more reasonable scale of ~0.37 arcsec/pixel.
As a consequence, CCD binning is no longer a user-selectable parameter at the 1.3m (this is a change from how we worked at the Yale 1-meter, and is not negotiable).
IR Filter
Select a filter from the list provided. Only one IR filter can be specified in a given obs file. To make a set of observations through more than one IR filter, you need to create a separate obs file for each filter.
IR Base Integration Time
Enter the integration time, in seconds, of a single IR array image. Times up to 1800s are allowed, but the background will typically saturate in a few minutes, especially at K. There is no default integration time, and this field may not be left blank.
The minimum IR detector integration time is 4 seconds. If you enter a base integration time between 0 and 4 seconds, you will get at 4 seconds of integration anyway. Above 4 seconds, the requested integration time will be achieved. See the ANDICAM manual for an explanation.
Number of IR Images
Select the total number of IR images to be acquired by this observation. Each IR image will have the base integration time entered above. Default is 1 image. The total effective IR integration time will be the number of IR images times the base integration time.
NOTE: You cannot select 0 IR images. If you do not wish to take IR images with this obs file, back up to the target info form and select "CCD-only Mode" as the Imaging Mode.
Number of CoAdds per IR image
Each IR image can be composed of a number of separate images averaged together ("co-added") in the detector control computer before being stored as a single image file on disk. Each IR CoAdd will have the base integration time entered above. For example, if you specify 5 IR images of 3 co-adds each, the instrument will acquire 15 images of the base integration time, averaging them in groups of 3, and storing them as 5 separate FITS files. Default is 1 Co-add/image.
In general, co-adding is most useful when a target is sufficiently bright that you are restricted to very short integration times to avoid saturation, and so would need a very large number of single images to build up sufficient signal. Co-adding helps build up signal while producing a reasonable number of final image files, and with the additional benefit of a slightly reduced overhead penalty compared to taking a large number of single images. The cumulative readout noise penalty, however, is the same regardless.
An internal tip-tilt mirror in the IR channel beam can be used to make small "dithering" offsets between IR images. Dithering is the standard way to reduce the effects of bad pixels and flat-field artifacts on the IR array by shifting and combining multiple images taken at slightly offset positions on the array. No dithering is done between IR Co-Adds.
To dither between images, check the "Dither between images" box, and select scale the dithering pattern ("dither scale") from the pull-down menu. The default dither scale is 40, which corresponds to a dither throw of approximately 20 arcseconds on the CTIO 1.3m telescope. This is the dither scale used for generation of IR dome flats, so this makes the most sense to use this for most observations. Dither scales range from 10 to 100 in steps of 10 (5-50 arcsec in steps of 5 arcsec). If you want to use another dither scale, you may need to arrange for additional flat-field calibration (at a cost to your time allocation).
The IR tip/tilt mirror dithers the image around the IR detector in a fixed hexagonal offset pattern. There are 7 dither positions: the first (1) centered on the array, and the following 6 (2-7) arranged in a lop-sided hexagon, stepped in (roughly) 120-degrees segments. The hexagon is lopsided due to the 45-degree difference between the tip/tilt actuator plane and the surface of the diagonal pickoff mirror. This pattern is repeated (modulo 7) until the total number of IR Images requested have been acquired. At the end of a dithering sequence, the mirror is returned to the home (centered) position. Tests at the telescope show that the dithering is repeatable to ~0.5 pixel (0.07 arcsec on this IR array).
If you do not wish to dither between images, check the "No Dithering between images" box. This will keep the IR tip/tilt mirror centered during the entire obs file's IR imaging sequence.
Once the exposure parameters have been entered in step 2, the obs file creation form generates the obs file and estimates the execution times for the CCD and/or IR images requested. You are asked to first validate your entries, using the estimated execution times to help adjust your exposure parameters to optimize your observations, and then select a filename for the obs file and save it to your project's working disk.
IMPORTANT NOTE:
Filenames must be kept "simple": only letters (a-z & A-Z) and numbers (0-9) are allowed. All other characters are forbidden (i.e., it cannot contain any of the following:
"'()[]{}-+_=.,:;|\/?><~!@#$%^&*
even though a few of these are are technically allowed by Unix!). Please remember that the observer has to type the name, sometimes many times, so think of them when you make up filenames. Difficult filenames can lead to errors and slow down observing, and will be changed by the queue management team without asking you.
The estimated execution times give the approximate amount of real time required to execute the requested exposures, from the first detector array reset until the end of the last detector readout (not including any instrument or telescope configuration overheads). The various data-acquisition overheads were measured during engineering runs in January/February 2003 with the new ANDICAM setup, and yield estimates based on our CCD and IR Array readout models that are accurate to within 5%. Be warned, your mileage *will* vary, so don't expend too much effort time optimizing out the last second of dead time in dual-channel observations - reality *will* have the last word. For those interested in factoring in instrument configuration overheads, at most this amounts to 10-seconds per observing template (assming change of name, filter, exposure time, etc.). Telescope pointing, target acquition, and guide-star acquisition/lock times are totally up for grabs. If your program requires a lot of hand offsets around the field, it will cost total observation execution time. If your program proves excessively costly in overhead, the queue manager will contact you regarding modification of your program.
This estimate takes into account:
1. The base integration time per CCD image.
2. The number of CCD images requested.
3. The time required to readout the CCD (vertical and horizontal clocking times and the readout amp integration time per pixel).
4. The number of readout amplifiers being used (2 at present, not user-selectable).
5. The pre-exposure "setup" overhead, including array erase cycles (~6-sec independent of binning).
For example, a single, full-frame, 2x2 binned 1024x1024 CCD image requires approximately 47 seconds over and above the base integration time to erase and readout the array. Future operation with 2-amplifier readout should reduce this to 20-odd seconds.
Taking many short exposures incurs a greater readout "penalty" compared to taking fewer longer exposures to achieve the same total integration time. For example, a single 300 second full-frame, unbinned image will require approximately 347 seconds to execute, while dividing the 300 seconds of integration time into two (2) exposures of 150 seconds each requires 394 seconds (~14% more time). Doing three exposures of 100 seconds each would require ~441 seconds to execute (27% more time).
This estimate takes into account the following:
1. The base integration time per IR image (the minimum integration time is 4 seconds).
2. The number of IR images requested.
3. The number frames co-added per IR image requested.
4. IR setup, readout, and post-processing (pre-read minus post-read math) overheads amounting to about 20 seconds.
5. The tip/tilt mirror overhead if dithering between images (approx. 2 seconds/position).
The algorithm for computing the execution time of IR images is complicated by execution latencies encountered during readout and storage due to the finite clock interval allowed in the hardware. In general, the times computed are good to 5%, although if a large number of images (>10) has been requested with a comparable number of co-adds per image, the calculator will systematically underestimate the total execution time by as much as 10% due to cumulative small latencies in the system.
Each ANDICAM project is assigned a private directory on the queue server for storing their observation template files.
This field asks you to provide a filename for your new obs file. The filenames of obs files should be kept simple (i.e., only letters and number: NO SPECIAL CHARACTERS), and should reflect as much as possible the contents of the file. For example, if the obs file is to acquire simultaneous V and H band images of a star cluster named NGC007, you might name the obs file ngc007vh. Including the object name in the filename like this helps to ensure relatively unique names, and makes it easy to know what file is doing what by just looking at the name. You only have to look at a few of these files, the operations staff has to handle hundreds! Give us a break, please!
Filenames are case sensitive, and may contain only letters and numbers, NO SPECIAL CHARACTERS (e.g., +, -, _, etc.) ARE ALLOWED (even though technically Unix might allow quite complex filenames). Please remember that the observers have to type them, sometimes many times a night, so complex or confusing filenames can cause problems, and will be changed to simpler names if they are crazy.
If the filename you provide will overwrite an existing obs file in your directory, you will be given a warning and asked to confirm that you really want to overwrite the existing file. Detailed instructions are provided if this occurs.
Note that the obs files will be given the .obs files extension automatically by the web forms, so do not include a file extension with the filename you type in the box provided.
Once you have a set of Obs files created, you can later go back and edit them with the Obs File Editor. This form will read in the contents of a existing Obs file and let you modify the entries, either to replace an old Obs file or to create a new Obs file using an old one as a template. In cases where readout or overhead times change substantially (e.g., in September 2000), the editor can be used to re-evaluate old Obs files and modify them to reduce deadtime in DUAL mode.
The basic entries are the same as on the Obs file creation form described above. The one potential point of confusion is if you are editing an Obs file that was originally either CCD-only or IR-only imaging mode. In these cases, the editor form provides boxes for the unused channel (after entries for the active channel). These entries will be ignored unless you decide to change the imaging mode as part of your editing session. It's easier to try than read about, trust me, you'll figure it out.
After a while, you can get quite a collection of Obs files. To provide a way to manage these semi-sensibly, we have provided the Obs File Manager Form [64]. The file manager is a table-based web form that shows you all of the obs files that have been created for your project, and lets you view, delete, or rename individual files. This lets you clean up after making your obs files, fix ugly filenames, etc., without having to go back through the creation or editor forms.
Obs files "deleted" from the active list are moved to the wastebasket for your project, where they are held until you decide to either delete them once and for all, or to "undelete" them and return them to the active list. If there are any files in your project's wastebasket when you open up the file manager, they will appear in a separate "wastebasket table" beneath the table of active files. This is a safety feature to prevent you from accidentally deleting obs files (you can delete them, we just make you think about it first).
Editing existing obs files is not an option during the early parts of the testing phases (the file parser is not working yet), but we hope to have something working eventually.
The instructions for using the File Manager are described in a separate document [64].
This is an obs file to take one 300-second CCD image of MB99018 with the I-band filter. The IR channel is kept idle during the observation (CCD-only mode).
# Prospero Observation Template File
# Created: 2003 Feb 9 [13:35:50] by saveobs.pl Version 1.5
# For: R. Pogge
#
PROJECT=OS03001
IMGTYPE=OBJECT
OBJECT=MB99018
RA=18:01:07.7
DEC=-28:31:41
EQUINOX=2000.0
MODE=CCD
#
# CCD Imaging Parameters
#
# Estimated Execution Time: 347 sec
#
CCD:
FILTER=0 # I
EXPTIME=300.0
NIMGS=1
END
This obs file takes a sequence of five (5) 60-second images at K of a Seyfert 1 galaxy, dithering between images with a dither scale of 20 units (about 10 arcsec). The CCD channel is kept idle during this observation (IR-only mode).
# Prospero Observation Template File
# Created: 2003 Feb 7 [13:27:45] by saveobs.pl Version 1.5
# For: Rick Pogge (OSU)
#
PROJECT=OS03011
IMGTYPE=OBJECT
OBJECT=Mrk 1347 K
RA=12:39:47.3
DEC=-23:27:16.0
EQUINOX=2000.0
MODE=IR
#
# IR Imaging Parameters
#
# Estimated Execution Time: 410 sec
#
IR:
FILTER=3 # K
EXPTIME=60.0
NCOADDS=1
NIMGS=5
DITHER=T
DSCALE=20
END
This obs file takes simultaneous V and K-band images of 47 Tucanae, one 180-sec integration at V and three 60-sec integrations at K, dithering by a factor of 40 between IR images.
# Prospero Observation Template File
# Created: 2003 Feb 7 [13:41:59] by saveobs.pl Version 1.5
# For: bailyn
#
PROJECT=YA03001
IMGTYPE=OBJECT
OBJECT=47 tuc
RA=00:26:00
DEC=07:02:22
EQUINOX=2000.0
MODE=DUAL
#
# CCD Imaging Parameters
#
# Estimated Execution Time: 227 sec
#
CCD:
FILTER=6 # V
EXPTIME=180.0
NIMGS=1
#
# IR Imaging Parameters
#
# Estimated Execution Time: 246 sec
#
IR:
FILTER=3 # K
EXPTIME=60.0
NCOADDS=1
NIMGS=3
DITHER=T
DSCALE=40
END
Note that there is approximately 19 seconds of "deadtime" between the IR and CCD images. Attempting to optimize the difference by more than 10-20 seconds, however, is usually a waste as this time can easily be consumed by various system latencies that are unpredictable (some dual-channel operations must execute serially instead of in parallel).
This is a multi-target obs file used to take simultaneous V and H-band images. No target name or coordinates are given because it is to be used on a number of different targets generically. Here, we take one 180-sec integration at V and three 60-sec integrations at H, dithering by 50 units between the successive IR images.
# Prospero Observation Template File
# Created: 2003 Mar 2 [14:21:34] by saveobs.pl Version 2.0
# For: pogge
#
PROJECT=OSU-TOO
IMGTYPE=OBJECT
MODE=DUAL
#
# CCD Imaging Parameters
#
# Estimated Execution Time: 227 sec
#
CCD:
FILTER=6 # V
EXPTIME=180.0
NIMGS=1
#
# IR Imaging Parameters
#
# Estimated Execution Time: 246 sec
#
IR:
FILTER=2 # H
EXPTIME=60.0
NCOADDS=1
NIMGS=3
DITHER=T
DSCALE=50
END
Note that unlike all of the other example obs files shown thus far, there are no OBJECT=, RA=, DEC=, or EQUINOX= entries. This makes the obs file "generic" in the sense that it can be used for any target. Such a generic obs file can only be executed by an accompanying multi-observation script that will prompt for the target name, and run any other multi-target obs files that are part of a sequence to be executed for each target in the program. Executing it without such a script will result in either a blank object name (bad), or with the object name of the last target observed (worse). See the Phase II Instructions for details.
If you came here from one of the entry forms, use the "BACK" button on your browser to return to the obs file generation form in progress.
Updated: 2006 May 11 [rwp/osu]
Contents: | |
1. | Overview |
2. | The Entry Page |
3. | File Manager Table Entries |
4. | Wastebasket Table Entries |
SMARTS Consortium
CTIO 1.3m Telescope ANDICAM Observation Template File Manager Instructions
Once you have created a set of Observation Template files ("obs files" for your program, you can delete or rename them using the Observation Template File Manager Form. This form shows you a table with all of the obs files that have been created for your project, and lets you view, delete, or rename individual files. This lets you clean up after making your obs files, fix ugly filenames, etc., without having to go back through the creation step.
Obs files "deleted" from the active list are moved to the wastebasket for your project, where they are held until you decide to either delete them once and for all or to "undelete" them and return them to the active list. If there are any files in our project's wastebasket, they will appear in a separate "wastebasket table" beneath the table of active files in the file manager form. This is a safety feature to prevent you from accidentally deleting obs files.
Each time the "Delete/Rename Marked Files" button is pressed, the file manager tables are regenerated, and a synopsis of any actions taken is printed. If there were errors, they appear in red below the buttons.
This page describes the Obs File Manager form and its contents.
Entrance into the File Manager is via a page with simple pull-down menu with the current list of approved ANDICAM projects. Select your project ID from among the entries in the pull-down menu, and click on the "Next>" button to see the obs files for that project. If you don't know your ID number, or don't find it, contact the current queue manager.
Project ID codes are assigned by the SMARTS scheduling committee when time is awarded with ANDICAM on the CTIO 1.3m telescope. Obs files are sorted by SMARTS Project ID Numbers. If there are no obs files in your project's working directory, you will be told this, otherwise, you will be shown a table of the obs files for your project.
At this time, it has not yet been decided whether or not the PI directories will be protected by passords assigned by the queue management team. This will mean that only Project PIs (and the queue management team) can use the web forms to view or manipulate a project's files. For now, the vagueries of web "security" being as they are, no protection works better than any protection at all. (Failure to grant access to PIs is not an option).
The following are brief descriptions of the entries in the Obs File Manager Table. These descriptions are also accessible by from within the form by clicking on the highlighted item.
If you have come to this page from the manager form, remember use the "Back" button on your browser to return to the form from whence you came.
Obs File (Column 1)
The names of all active obs files found in your project's working directory are shown in this column. Only the files for your project are shown.
To view the contents of an obs file, click on the highlighted filename. You can also save it to your local disk using "Shift+Click".
If you click on this radio button, you will mark the obs file for deletion. Once you have marked all of the files you wish to delete, you can press the "Delete/Rename Marked Files" button to delete them.
The "deleted" file is moved to the wastebasket, where it is held until it is either (a) expunged (deleted forever) either individually or by emptying the wastebasket, or (b) it is undeleted and restored to the active obs file list.
If you click on this radio button, you will mark the obs file for renaming. You will need to enter new name for the file in the New Name box in Column 4.
Note that deletion and renaming are mutually exclusive (they are both "radio buttons").
New Name Box (Column 4)
If you are Renaming an obs file, enter the new filename in this box. New files names follow the same rules for old files names, and names up to 16 characters long are allowed. There is no need to type the ".obs" extension, that will be added by the file manager automatically.
Once you have marked all of the files you wish to rename, you can press the "Delete/Rename Marked Files" button to rename them.
Warning! The file manager form will not let you rename a file so as to overwrite an existing file. However, if the new name is that of a file that you are also Deleting with the manager in this session, file deletion operation is done before renaming, so there should be no problem.
Files that are "deleted" from the active obs file list are moved to a "Wastebasket". This allows you to undelete a file later if you decide it shouldn't have been marked for deletion, or to delete it forever by "expunging" it from the wastebasket, at which point it will be physically deleted from the disk. These descriptions are also accessible by from within the Wastebasket table form by clicking on the highlighted items.
If you have come to this page from the manager form, remember use the "Back" button on your browser to return to the form from whence you came.
Trash File (Column 1)
The names of defunct obs files found in your project wastebasket are listed in this column. Only the files for your project are shown.
To view the contents of an obs file in the wastebasket, click on the highlighted filename. You can also save it to your local disk using "Shift+Click".
If you click on this radio button, you will mark the file for expunging from the wastebasket. "Expunging" a file from the wastebasket means it is deleted from the system and gone forever.
If you click on this radio button, you will mark the defunct obs file in the wastebasket for un-deletion. This means it will be restored to the list of "active" obs files, and available for implementation.
Note that expunging and un-deletion are mutually exclusive (they are both "radio buttons").
Undelete To box(Column 4)
If you are Undeleting a file in the wastebasket, you can give it a new name at the same time. By default, if this box is left empty, the file will recover its original name when undeleted. If this might overwrite an existing file with the same name, you can give it a new name.
Warning! The file manager form will not let you undelete a file so as to overwrite an existing file. However, if the new name is that of a file that you are also Deleting from the active list in this session, file deletion operation is done before undeletion, so there should be no problem.
By checking the Empty Wastebasket check box at the top of the Wastebasket table, you will mark all files in the wastebasket for final, irretrievable deletion. Any files marked with to undelete below will be ignored.
Note: Emptying the wastebasket is final, there are no recovery options once it is empty!
If you came here from one of the entry forms, use the "BACK" button on your browser to return to the obs file manager form in progress.
Updated: 2003 January 29 [rwp/osu]
ANDICAM Phase II Observing Preparation Tools [66]
ANDICAM Instrument & Detector Characteristics [3] [OSU]
ANDICAM Filters [70]
ANDICAM Data Products [2]
SMARTS2 and ANDICAM Contact Information [67]
ANDICAM Email Lists [20]
SMARTS2 Consortium [49]
1.3m Telescope [40]
ANDICAM [57] home
Yale University's 1.0 meter telescope was automated by the Astronomical Research Institute (ARI https://www.astro-research.org/ [71]). It is operated with NASA funding to recover and follow-up NEOs.
The CTIO/Yale 1-meter telescope is an f/10 reflecting telescope with a closed tube Cassegrain design. It is controlled using a custom Comsoft PC-TCS/DCS system which includes full automation of the dome. A CTIO-built autoguider (with a fixed-position CCD guide camera) was installed in early 2004. From June 1998 until September 2002, the 1.0-m was used by the YALO consortium with the OSU-built ANDICAM [57] dual optical/IR imager. When the ANDICAM [57] was moved to the CTIO 1.3-m [72] as part of the SMARTS collaboration startup in 2003, the 1.0-m sat idle until a new 12-position filter wheel and CCD was installed by OSU in March 2003.
From July 2005 until the present, the 1.0-m has been equipped with the dedicated STA 4064x4064 CCD known as Y4KCam [73]. Prior to July 2005, the 1.0-m was equipped with a 512x512 Apogee AP7 CCD [74] . The 1.0-m is equipped with a 12 position filter wheel using 4"x4" filters. Available filters include BVRcIc (standard CTIO/KPNO Kron-Cousins set), SDSS ugriz, and U+CuSO4. The complete suite of filters available is listed here [75].
For more information, please see the 1.0m website [76].
Y4KCam is a 4Kx4K optical CCD optimized for wide-field broad-band imaging. It has a 12-position filter wheel and uses a corrector lens (doubling as the dewar window) that provides a nearly undistorted 20x20-arcminute field of view for UBVRI imaging. The CCD has excellent blue sensitivity, especially at U-band.
Detector Parameters | |
Pixels | 4064x4064 |
Pixel Scale | 0.289"/pixel |
Field Size | 20'x20' |
The CCD is operated using multiple amplifier readout (quad). There is no region-of-interest capability.
Conversion Gain | : 1.38 electrons/DN | |
Readout Noise | : 6.6 electrons (rms) per quadrant | |
Linearity | : <1% linear to 42,000 ADU above bias | |
Full Well | : ~66,000 electrons | |
Acquisition Overheads: | ||
1x1 binning | : 51 sec | |
2x2 binning | : 16 sec | |
4x4 binning | : <5 sec |
Additional CCD characteristics can be found at the Ohio State Y4KCam Detector page [78].
Gain and Readout noise measurements by quadrant (2010 April 28) are
(1,1) +------+------+ | | | | Q1 | Q2 | | | | +------+------+ | | | | Q3 | Q4 | | | | +------+------+ Q1: g=1.33 e-/ADU ron=7.12 e- Q2: g=1.33 e-/ADU ron=6.91 e- Q3: g=1.43 e-/ADU ron=6.01 e- Q4: g=1.45 e-/ADU ron=6.53 e-
These gain numbers are consistent with the last measurement in August 2007, but the measurement of the readout noise is improved (better method not a better CCD!). This number is inline with expectations for the STA0500 detector.
The CCD conversion gain and readout noise are measured using Janesick's Photon Transfer method, using pairs of biases and a sequence of pairs of flat-field images taken with 1 to 300 second exposures running from low level to at or near saturation.
The gain and readout noise vary from quadrant-to-quadrant, as expected for 4 independent readout amplifiers, ranging from 1.33 to 1.45 e-/ADU. The nominal 1.4 e-/ADU quoted above represents a round average of the 4 quadrants that should be useful for exposure time estimates based on predicted photon fluxes at the detector.
Prior to 2007 February, readout noise was dominated by a 60Hz pickup noise which resulted in an effective readout noise of ~15 electrons per quadrant. This noise source was eliminated by identifying and electrically isolating the offending component, in this case the camera power supply leaking dirty power from the telescope. Now bias images are much cleaner and yield a high-quality 2D bias frame from a median of 5-10 zero images. Recent measurements put the readout noise at about 6.6 electrons.
Examination of overexposed star images (saturated but not pushed past full-well and "bleeding") on raw images shows that the nominal full-well saturation occurs at about 50000ADU, or about 44000ADU above bias, corresponding to about 66,000 electrons full-well depth for a nominal gain of 1.4 e-/ADU.
Tests during February 2007 show that the shading correction function has been stable on a few-year timescale. We recommend that a set of shading correction data be taken only once per semester and stored on the data-taking computer at the 1-meter as well as in the Yale respository.
Data were taken during February 2011 to calculate correction coefficients. Those coefficients and brief instructions on the correction methodology can be found here [88].
Please refer to the Prospero Observer's Guide for the Y4KCam [89] for a complete discussion of data acquisition procedures. For previous users of Y4KCam, this Quick Guide [90] may be helpful as a refresher.
There is a nice package of IRAF-based scripts written by Phil Massey for the Y4KCam that can be found at his website [91]. In addition, IRAF's QUADPROC can also be used if a keyword file is added to the header. This file (binning 1x1 [92] or 2x2 [93]) can be added to the fits headers using IRAF script noao.artdata.mkheader. Please note that, to do standardized photometry with Y4KCam, it is necessary to take sky flats to get the full FOV sufficiently flat (see Phil Massey's note [94] on the subject).
SMARTS Nightly Observing Logs
1.5-m | 1.3-m | 1.0-m | 0.9-m | |
2011 | 1.3-m Logs 2011 [95] | 1.0-m Logs 2011 | ||
2010 | --- | 1.3-m Logs 2010 [96] | 1.0-m Logs 2010 | |
--- | ||||
2009 | --- | 1.3-m Logs 2009 [97] | 1.0-m Logs 2009 | |
--- | ||||
2008 | --- | 1.3-m Logs 2008 [98] | 1.0-m Logs 2008 | |
--- | ||||
2007 | --- | 1.3-m Logs 2007 [99] | 1.0-m Logs 2007 | |
--- | ||||
2006 | --- | 1.3-m Logs 2006 [100] | 1.0-m Logs 2006 | |
1.5-m Logs 2006A [101] | ||||
2005 | 1.5-m Logs 2005B [102] | 1.3-m Logs 2005 [103] | 1.0-m Logs 2005 | |
1.5-m Logs 2005A [104] | ||||
2004 | 1.5-m Logs 2004B [105] | 1.3-m Logs 2004 [106] | 1.0-m Logs 2004 [107] | |
1.5-m Logs 2004A [108] | ||||
2003 | 1.5-m Logs 2003B [109] | 1.3-m Logs 2003 [110] | ||
--- |
The creation of official nightly logs on the 1.5m did not begin until mid-November, 2003. Logs prior to this point can be found here [111]. Also, logs for dates after May 9, 2006 can be found in the same place.
ANDICAM began SMARTS operations on the CTIO 1.3m telescope on 2003 Feb 3.
ANDICAM nightly observing logs contain a list of all images acquired during a given night. Observing logs are filed by the local date at the start of the observing night. For example, to find the observing logs for the night that began the evening of 2003 June 12 and ended at sunrise on June 13, you would consult the observing log dated 2003 June 12 (20030612.log).
SMARTS2 operations began in January 2006. ANDICAM operations at the CTIO 1.3m telescope began as part of the original SMARTS consortium on 2003 February 3 and ran through 2005 December.
Observing logs are generated automatically by the AutoLog program running as part of the data-taking system and are updated automatically at 10am Eastern Time.
Observing logs are organized by month. Within each month the logs are filed by "Observing Date", which is defined as the local date at the start of the observing night. For example, to see what was observed during the night that began at sunset on 2010 June 12 and ended at sunrise on June 13, you would look at the log for 2010 June 12.
Logs are updated automatically at 10am Eastern Time.
CTIO 1.0m operations did not begin until 2004 May 12.
This is the book page to refer to old pages containing plate logs per month.
1969 Plate logs for 1.5-m Telescope
January 1969 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time |
Emulsion | Filtro | Seeing | Observer | Date | Object | Re- marks |
CTIO |
17 | 05 09 42 | - 68 49 | 15 m | lla - O | GG 385 | 2" | B . Bok | 31 01 69 | NGC 1854 | |||
18 | 05 09 42 | - 68 49 | 30 m | lla - O | UG 2 | 2" | B . Bok | 31 01 69 | NGC 1854 | |||
19 | 05 09 42 | - 68 49 | 30 m | 103a - D | GG 495 | 2" | B . Bok | 31 01 69 | NGC 1854 | |||
20 | 05 40 00 | - 69 04 | 45 m | 103a - E | R G 610 | 2" | B . Bok | 31 01 69 | 30 Dor. | |||
21 | 11 39 05 | - 61 54 | 15 m | lla - O | GG 385 | 2" | B . Bok | 31 01 69 | HD 101545 | |||
22 | 11 39 05 | - 61 54 | 45 m | lla - O | UG 2 | 2" | B . Bok | 31 01 69 | HD 101545 | |||
23 | 11 39 05 | - 61 54 | 45 m | 103a - D | GG 495 | 4.5" | B . Bok | 31 01 69 | HD 101545 |
Last Updated on 8/27/99
By Guerra & Marin
February 1969 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp.Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
24 | 05 07 44 | - 69 05.7 | 10 m | 103a - D | GG 495 | 2" | B . Bok | 01 02 69 | Sec Tifft | |||
25a | 05 07 44 | - 69 05.7 | 07 m | lla - O | GG 385 | 2" | B . Bok | 01 02 69 | Sec Tifft | |||
25b | 05 07 44 | - 69 05.7 | 45 m | lla - O | UG 2 | 2.5" | B . Bok | 01 02 69 | Sec Tifft | |||
26 | 05 22 28 | - 68 00.3 | 10 m | 103a - D | GG 495 | 2.5" | B . Bok | 01 02 69 | NGC 1927 | Broken Ok" ? | CTIO | |
27a | 05 22 28 | - 68 00.3 | ? | lla - O | UG 2 | 2.5" | B . Bok | 01 02 69 | NGC 1927 | |||
27b | 05 22 28 | - 68 00.3 | 07 m | lla - O | GG 385 | 1.5 | B . Bok | 01 02 69 | NGC 1927 | Broken Ok" | CTIO | |
28 | 10 18 54 | - 56 03.4 | 10 m | 103a - D | GG 495 | 3" | B . Bok | 01 02 69 | ? | |||
29a | 10 18 54 | - 56 03.4 | 07 m | lla - O | GG 385 | 3" | B . Bok | 01 02 69 | ? | |||
29b | 10 18 54 | - 56 03.4 | 45 m | lla - O | UG 2 | 3" | B . Bok | 01 02 69 | ? | |||
30 | 11 36 33 | - 63 12.4 | 10 m | 103a - D | GG 495 | 3" | B . Bok | 01 02 69 | IC 2944 | |||
31a | 11 36 33 | - 63 12.4 | 07 m | lla - O | GG 385 | 2.5" | B . Bok | 01 02 69 | IC 2944 | |||
31b | 11 36 33 | - 63 12.4 | 40 m | lla - O | UG 2 | 2" | B . Bok | 01 02 69 | IC 2944 |
Last Updated on 8/27/99
By Guerra & Marin
April 1969 Plate logs for 1.5-m telescope
Plate | N.N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
32 | 16 52 15 | -42 52 | 01 m | lla - O | - | Every Body | 29 04 69 | NGC 6231 | focus plate |
Last Updated on 8/27/99
By Jorge Marin
June 1969 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
89 | 17 23 06 | - 48 27 | 01 m | 103a - O | GG 385 | Hartwick | 09 06 69 | NGC 6352 | focus plate | |||
90 | 12 22 30 | - 72 31 | 15 m | 103a - O | GG 385 | Hartwick | 09 06 69 | NGC 4372 | ||||
91 | 12 20 31 | - 72 31 | 01 m | 103a - D | GG 495 | Hartwick | 09 06 69 | NGC 4372 | focus plate | |||
92 | 12 20 31 | - 72 31 | 45 m | 103a - D | GG 495 | Hartwick | 09 06 69 | NGC 4372 | ||||
93 | 12 20 30 | - 72 31 | 30 m | 103a - D | GG 495 | Hartwick | 09 06 69 | NGC 4372 | ||||
94 | 12 20 30 | - 72 31 | 30 m | 103a - O | GG 385 | Hartwick | 09 06 69 | NGC 4372 | ||||
95 | 17 21 48 | - 17 49 | 60 m | 103a - O | GG 385 | Hartwick | 09 06 69 | NGC 6356 | Broken Ok" | |||
96 | 17 21 48 | - 17 49 | 60 m | 103a - D | GG 495 | Hartwick | 09 06 69 | NGC 6356 | ||||
97 | 17 21 30 | - 48 25 | 15 m | 103a - D | GG 495 | Hartwick | 09 06 69 | NGC 6352 | ||||
98 | 17 21 30 | - 48 25 | 15 m | 103a - D | GG 495 | Hartwick | 09 06 69 | NGC 6352 | ||||
99 | 17 21 30 | - 48 25 | 15 m | 103a - O | GG 385 | Hartwick | 09 06 69 | NGC 6352 | ||||
100 | 17 21 30 | - 48 25 | 15 m | 103a - O | GG 385 | Hartwick | 09 06 69 | NGC 6352 | ||||
101 | 12 23 00 | - 72 24 | 103a - O | GG 385 | Hartwick | 15 06 69 | NGC 4372 | focus plate | CTIO | |||
102 | 12 23 00 | - 72 24 | 103a - O | GG 385 | Hartwick | 15 06 69 | NGC 4372 | focus plate | ||||
103 | 12 23 00 | - 72 24 | 15 m | 103a - O | GG 385 | Hartwick | 15 06 69 | NGC 4372 | ||||
104 | 12 23 00 | - 72 24 | 15 m | 103a - D | GG 495 | Hartwick | 15 06 69 | NGC 4372 | ||||
105 | 17 20 00 | - 17 46 | 30 m | 103a - D | GG 495 | Hartwick | 15 06 69 | NGC 6356 | ||||
106 | 17 20 00 | - 17 46 | 30 m | 103a - O | GG 385 | Hartwick | 15 06 69 | NGC 6356 | ||||
107 | 17 21 36 | - 48 26 | 30 m | 103a - O | GG 385 | Hartwick | 15 06 69 | NGC 6352 | ||||
108 | 17 21 36 | - 48 26 | 30 m | 103a - D | GG 495 | Hartwick | 15 06 69 | NGC 6352 | ||||
109 | 17 21 36 | - 48 26 | 15 m | 103a - D | GG 495 | Hartwick | 15 06 69 | NGC 6352 | ||||
110 | 17 21 36 | - 48 26 | 30 m | 103a - D | GG 495 | Hartwick | 15 06 69 | NGC 6352 | focus plate | CTIO | ||
111 | 17 21 36 | - 48 26 | 30 m | 103a - D | GG 495 | Hartwick | 15 06 69 | NGC 6352 | ||||
112 | 17 21 36 | - 48 26 | 15 m | 103a - D | GG 495 | Hartwick | 15 06 69 | NGC 6352 | ||||
113 | 17 21 36 | - 48 26 | 15 m | 103a - O | GG 385 | Hartwick | 15 06 69 | NGC 6352 | ||||
114 | 17 21 36 | - 48 26 | 15 m | 103a - O | GG 385 | Hartwick | 15 06 69 | NGC 6352 | ||||
115 | 17 21 36 | - 48 26 | 15 m | 103a - D | GG 495 | Hartwick | 15 06 69 | NGC 6352 | ||||
116 | 12 23 00 | - 72 24 | 60 seg | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 4372 | focus plate | CTIO | ||
117 | 12 23 00 | - 72 24 | 60 seg | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 4372 | focus plate | CTIO | ||
118 | 12 23 00 | - 72 24 | 30 seg | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 4372 | focus plate | CTIO | ||
119 | 12 23 00 | - 72 24 | 30 m | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 4372 | ||||
120 | 18 00 00 | - 30 02 | 30 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6522 | Broken Ok" | CTIO | ||
121 | 18 00 00 | - 30 02 | 30 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6522 | CTIO | |||
122 | 17 20 00 | - 17 46 | 30 m | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 6356 | ||||
123 | 17 21 00 | - 48 26 | 01 m | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 6352 | focus plate | |||
124 | 17 21 00 | - 48 26 | 30 m | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 6352 | ||||
125 | 18 00 00 | - 30 02 | 30 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6522 | CTIO | |||
126 | 18 00 00 | - 30 02 | 30 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6522 | CTIO | |||
127 | 17 21 00 | - 48 26 | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6352 | focus plate | CTIO | |||
128 | 17 21 00 | - 48 26 | 30 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6352 | ||||
129 | 17 46 48 | - 37 02 | 15 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6441 | ||||
130 | 17 46 48 | - 37 02 | 15 m | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 6441 | ||||
131 | 17 46 48 | - 37 02 | 05 m | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 6441 | ||||
132 | 17 46 48 | - 37 02 | 05 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6441 | ||||
133 | 18 00 00 | - 30 02 | 30 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6522 | Broken Ok" | CTIO | ||
134 | 18 00 00 | - 30 02 | 30 m | 103a - D | GG 495 | Hartwick | 16 06 69 | NGC 6522 | CTIO | |||
135 | 18 00 00 | - 30 02 | 25 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6522 | Broken Ok" | CTIO | ||
136 | 18 00 00 | - 30 02 | 30 m | 103a - O | GG 385 | Hartwick | 16 06 69 | NGC 6522 | Destroyed | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
August 1969 Plate logs for 1.5-m telescope
Plate | N.N. | R.A. | Dec | Exp Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
137 | 11 38 00 | -45 36 | 15 m | 103a - O | none | Mintz/Blanco | 16 08 69 | 1620 Geographos | ||||
138 | 11 38 00 | -45 37 | 15 m | 103a - O | none | Mintz/Blanco | 17 08 69 | 1620 Geographos | ||||
139 | 11 53 00 | -47 24 | 15 m | 103a - O | none | Mintz/Blanco | 18 08 69 | 1620 Geographos | ||||
140 | 11 53 00 | -47 24 | 15 m | 103a - O | none | Mintz/Blanco | 18 08 69 | 1620 Geographos | ||||
141 | 12 10 43 | -49 12.7 | 15 m | 103a - O | none | Mintz/Blanco | 19 08 69 | 1620 Geographos | ||||
142 | 12 10 43 | -49 12.7 | 15 m | 103a - O | none | Mintz/Blanco | 19 08 69 | 1620 Geographos | ||||
143 | 12 32 04 | -51 02.5 | 15 m | 103a - O | none | Mintz/Blanco | 20 08 69 | 1620 Geographos | ||||
144 | 12 32 04 | -51 02.5 | 15 m | 103a - O | none | Mintz/Blanco | 20 08 69 | 1620 Geographos | ||||
145 | 12 58 03 | -56 42.4 | 15 m | 103a - O | none | Mintz/Blanco | 21 08 69 | 1620 Geographos | ||||
146 | 12 58 03 | -56 42.4 | 15 m | 103a - O | none | Mintz/Blanco | 21 08 69 | 1620 Geographos | ||||
147 | 12 58 03 | -56 42.4 | 05 m | 103a - O | none | Mintz/Blanco | 21 08 69 | 1620 Geographos |
Last Updated on 8/27/99
Jorge Marin
September 1969 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp.Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
148 | 17 58 36 | - 25 00 | 35 m | 103a - O | UG 2 | Hiltner / Blanco | 04 09 69 | GX 5 - 1 | ||||
149 | 17 58 36 | - 25 00 | 117 m | 103a - O | UG 2 | Hiltner / Blanco | 06 09 69 | GX 5 - 1 | ||||
150 | 17 58 36 | - 25 00 | 20 m | 103a - E | GG 385 | Hiltner / Blanco | 06 09 69 | GX 5 - 1 | ||||
151 | 00 51 15 | - 26 56.3 | 20 m | lla - O | UG 2 | Hiltner / Blanco | 06 09 69 | NGC 288 | ||||
152 | 00 51 15 | - 26 56.3 | 10 m | 103a - D | GG 495 | Hiltner / Blanco | 06 09 69 | NGC 288 | ||||
153 | 00 51 15 | - 26 56.3 | 20 m | lla - O | UG 2 | Figueroa | 06 09 69 | NGC 288 | ||||
154 | 00 51 15 | - 26 56.3 | 10 m | 103a - D | GG 495 | 3" | Figueroa | 06 09 69 | NGC 288 | |||
155 | 00 13 30 | - 39 23 | 45 m | lla - O | none | Figueroa | 06 09 69 | NGC 55 | ||||
156 | 05 39 06 | - 69 09 | 45 m | lla - O | UG 2 | Figueroa | 06 09 69 | 30 Dor. |
Last Updated on 8/27/99
By Guerra & Marin
October 1969 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
157 | 01 01 23 | - 73 54 | 30 m | 103a - O | GG 385 | Landi | 07 10 69 | S M C RF | Broken Ok" | |||
158 | 01 01 23 | - 73 54 | 30 m | 103a - O | GG 385 | Landi | 07 10 69 | S M C RF | ||||
159 | 23 16 00 | - 72 00 | 30 m | 103a - O | GG 385 | Landi | 07 10 69 | Center Zona F1 | ||||
160 | 01 01 23 | - 73 54 | 30 m | 103a - O | GG 385 | Landi | 07 10 69 | S M C RF | ||||
161 | 01 01 23 | - 73 54 | 30 m | 103a - D | GG 495 | Landi | 07 10 69 | S M C RF | ||||
162 | 01 07 00 | - 73 02 | 30 m | 103a - D | GG 495 | Landi | 07 10 69 | SMC cum 419 | ||||
163 | 01 01 23 | - 73 54 | 30 m | 103a - D | GG 495 | Landi | 07 10 69 | S M C RF | ||||
164 | 01 01 23 | - 73 54 | 30 m | 103a - O | GG 385 | Landi | 07 10 69 | S M C RF | ||||
165 | 02 17 00 | - 70 40 | 30 m | 103a - O | GG 385 | Landi | 07 10 69 | Zona A II | ||||
166 | 01 01 23 | - 73 54 | 30 m | 103a - O | GG 385 | Landi | 07 10 69 | S M C RF | ||||
167 | 23 16 00 | - 72 00 | 30 m | 103a - O | GG 385 | Landi | 08 10 69 | Zona CF l | Broken Ok" | |||
168 | 01 01 23 | - 73 54 | 40 m | 103a - O | GG 385 | Landi | 08 10 69 | S M C RF | ||||
169 | 01 01 23 | - 73 54 | 40 m | 103a - D | GG 495 | Landi | 08 10 69 | S M C RF | ||||
170 | 23 16 00 | - 72 00 | 30 m | 103a - O | GG 385 | Landi | 08 10 69 | Zona CF l | ||||
171 | 01 01 23 | - 73 54 | 35 m | 103a - D | GG 495 | Landi | 08 10 69 | S M C RF | ||||
172 | 01 07 00 | - 73 02 | 35 m | 103a - O | GG 385 | Landi | 08 10 69 | SMC cum 419 | ||||
173 | 01 07 00 | - 73 02 | 25 m | 103a - O | GG 385 | Landi | 08 10 69 | SMC cum 419 | ||||
174 | 01 01 23 | - 73 54 | 25 m | 103a - O | GG 385 | Landi | 08 10 69 | S M C RF | ||||
175 | 01 01 23 | - 73 54 | 30 m | 103a - D | GG 495 | Landi | 08 10 69 | S M C RF | ||||
176 | 01 07 00 | - 73 02 | 30 m | 103a - D | GG 495 | Landi | 08 10 69 | SMC cum 419 | ||||
177 | 01 01 23 | - 73 54 | 25 m | 103a - O | GG 385 | Landi | 08 10 69 | S M C RF | ||||
178 | 17 59 42 | - 20 32 | 106 m | 103a - O | UG 2 | Landi | 10 10 69 | GX 9 + 1 | ||||
179 | 17 59 42 | - 20 32 | 10 m | 103a - D | GG 495 | Landi | 10 10 69 | GX 9 + 1 | ||||
180 | 17 59 48 | - 25 20 | 96 m | 103a - O | UG 2 | Landi | 11 10 69 | GX 5 - l | ||||
181 | 17 59 48 | - 25 20 | 10 m | 103a - D | GG 495 | Landi | 11 10 69 | GX 5 - l | ||||
182 | 01 01 23 | - 73 54 | 35 m | 103a - O | GG 385 | 3" | Landi | 11 10 69 | S M C RF | |||
183 | 01 07 00 | - 73 02 | 35 m | 103a - O | GG 385 | Landi | 11 10 69 | SMC cum 419 | ||||
184 | 01 07 00 | - 73 02 | 25 m | 103a - O | GG 385 | Landi | 11 10 69 | SMC cum 419 | ||||
185 | 01 01 23 | - 73 54 | 25 m | 103a - O | GG 385 | Landi | 11 10 69 | S M C RF | ||||
186 | 23 16 00 | - 72 00 | 30 m | 103a - O | GG 385 | Landi | 11 10 69 | Zona CF l | ||||
187 | 02 17 00 | - 70 40 | 30 m | 103a - O | GG 385 | Landi | 11 10 69 | Zona A II | ||||
188 | 01 01 23 | - 73 54 | 30 m | 103a - O | GG 385 | Landi | 11 10 69 | S M C RF | ||||
189 | 01 01 23 | - 73 54 | 35 m | 103a - O | GG 385 | 4" | Landi | 11 10 69 | S M C RF | |||
190 | 01 01 23 | - 73 54 | 35 m | 103a - O | GG 385 | Landi | 13 10 69 | S M C RF | ||||
191 | 23 16 00 | - 72 00 | 30 m | 103a - O | GG 385 | Landi | 13 10 69 | Zona CF l | ||||
192 | 01 01 23 | - 73 54 | 35 m | 103a - D | GG 495 | Landi | 13 10 69 | S M C RF | ||||
193 | 01 07 21 | - 73 02 | 35 m | 103a - D | GG 495 | Landi | 13 10 69 | SMC cum 419 | ||||
194 | 01 07 21 | - 73 02 | 40 m | 103a - O | UG 2 | Landi | 13 10 69 | SMC cum 419 | ||||
195 | 01 01 23 | - 73 54 | 40 m | 103a - O | UG 2 | Landi | 13 10 69 | S M C RF | ||||
196 | 01 01 23 | - 73 54 | 35 m | 103a - O | GG 385 | Landi | 13 10 69 | S M C RF | ||||
197 | 01 07 21 | - 73 02 | 35 m | 103a - O | GG 385 | Landi | 13 10 69 | SMC cum 419 | ||||
198 | 01 01 23 | - 73 54 | 35 m | 103a - O | GG 385 | Landi | 13 10 69 | S M C RF |
Last Updated on 8/27/99
By Guerra & Marin
November 1969 Plate logs for 1.5-m telescope.
Plate | N. N. | R. A. | Dec | Exp.Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
199 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | J. Graham | 02 11 69 | NGC 121 | ||||
200 | 01 49 06 | - 73 51 | 60 m | 103a - O | GG 385 | J. Graham | 02 11 69 | Lindsay 133 | ||||
201 | 03 44 36 | - 71 45 | 60 m | 103a - O | GG 385 | J. Graham | 02 11 69 | NGC 1466 | ||||
202 | 02 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | J. Graham | 02 11 69 | NGC 121 | ||||
203 | 02 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | J. Graham | 03 11 69 | NGC 121 | ||||
204 | 01 49 06 | - 73 51 | 60 m | 103a - O | GG 385 | J. Graham | 03 11 69 | Lindsay 133 | ||||
205 | 03 44 36 | - 71 45 | 60 m | 103a - O | GG 385 | J. Graham | 03 11 69 | NGC 1466 | ||||
206 | 02 25 42 | - 71 41 | 70 m | 103a - O | GG 385 | J. Graham | 03 11 69 | NGC 121 | ||||
207 | 01 49 06 | - 73 51 | 60 m | 103a - O | GG 385 | J. Graham | 03 11 69 | Lindsay 133 | ||||
208 | 03 44 36 | - 71 45 | 60 m | 103a - O | GG 385 | J. Graham | 03 11 69 | NGC 1466 | ||||
209 | 18 00 24 | - 30 02 | 30 m | lla - O | GG 385 | J. Hesser | 04 11 63 | NGC 6522 | CTIO | |||
210 | 20 52 30 | - 12 34.5 | 30 m | lla - O | GG 385 | J. Hesser | 04 11 63 | NGC 6994 | ||||
211 | 20 52 30 | - 12 34.5 | 30 m | 103a - D | GG 495 | J. Hesser | 04 11 63 | NGC 6994 | ||||
212 | 03 27 00 | - 53 00 | 100 m | 103a - D | GG 495 | J. Hesser | 04 11 63 | Klemola 8 | ||||
213 | 07 48 42 | - 38 17 | 30 m | 103a - D | GG 495 | J. Hesser | 04 11 63 | NGC 2447 | ||||
214 | 07 48 42 | - 38 17 | 30 m | lla - O | GG 385 | J. Hesser | 04 11 63 | NGC 2447 | ||||
215 | 07 48 42 | - 38 17 | 30 m | lla - O | GG 385 | J. Hesser | 04 11 63 | NGC 2447 | ||||
216 | 07 48 42 | - 38 17 | 30 m | 103a - D | GG 495 | J. Hesser | 04 11 63 | NGC 2447 | ||||
217 | 18 00 24 | - 30 02 | 45 m | 103a - O | GG 385 | J. Hesser | 05 11 63 | NGC 6522 | Broken Ok" | CTIO | ||
218 | 20 52 30 | - 12 34.5 | 30 m | 103a - O | GG 385 | J. Hesser | 05 11 63 | NGC 6994 | ||||
219 | 20 52 30 | - 12 34.5 | 16 m | 103a - D | GG 495 | J. Hesser | 05 11 63 | NGC 6994 | ||||
220 | 00 23 00 | - 72 00 | 15 m | 103a - D | GG 495 | J. Hesser | 05 11 63 | 47 Tuc | ||||
221 | 00 23 00 | - 72 00 | 15 m | lla - O | GG 385 | J. Hesser | 05 11 63 | 47 Tuc | ||||
222 | 00 23 00 | - 72 00 | 15 m | 103a - D | GG 495 | J. Hesser | 05 11 63 | 47 Tuc | ||||
223 | 00 23 00 | - 72 00 | 15 m | 103a - O | GG 385 | J. Hesser | 05 11 63 | 47 Tuc | Destroyed | |||
224 | 07 48 42 | - 38 17 | 30 m | 103a - O | GG 385 | J. Hesser | 05 11 63 | NGC 2447 | ||||
225 | 07 48 42 | - 38 17 | 30 m | 103a - O | GG 385 | J. Hesser | 05 11 63 | NGC 2447 | ||||
226 | 07 48 42 | - 38 17 | 30 m | 103a - D | GG 495 | J. Hesser | 05 11 63 | NGC 2447 | ||||
227 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | J. Graham | 07 11 69 | NGC 121 | ||||
228 | 01 49 06 | - 73 51 | 15 m | 103a - O | GG 385 | J. Graham | 07 11 69 | Lindsay 133 | ||||
229 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | J. Graham | 07 11 69 | NGC 121 | ||||
230 | 18 00 24 | - 30 02 | 30 m | 103a - O | GG 385 | J. Hesser | 09 11 69 | NGC 6522 | Destroyed | CTIO | ||
231 | 20 52 30 | - 12 34.5 | 30 m | 103a - O | GG 385 | J. Hesser | 09 11 69 | NGC 6994 | ||||
232 | 20 52 30 | - 12 34.5 | 30 m | 103a - D | GG 495 | J. Hesser | 09 11 69 | NGC 6994 | ||||
233 | 03 27 00 | - 53 00 | 90 m | 103a - O | GG 385 | J. Hesser | 09 11 69 | Klemola 8 | ||||
234 | 07 48 42 | - 38 17 | 60 m | 103a - O | GG 385 | J. Hesser | 09 11 69 | NGC 2447 | ||||
235 | 07 48 42 | - 38 17 | 60 m | 103a - D | GG 495 | J. Hesser | 09 11 69 | NGC 2447 | ||||
236 | 07 48 42 | - 38 17 | 10 m | 103a - O | GG 385 | J. Hesser | 09 11 69 | NGC 2447 | ||||
237 | 01 09 06 | - 32 19 | 45 m | 103a - O | GG 385 | M. Smith | 10 11 69 | Klemola 1 | ||||
238 | 01 09 06 | - 32 19 | 90 m | 103a - D | GG 495 | M. Smith | 10 11 69 | Klemola 1 | ||||
239 | 03 15 42 | - 54 18 | 120 m | 103a - D | GG 495 | M. Smith | 10 11 69 | Klemola 7 | ||||
240 | 02 45 30 | - 35 19 | 90 m | 103a - D | GG 495 | M. Smith | 10 11 69 | Klemola 3 | ||||
241 | 02 45 30 | - 35 19 | 90 m | 103a - O | GG 385 | M. Smith | 11 11 69 | Klemola 3 | ||||
242 | 03 15 42 | - 54 18 | 48 m | 103a - O | GG 385 | M. Smith | 11 11 69 | Klemola 7 | ||||
243 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | J. Graham | 12 11 69 | NGC 121 | ||||
244 | 01 49 06 | - 73 51 | 60 m | 103a - O | GG 385 | J. Graham | 12 11 69 | Lindsay 133 | ||||
245 | 04 59 00 | - 66 01 | 60 m | 103a - O | GG 385 | J. Graham | 12 11 69 | NGC 1783 | ||||
246 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | J. Graham | 12 11 69 | NGC 121 | bad plate | |||
247 | 03 44 36 | - 71 45 | 55 m | 103a - O | GG 385 | J. Graham | 12 11 69 | NGC 1466 | ||||
248 | 04 59 00 | - 66 01 | 55 m | 103a - O | GG 385 | J. Graham | 12 11 69 | NGC 1783 | ||||
249 | 00 47 56 | - 25 25 | 45 m | 103a - O | none | V. Blanco | 14 11 69 | NGC 2453 | Plate 11 X 14 | |||
250 | 02 38 18 | - 34 39 | 45 m | 103a - O | none | V. Blanco | 14 11 69 | Fornax | Plate 11 X 14 | |||
251 | 05 39 00 | - 69 06.8 | 20 m | 103a - O | none | V. Blanco | 14 11 69 | Tarantula | Plate 11 X 14 | |||
252 | 05 39 00 | - 69 06.8 | 20 m | 103a - O | none | V. Blanco | 14 11 69 | Tarantula | Plate 11 X 14 | |||
253 | 05 22 28 | - 68 00.3 | 20 m | 103a - O | none | V. Blanco | 14 11 69 | NGC 1927 | Plate 11 X 14 | |||
219 |
Last Updated on 8/27/99
By Guerra & Marin
December 1969 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp.Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
254 | 05 39 00 | - 69 11.9 | 15 m | lla - O | UG 2 | 2" - 3" | Mendoza | 02 12 69 | R 136 | |||
255 | 05 39 00 | - 69 11.9 | 85 m | I N hip. | RG 695 | 2" - 3" | Mendoza | 02 12 69 | R 136 | |||
256 | 05 39 00 | - 69 11.9 | 45 m | I N hip. | RG 695 | 3" | Mendoza | 02 12 69 | R 136 | |||
257 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 2" | Graham | 03 12 69 | NGC 1783 | |||
258 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 2" | Graham | 03 12 69 | Boktifft | |||
259 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 1.5" | Graham | 03 12 69 | NGC 1783 | |||
260 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 1.5" | Graham | 03 12 69 | Boktifft | |||
261 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 1.5" | Graham | 03 12 69 | NGC 1783 | |||
262 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 1" | Graham | 03 12 69 | Boktifft | |||
263 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 1" | Graham | 03 12 69 | NGC 1783 | |||
264 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 2.5" | Graham | 03 12 69 | Boktifft | |||
265 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 2.5" | Graham | 04 12 69 | NGC 1783 | |||
266 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 2" | Graham | 04 12 69 | Boktifft | |||
267 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 2" | Graham | 04 12 69 | NGC 1783 | |||
268 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 2" | Graham | 04 12 69 | Boktifft | |||
269 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 2" | Graham | 04 12 69 | NGC 1783 | |||
270 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 2" | Graham | 04 12 69 | Boktifft | |||
271 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 1" | Graham | 04 12 69 | NGC 1783 | |||
272 | 05 09 00 | - 69 00 | 31 m | 103a - O | none | 1" | Graham | 04 12 69 | Boktifft | |||
273 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 1" | Graham | 04 12 69 | NGC 1783 | |||
274 | 00 22 36 | - 72 14 | 40 m | 103a - O | none | 2" | Graham | 05 12 69 | 47 Tucan | |||
275 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 2" | Graham | 05 12 69 | NGC 1783 | |||
276 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 2" | Graham | 05 12 69 | Boktifft | |||
277 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 2" - 3" | Graham | 05 12 69 | NGC 1783 | |||
278 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 2" - 3" | Graham | 05 12 69 | Boktifft | |||
279 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 2" - 3" | Graham | 05 12 69 | NGC 1783 | |||
280 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 1.5" | Graham | 05 12 69 | Boktifft | |||
281 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 1.5" | Graham | 05 12 69 | NGC 1783 | |||
282 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | 1.5" | Graham | 05 12 69 | Boktifft | |||
283 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | 1.5" | Graham | 05 12 69 | NGC 1783 | |||
284 | 03 10 54 | - 55 25 | 10 m | 103a - D | GG 495 | Contreras | 14 12 69 | NGC 1261 | ||||
285 | 03 10 54 | - 55 25 | 30 m | 103a - O | GG 385 | Contreras | 14 12 69 | NGC 1261 | ||||
286 | 03 13 23 | - 55 21 | 20 m | 103a - O | GG 385 | Contreras | 14 12 69 | NGC 1261 | ||||
287 | 03 13 23 | - 55 21 | 20 m | 103a - D | GG 495 | Contreras | 14 12 69 | NGC 1261 | ||||
288 | 07 17 00 | - 24 50 | 05 m | 103a - O | GG 385 | Contreras | 14 12 69 | NGC 2362 | ||||
289 | 07 17 00 | - 24 50 | 20 m | 103a - O | GG 385 | Contreras | 15 12 69 | NGC 2362 | ||||
290 | 07 17 00 | - 24 50 | 20 m | 103a - D | GG 495 | Contreras | 15 12 69 | NGC 2362 | ||||
291 | 07 17 00 | - 24 50 | 20 m | 103a - D | GG 495 | Contreras | 15 12 69 | NGC 2362 | ||||
292 | 07 17 00 | - 24 50 | 20 m | 103a - O | GG 385 | Contreras | 15 12 69 | NGC 2362 | ||||
293 | 07 17 00 | - 24 50 | 20 m | 103a - D | GG 495 | Contreras | 15 12 69 | NGC 2362 | ||||
294 | 05 12 24 | - 40 05 | 20 m | 103a - O | GG 385 | Contreras | 15 12 69 | NGC 1851 | ||||
295 | 05 12 24 | - 40 05 | 20 m | 103a - D | GG 495 | Contreras | 15 12 69 | NGC 1851 | ||||
296 | 13 25 00 | - 47 09 | 20 m | 103a - O | GG 385 | Contreras | 15 12 69 | Omega Cen | ||||
297 | 03 10 54 | - 55 25 | 10 m | 103a - O | GG 385 | Contreras | 15 12 69 | NGC 1261 | ||||
298 | 03 10 54 | - 55 25 | 20 m | 103a - D | GG 495 | Contreras | 16 12 69 | NGC 1261 | ||||
299 | 03 10 54 | - 55 25 | 10 m | 103a - O | GG 385 | Contreras | 16 12 69 | NGC 1261 | ||||
300 | 03 10 54 | - 55 25 | 20 m | 103a - D | GG 495 | Contreras | 16 12 69 | NGC 1261 | ||||
301 | 05 12 00 | - 44 05 | 10 m | 103a - O | GG 385 | Contreras | 16 12 69 | NGC 1851 | ||||
302 | 05 12 00 | - 44 05 | 20 m | 103a - D | GG 495 | Contreras | 16 12 69 | NGC 1851 | ||||
303 | 05 12 00 | - 44 05 | 10 m | 103a - O | GG 385 | Contreras | 16 12 69 | NGC 1851 | ||||
304 | 07 17 00 | - 24 50 | 05 m | 103a - O | GG 385 | Contreras | 16 12 69 | NGC 2362 | ||||
305 | 07 17 00 | - 24 50 | 15 m | 103a - O | UG 2 | Contreras | 16 12 69 | NGC 2362 | ||||
306 | 07 17 00 | - 24 50 | 10 m | 103a - D | GG 495 | Contreras | 16 12 69 | NGC 2362 | ||||
307 | 09 10 54 | - 64 39 | 20 m | 103a - D | GG 495 | Contreras | 16 12 69 | NGC 2808 | ||||
308 | 09 10 54 | - 64 39 | 10 m | 103a - O | GG 385 | Contreras | 16 12 69 | NGC 2808 |
Last Updated on 8/27/99
By Jorge Marin
1970 Plate logs for 1.5-m
February 1970 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
311 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | Graham | 04 02 70 | NGC 1783 | ||||
312 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | Graham | 04 02 70 | Bok tifft | ||||
313 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | Graham | 04 02 70 | NGC 1783 | ||||
314 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | Graham | 04 02 70 | Bok tifft | ||||
315 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | Graham | 04 02 70 | NGC 1783 | ||||
316 | 08 56 30 | - 28 41 | 15 m | 103a - O | GG 385 | Graham | 04 02 70 | K 1 - 2 | ||||
317 | 09 40 00 | - 54 00 | 04 m | lla - O | GG 385 | Graham | 04 02 70 | Field | ||||
318 | 09 40 00 | - 54 00 | 05 m | 103a - D | GG 495 | Graham | 04 02 70 | Field | ||||
319 | 11 12 00 | - 61 05 | 60 m | 103a - E | RG 610 | Graham | 04 02 70 | NGC 3603 | ||||
320 | 10 44 00 | -59 26 | 20 m | 103a - E | RG 610 | Graham | 04 02 70 | Eta Carina | ||||
321 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | Graham | 05 02 70 | NGC 1783 | ||||
322 | 05 05 30 | - 69 26 | 30 m | 103a - O | none | Graham | 05 02 70 | NGC 1835 | ||||
323 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | Graham | 05 02 70 | NGC 1783 | ||||
324 | 05 09 00 | - 69 00 | 30 m | 103a - O | none | Graham | 05 02 70 | Bok tifft | ||||
325 | 04 59 00 | - 66 01 | 30 m | 103a - O | none | Graham | 05 02 70 | NGC 1783 | ||||
326 | 08 56 30 | - 28 41 | 20 m | lla - D | GG 495 | J Graham | 05 02 70 | K 1 - 2 | Numeracion correcta | |||
327 | 09 40 00 | - 54 00 | 05 m | lla - O | GG 385 | J Graham | 05 03 70 | Vela Field | Numeracion correcta | |||
328 | 09 40 00 | - 54 00 | 05 m | 103a - D | GG 495 | J Graham | 05 02 70 | Vela Field | Numeracion correcta | |||
329 | 11 00 00 | - 62 00 | 60 m | lla - O | none | J Graham | 05 02 70 | Carina | Numeracion correcta | |||
330 | 13 23 27 | - 42 45.7 | 20 m | 103a - O | none | Smith | 09 02 70 | NGC 5128 | Numeracion correcta | |||
331 | 13 23 27 | - 42 45.7 | 10 m | 103a - O | none | Smith | 09 02 70 | NGC 5128 | Numeracion correcta | |||
332 | 13 23 27 | - 42 45.7 | 160 m | 103a - O | none | Smith | 09 02 70 | NGC 5128 | Numeracion correcta | |||
326 | 09 25 18 | - 52 50.8 | 04 m | 103a - D | GG 495 | Miller | 08 02 70 | HD 81848 | Numeracion ??? | |||
327 | 09 25 18 | - 52 50.8 | 04 m | 103a - D | GG 495 | Miller | 08 02 70 | HD 81848 | ||||
328 | 09 25 18 | - 52 50.8 | 20 m | 103a - D | GG 495 | Miller | 08 02 70 | HD 81848 | ||||
329 | 09 25 18 | - 52 50.8 | 15 m | 103a - O | GG 385 | Miller | 08 02 70 | HD 81848 | ||||
330 | 09 25 18 | - 52 50.8 | 45 m | 103a - O | UG 2 | Miller | 08 02 70 | HD 81848 | ||||
331 | 10 58 54 | - 60 17 | 45 m | 103a - O | UG 2 | Miller | 08 02 70 | HD 95414 | ||||
332 | 10 58 54 | - 60 17 | 15 m | 103a - O | GG 385 | Miller | 08 02 70 | HD 95414 | ||||
333 | 10 58 54 | - 60 17 | 20 m | 103a - D | GG 495 | Miller | 08 02 70 | HD 95414 | ||||
334 | 12 10 42 | - 62 47 | 20 m | 103a - D | GG 495 | Miller | 08 02 70 | HD 106068 | ||||
335 | 12 10 42 | - 62 47 | 15 m | 103a - O | GG 385 | Miller | 08 02 70 | HD 106068 | ||||
336 | 12 10 42 | - 62 47 | 45 m | 103a - O | UG 2 | Miller | 08 02 70 | HD 106068 | ||||
337 | 15 50 48 | - 53 04 | 45 m | 103a - O | UG 2 | Miller | 08 02 70 | Norma lll | ||||
338 | 15 50 48 | - 53 04 | 15 m | 103a - O | GG 385 | Miller | 08 02 70 | Norma lll | ||||
339 | 15 50 48 | - 53 04 | 20 m | 103a - D | GG 495 | Miller | 08 02 70 | Norma lll | ||||
340 | 15 50 48 | - 53 04 | 10 m | 103a - D | GG 495 | Miller | 08 02 70 | Norma lll | ||||
341 | 15 50 48 | - 53 04 | 15 m | 103a - O | UG 2 | Miller | 08 02 70 | Norma lll | ||||
342 | 09 25 00 | - 52 51 | 05 m | 103a - O | GG 385 | Miller | 09 02 70 | HD 81848 | ||||
343 | 09 25 00 | - 52 51 | 10 m | 103a - D | GG 495 | Miller | 09 02 70 | HD 81848 | ||||
344 | 09 25 00 | - 52 51 | 15 m | 103a - O | UG 2 | Miller | 09 02 70 | HD 81848 | ||||
345 | 09 40 12 | - 53 58 | 45 m | 103a - O | UG 2 | Miller | 09 02 70 | HD 84092 | ||||
346 | 09 40 12 | - 53 58 | 15 m | 103a - O | GG 385 | Miller | 09 02 70 | HD 84092 | ||||
347 | 09 40 12 | - 53 58 | 20 m | 103a - D | GG 495 | Miller | 09 02 70 | HD 84092 | ||||
348 | 09 40 12 | - 53 58 | 15 m | 103a - O | UG 2 | Miller | 09 02 70 | HD 84092 | ||||
349 | 11 30 12 | - 60 31 | 60 m | lla - O | UG 2 | Miller | 09 02 70 | SA 193 | Broken Ok" | CTIO | ||
350 | 11 30 12 | - 60 31 | 20 m | lla - O | GG 385 | Miller | 09 02 70 | SA 193 | CTIO | |||
351 | 11 30 12 | - 60 31 | 15 m | 103a - D | GG 495 | Miller | 09 02 70 | SA 193 | CTIO | |||
352 | 11 30 12 | - 60 31 | 04 m | 103a - D | GG 495 | Miller | 09 02 70 | SA 193 | ||||
353 | 12 11 00 | - 62 47 | 30 m | lla - O | UG 2 | Miller | 09 02 70 | HD 106068 | ||||
354 | 12 11 00 | - 62 47 | 10 m | lla - O | GG 385 | Miller | 09 02 70 | HD 106068 | ||||
355 | 12 11 00 | - 62 47 | 04 m | 103a - D | GG 495 | Miller | 09 02 70 | HD 106068 | ||||
356 | 15 50 48 | - 53 04 | 10 m | 103a - D | GG 495 | Miller | 09 02 70 | Norma lll | ||||
357 | 15 50 48 | - 53 04 | 04 m | lla - O | GG 385 | Miller | 09 02 70 | Norma lll | ||||
358 | 15 50 48 | - 53 04 | 20 m | lla - O | UG 2 | Miller | 09 02 70 | Norma lll | ||||
359 | 15 50 06 | - 56 14.4 | 30 m | lla - O | UG 2 | Miller | 09 02 70 | Norma ll | ||||
360 | 09 39 18 | - 54 04.7 | 60 m | lla - O | UG 2 | Miller | 10 02 70 | HD 84092 | ||||
361 | 10 19 54 | - 55 55.6 | 30 m | lla - O | UG 2 | Miller | 10 02 70 | HD 89890 | ||||
362 | 10 19 54 | - 55 55.6 | 10 m | lla - O | GG 385 | Miller | 10 02 70 | HD 89890 | ||||
363 | 10 19 54 | - 55 55.6 | 04 m | 103a - D | GG 495 | Miller | 10 02 70 | HD 89890 | CTIO | |||
364 | 10 58 48 | - 60 16.6 | 04 m | 103a - D | GG 495 | Miller | 10 02 70 | HD 95414 | ||||
365 | 10 58 48 | - 60 16.6 | 10 m | lla - O | GG 385 | Miller | 10 02 70 | HD 95414 | ||||
366 | 10 58 48 | - 60 16.6 | 30 m | lla - O | UG 2 | Miller | 10 02 70 | HD 95414 | ||||
367 | 11 30 12 | - 60 32 | 30 m | lla - O | UG 2 | Miller | 10 02 70 | SA 193 | ||||
368 | 11 30 12 | - 60 32 | 10 m | lla - O | GG 385 | Miller | 10 02 70 | SA 193 | ||||
369 | 12 10 42 | - 62 32 | 10 m | 103a - D | GG 495 | Miller | 10 02 70 | HD 106068 | ||||
370 | 14 19 00 | - 60 48 | 05 m | 103a - D | GG 495 | Miller | 10 02 70 | HD 125206 | ||||
371 | 14 19 00 | - 60 48 | 10 m | lla - O | GG 385 | Miller | 10 02 70 | HD 125206 | ||||
372 | 14 19 00 | - 60 48 | 30 m | lla - O | UG 2 | Miller | 10 02 70 | HD 125206 | ||||
373 | 15 55 30 | - 54 15.7 | 30 m | lla - O | UG 2 | Miller | 10 02 70 | Norma l | ||||
374 | 15 55 30 | - 54 15.7 | 10 m | lla - O | GG 385 | Miller | 10 02 70 | Norma l | ||||
375 | 15 55 30 | - 54 15.7 | 05 m | 103a - D | GG 495 | Miller | 10 02 70 | Norma l | ||||
376 | 15 50 06 | - 56 14.4 | 20 m | 103a - D | GG 495 | Miller | 10 02 70 | Norma ll | ||||
377 | 15 50 06 | - 56 14.4 | 30 m | lla - O | GG 385 | Miller | 10 02 70 | Norma ll | ||||
378 | 15 50 06 | - 56 14.4 | 53 m | lla - O | UG 2 | Miller | 10 02 70 | Norma ll | ||||
379 | 12 23 54 | - 72 24.5 | 30 m | 103a - O | GG 385 | J. Hesser | 14 02 70 | NGC 4372 | ||||
380 | 17 23 35 | - 48 23.5 | 45 m | 103a - O | GG 385 | J. Hesser | 14 02 70 | NGC 6352 | ||||
381 | 17 23 35 | - 48 23.5 | 45 m | 103a - D | GG 495 | J. Hesser | 14 02 70 | NGC 6352 | ||||
382 | 17 23 35 | - 48 23.5 | 45 m | 103a - O | GG 385 | J. Hesser | 14 02 70 | NGC 6352 | ||||
383 | 17 23 35 | - 48 23.5 | 22 m | 103a - D | GG 495 | J. Hesser | 14 02 70 | NGC 6352 | ||||
384 | 07 50 32 | - 38 26 | 30 m | lla - O | GG 385 | J. Hesser | 16 02 70 | NGC 2477 | ||||
385 | 12 22 42 | - 72 29.5 | 30 m | lla - O | GG 385 | J. Hesser | 16 02 70 | NGC 4372 | ||||
386 | 12 22 42 | - 72 29.5 | 30 m | 103a - D | GG 495 | J. Hesser | 16 02 70 | NGC 4372 | ||||
387 | 12 22 42 | - 72 29.5 | 30 m | lla - O | GG 385 | J. Hesser | 16 02 70 | NGC 4372 | ||||
388 | 17 12 00 | - 29 26.7 | 30 m | lla - O | GG 385 | J. Hesser | 16 02 70 | NGC 6304 | ||||
389 | 17 12 00 | - 29 26.7 | 30 m | 103a - D | GG 495 | J. Hesser | 16 02 70 | NGC 6304 | ||||
390 | 17 22 30 | - 48 24.2 | 45 m | lla - O | GG 385 | J. Hesser | 16 02 70 | NGC 6352 | ||||
391 | 17 22 30 | - 48 24.2 | 45 m | 103a - D | GG 495 | J. Hesser | 16 02 70 | NGC 6352 | ||||
392 | 17 22 30 | - 48 24.2 | 60 m | lla - O | GG 385 | J. Hesser | 16 02 70 | NGC 6352 | ||||
393 | 07 50 24 | - 38 25.8 | 15 m | lla - O | GG 385 | J. Hesser | 17 02 70 | NGC 2477 | ||||
394 | 07 50 24 | - 38 25.8 | 15 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 2477 | ||||
395 | 07 50 24 | - 38 25.8 | 15 m | lla - O | GG 385 | J. Hesser | 17 02 70 | NGC 2477 | ||||
396 | 07 50 24 | - 38 25.8 | 15 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 2477 | ||||
397 | 07 50 24 | - 38 25.8 | 15 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 2477 | ||||
398 | 30 m | lla - O | GG 385 | J. Hesser | 17 02 70 | NGC 2260 | ||||||
399 | 30 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 2260 | ||||||
400 | 12 22 15 | - 72 28.8 | 30 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 4372 | ||||
401 | 12 22 15 | - 72 28.8 | 30 m | lla - O | GG 385 | J. Hesser | 17 02 70 | NGC 4372 | ||||
402 | 17 12 00 | - 29 26.7 | 30 m | lla - O | GG 385 | J. Hesser | 17 02 70 | NGC 6304 | ||||
403 | 17 12 00 | - 29 26.7 | 30 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 6304 | ||||
404 | 17 12 00 | - 29 26.7 | 15 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 6304 | ||||
405 | 17 12 00 | - 29 26.7 | 15 m | lla - O | GG 385 | J. Hesser | 17 02 70 | NGC 6304 | ||||
406 | 17 12 00 | - 29 26.7 | 30 m | lla - O | GG 385 | J. Hesser | 17 02 70 | NGC 6304 | ||||
407 | 17 12 00 | - 29 26.7 | 30 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 6304 | ||||
408 | 17 23 35 | - 48 23.5 | 45 m | 103a - D | GG 495 | J. Hesser | 17 02 70 | NGC 6352 | ||||
409 | 18 00 24 | - 30 02 | 40 m | lla - O | GG 385 | J. Hesser | 17 02 70 | NGC 6522 | CTIO | |||
410 | 09 10 54 | - 64 39 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 2808 | ||||
411 | 09 10 54 | - 64 39 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 2808 | ||||
412 | 09 10 54 | - 64 39 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 2808 | ||||
413 | 09 10 54 | - 64 39 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 2808 | ||||
414 | 09 10 54 | - 64 39 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 2808 | ||||
415 | 09 10 54 | - 64 39 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 2808 | ||||
416 | 09 10 54 | - 64 39 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 2808 | ||||
417 | 09 10 54 | - 64 39 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 2808 | ||||
418 | 12 56 00 | - 70 36 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 4833 | ||||
419 | 12 56 00 | - 70 36 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 4833 | ||||
420 | 12 56 00 | - 70 36 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 4833 | ||||
421 | 12 56 00 | - 70 36 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 4833 | ||||
422 | 12 56 00 | - 70 36 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 4833 | ||||
423 | 12 56 00 | - 70 36 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 4833 | ||||
424 | 17 21 36 | - 48 26 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 6352 | ||||
425 | 17 21 36 | - 48 26 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 6352 | ||||
426 | 17 21 36 | - 48 26 | 18 m | 103a - D | GG 495 | G. Alcaino | 23 02 70 | NGC 6352 | ||||
427 | 17 21 36 | - 48 26 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 6352 | ||||
428 | 17 21 36 | - 48 26 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 6352 | ||||
429 | 17 21 36 | - 48 26 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 6352 | ||||
430 | 19 06 24 | - 60 04 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 6752 | ||||
431 | 19 06 24 | - 60 04 | 18 m | lla - O | GG 385 | G. Alcaino | 23 02 70 | NGC 6752 | ||||
432 | 05 12 24 | - 40 05 | 18 m | 103a - D | GG 495 | G. Alcaino | 24 02 70 | NGC 1851 | ||||
433 | 05 12 24 | - 40 05 | 18 m | 103a - D | GG 495 | G. Alcaino | 24 02 70 | NGC 1851 | ||||
434 | 12 23 00 | - 72 24 | 25 m | lla - O | GG 385 | G. Alcaino | 24 02 70 | NGC 4372 | ||||
435 | 12 23 00 | - 72 24 | 25 m | lla - O | GG 385 | G. Alcaino | 24 02 70 | NGC 4372 | ||||
436 | 12 23 00 | - 72 24 | 25 m | 103a - D | GG 495 | G. Alcaino | 24 02 70 | NGC 4372 | ||||
437 | 12 23 00 | - 72 24 | 25 m | 103a - D | GG 495 | G. Alcaino | 24 02 70 | NGC 4372 | ||||
438 | 13 43 00 | - 51 07 | 25 m | lla - O | GG 385 | G. Alcaino | 24 02 70 | NGC 5286 | ||||
439 | 13 43 00 | - 51 07 | 25 m | 103a - D | GG 495 | G. Alcaino | 24 02 70 | NGC 5286 | ||||
440 | 13 43 00 | - 51 07 | 35 m | lla - O | GG 385 | G. Alcaino | 24 02 70 | NGC 5286 | ||||
441 | 13 43 00 | - 51 07 | 35 m | 103a - D | GG 495 | G. Alcaino | 24 02 70 | NGC 5286 | ||||
442 | 13 25 00 | - 47 09 | 25 m | lla - O | GG 385 | G. Alcaino | 24 02 70 | NGC 5139 | ||||
443 | 13 25 00 | - 47 09 | 25 m | 103a - D | GG 495 | G. Alcaino | 24 02 70 | NGC 5139 | ||||
444 | 05 12 24 | - 40 05 | 25 m | lla - O | GG 385 | G. Alcaino | 25 02 70 | NGC 1851 | ||||
445 | 05 12 24 | - 40 05 | 30 m | lla - O | GG 385 | G. Alcaino | 25 02 70 | NGC 1851 | ||||
446 | 05 12 24 | - 40 05 | 23 m | 103a - D | GG 495 | G. Alcaino | 25 02 70 | NGC 1851 | ||||
447 | 10 44 00 | - 59 33 | 05 m | 103a - D | GG 495 | G. Alcaino | 25 02 70 | Eta Carina | ||||
448 | 12 23 00 | - 72 24 | 25 m | 103a - D | GG 495 | G. Alcaino | 25 02 70 | NGC 4372 | ||||
449 | 12 23 00 | - 72 24 | 20 m | 103a - D | GG 495 | G. Alcaino | 25 02 70 | NGC 4372 | ||||
450 | 12 23 00 | - 72 24 | 25 m | lla - O | GG 385 | G. Alcaino | 25 02 70 | NGC 4372 | ||||
451 | 12 23 00 | - 72 24 | 35 m | lla - O | GG 385 | G. Alcaino | 25 02 70 | NGC 4372 | ||||
452 | 13 43 00 | - 51 07 | 30 m | lla - O | GG 385 | G. Alcaino | 25 02 70 | NGC 5286 | ||||
453 | 13 43 00 | - 51 07 | 30 m | 103a - D | GG 495 | G. Alcaino | 25 02 70 | NGC 5286 | ||||
454 | 13 43 00 | - 51 07 | 40 m | 103a - D | GG 495 | G. Alcaino | 25 02 70 | NGC 5286 | ||||
455 | 13 43 00 | - 51 07 | 40 m | 103a - D | GG 495 | G. Alcaino | 25 02 70 | NGC 5286 | ||||
456 | 05 12 24 | - 40 05 | 30 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | NGC 1851 | ||||
457 | 05 12 24 | - 40 05 | 22 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 1851 | ||||
458 | 10 44 00 | - 59 33 | 04 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | Eta Carina | ||||
459 | 10 44 00 | - 59 33 | 06 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | Eta Carina | ||||
460 | 10 44 00 | - 59 33 | 09 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | Eta Carina | ||||
461 | 10 44 00 | - 59 33 | 06 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | Eta Carina | ||||
462 | 10 44 00 | - 59 33 | 08 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | Eta Carina | ||||
463 | 10 44 00 | - 59 33 | 12 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | Eta Carina | ||||
464 | 10 44 00 | - 59 33 | 15 m | lla - O | U G 2 | G. Alcaino | 26 02 70 | Eta Carina | ||||
465 | 10 44 00 | - 59 33 | 30 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | Eta Carina | ||||
466 | 13 43 00 | - 51 07 | 25 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 5286 | ||||
467 | 13 43 00 | - 51 07 | 30 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | NGC 5286 | ||||
468 | 13 43 00 | - 51 07 | 35 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | NGC 5286 | ||||
469 | 17 21 36 | - 48 26 | 30 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | NGC 6352 | ||||
470 | 17 26 36 | - 67 01 | 20 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | NGC 6362 | ||||
471 | 17 26 36 | - 67 01 | 30 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | NGC 6362 | ||||
472 | 17 26 36 | - 67 01 | 18 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 6362 | ||||
473 | 17 26 36 | - 67 01 | 25 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 6362 | ||||
474 | 18 04 24 | - 43 44 | 18 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 6541 | ||||
475 | 18 04 24 | - 43 44 | 20 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 6541 | ||||
476 | 18 04 24 | - 43 44 | 20 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | NGC 6541 | ||||
477 | 18 04 24 | - 43 44 | 30 m | lla - O | GG 385 | G. Alcaino | 26 02 70 | NGC 6541 | ||||
478 | 18 04 24 | - 43 44 | 16 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 6541 | ||||
479 | 19 06 24 | - 60 04 | 18 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 6752 | ||||
480 | 19 06 24 | - 60 04 | 15 m | 103a - D | GG 495 | G. Alcaino | 26 02 70 | NGC 6752 | ||||
481 | 01 al 40 | 481 al 520 | (*) | |||||||||
521 | ¿ | |||||||||||
522 | ¿ | |||||||||||
523 | ¿ | |||||||||||
524 | ¿ |
(*) Numeración correspondiente a tubo imagen
Last updated on 8/27/99
By Guerra & Marin
March 1970 Plate log for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
525 | 08 56 30 | - 28 41 | 20 m | lla - D | GG 495 | J Graham | 05 03 70 | K 1 - 2 | ||||
526 | 09 40 00 | - 54 00 | 05 m | lla - O | GG 385 | J Graham | 05 03 70 | Vela Field | ||||
527 | 09 40 00 | - 54 00 | 05 m | 103a - D | GG 495 | J Graham | 05 03 70 | Vela Field | ||||
528 | 11 00 00 | - 62 00 | 60 m | lla - O | none | J Graham | 05 03 70 | Carina | ||||
529 | 13 23 27 | - 42 45.7 | 20 m | 103a - O | none | Smith | 05 03 70 | NGC 5128 | ||||
530 | 13 23 27 | - 42 45.7 | 10 m | 103a - O | none | Smith | 05 03 70 | NGC 5128 | ||||
531 | 13 23 27 | - 42 45.7 | 160 m | 103a - O | none | Smith | 05 03 70 | NGC 5128 | ||||
41-42 | 532 - 533 | (*) |
(*) Numeración correspondiente a tubo imagen
Last Updated on 8/27/99
By Guerra & Marin
April 1970 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
534 | 05 35 29 | - 49 45.3 | 15 m | 103a - O | none | Kunkel /Smith | 02 04 70 | PKS 0534-49 | ||||
´43 | 535 | (*) | ||||||||||
536 | 07 19 37 | - 55 21.8 | 15 m | 103a - O | none | Kunkel /Smith | 02 04 70 | PKS 0719-55 | ||||
´44 | 537 | (*) | ||||||||||
538 | 07 43 26 | - 67 22 | 15 m | 103a - O | none | Kunkel /Smith | 02 04 70 | PKS 0743-67 | ||||
539 | (*) | |||||||||||
540 | 10 11 25 | - 64 49 | 15 m | 103a - O | none | Kunkel /Smith | 02 04 70 | PKS 1010-64 | ||||
541 | (*) | |||||||||||
542 | 10 37 33 | -69 53.7 | 15 m | 103a - O | none | Kunkel /Smith | 02 04 70 | PKS 1036-69 | ||||
543 - 544 | (*) | |||||||||||
545 | 17 20 06 | - 80 03.4 | 15 m | 103a - O | none | Kunkel /Smith | 02 04 70 | PKC 1716-80 | ||||
546 - 547 | (*) | |||||||||||
548 | 17 56 25 | - 59 46.8 | 15 m | 103a - O | none | Kunkel /Smith | 02 04 70 | PKS 1754-59 | ||||
549 | 17 55 30 | - 26 33 | 30 m | 103a - O | none | Kunkel /Smith | 02 04 70 | GX 3 + 1 | ||||
550 | 17 59 30 | - 25 05 | 30 m | 103a - O | none | Kunkel /Smith | 02 04 70 | GX 5 - 1 | ||||
551 | 17 59 48 | - 20 31 | 25 m | 103a - O | none | Kunkel /Smith | 02 04 70 | GX 9 - 1 |
(*) Numeración correspondiente a tubo imagen
Last Updated on 8/27/99
By Jorge Marin
May 1970 Plate log for 1.5-m telescope
September 1970 Plate log for 1.5-m telescope
October 1970 Plate log for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1017 | 01 30 00 | - 71 30 | 40 m | 103a - O | nones | Graham | 28 09 70 | Gascoigne | ||||
1018 | 22 05 50 | - 53 56.5 | 10 m | 103a - O | nones | Smith | 01 10 70 | PKS 2204-52 | CTIO | |||
1019 | 22 08 27 | - 45 52 | 10 m | 103a - O | nones | Smith | 01 10 70 | PKS 2207-45 | CTIO | |||
1020 | 22 15 02 | - 45 15.1 | 10 m | 103a - O | nones | Smith | 01 10 70 | PKS 2213-45 | CTIO | |||
1021 | 22 25 06 | - 52 42.9 | 10 m | 103a - O | nones | Smith | 01 10 70 | PKS 2223-52 | CTIO | |||
1022 | 22 55 00 | - 52 55.5 | 10 m | 103a - O | nones | Smith | 01 10 70 | PKS 2252-53 | CTIO | |||
1023 | 00 14 36 | - 63 19.9 | 10 m | 103a - O | nones | Smith | 01 10 70 | PKS 0013-63 | CTIO | |||
1024 | 1024 | to 1033 | (*) | |||||||||
1034 | 00 25 42 | - 71 41 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 121 | ||||
1035 | 00 23 48 | - 72 56 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | Kron 3 | ||||
1036 | 05 05 18 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 1835 | |||||
1037 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 1783 | ||||
1038 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 1835 | ||||
1039 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 1783 | ||||
1040 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 1835 | ||||
1041 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 1783 | ||||
1042 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 1835 | ||||
1043 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 30 10 70 | NGC 1783 | ||||
1044 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 31 10 70 | NGC 1835 | ||||
1045 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 31 10 70 | NGC 1783 | ||||
1046 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 31 10 70 | NGC 1835 | ||||
1047 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 31 10 70 | NGC 1783 | ||||
1048 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 31 10 70 | NGC 1835 |
(*) Corresponde al Tubo Imagen
Last Updated on 8/27/99
By Guerra & Marin
November 1970 Plate log for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1049 | 00 25 42 | - 71 41 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 121 | ||||
1050 | 00 23 48 | - 72 56 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | Kron 3 | ||||
1051 | 00 25 42 | - 71 41 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 121 | ||||
1052 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1835 | ||||
1053 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1783 | ||||
1054 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1835 | ||||
1055 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1783 | ||||
1056 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1835 | ||||
1057 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1783 | ||||
1058 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1835 | ||||
1059 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1783 | ||||
1060 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1835 | ||||
1061 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 01 11 70 | NGC 1783 | ||||
1062 | 00 25 42 | - 71 41 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 121 | ||||
1063 | 00 23 48 | - 72 56 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | Kron 3 | ||||
1064 | 00 25 42 | - 71 41 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 121 | ||||
1065 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1835 | ||||
1066 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1783 | ||||
1067 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1835 | ||||
1068 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1783 | ||||
1069 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1835 | ||||
1070 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1783 | ||||
1071 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1835 | ||||
1072 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1783 | ||||
1073 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1835 | ||||
1074 | 04 59 00 | - 66 01 | 25 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1783 | ||||
1075 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | Graham / M.T.Ruiz | 02 11 70 | NGC 1835 | ||||
1076 | 22 28 00 | - 21 00 | 30 m | 103a - O | nones | Smith | 03 11 70 | NGC 7293 | ||||
1077 | 22 28 00 | - 21 00 | 180 m | 098 - 02 | nones | Smith | 03 11 70 | NGC 7293 | ||||
1078+A10 | (1) | (2) | ||||||||||
1088 | al 1097 | (*) | ||||||||||
1098 | 00 14 36 | - 63 19.9 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0013-63 | ||||
1099 | 01 10 42 | - 69 09.5 | 105 seg | lla - D | nones | Smith | 03 11 70 | Pks 0110-69 | CTIO | |||
1100 | 01 20 36 | - 63 18.4 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0119-63 | ||||
1101 | 01 30 00 | - 51 10.8 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0129-51 | ||||
1102 | 02 23 36 | - 71 07.8 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0223-71 | ||||
1103 | 02 31 18 | - 66 34.6 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0230-66 | ||||
1104 | 03 54 36 | - 48 28.2 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0354-48 | ||||
1105 | 04 20 33 | - 62 21.8 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0420-62 | ||||
1106 | 04 43 46 | - 59 28.1 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0443-59 | ||||
1107 | 05 35 29 | - 49 45.2 | 105 seg | lla - D | nones | Smith | 03 11 70 | PKS 0534-49 | ||||
1108 | 05 06 44 | - 37 33 | 30 m | lla - D | nones | Smith | 03 11 70 | NGC 1808 | ||||
1109 | 05 39 42 | - 69 09 | 2 m | lla - D | nones | Smith | 03 11 70 | 30 Doradus | ||||
1110 | 05 39 42 | - 69 09 | 5 m | lla - D | nones | Smith | 03 11 70 | 30 Doradus | ||||
1111 | 22 28 00 | - 21 00 | 180 m | lla - D | nones | Smith | 04 11 70 | NGC 7293 | ||||
1102 | al 1107 | (*) | ||||||||||
1108 | 05 06 44 | - 37 33 | 30 m | lla - D | nones | Smith | 04 11 70 | NGC 1808 | ||||
1109 | 05 06 44 | - 37 33 | 30 m | llla - j | GG 385 | Smith | 04 11 70 | NGC 1808 | ||||
1110 | 05 06 44 | - 37 33 | 30 m | 098 - 02 | RG 610 | Smith | 04 11 70 | NGC 1808 | ||||
1111 | 05 06 44 | - 37 33 | 5 m | 098 - 02 | RG 610 | Smith | 04 11 70 | NGC 1808 | ||||
1112 | 21 03 00 | - 51 27.5 | 30 m | 103a -O | GG 385 | Hesser | 05 11 70 | IC 5152 | ||||
1113 | 23 08 39 | - 35 36 | 30 m | 103a -O | GG 385 | Hesser | 05 11 70 | Field | ||||
1114 | 23 08 39 | - 35 36 | 30 m | 103a - D | GG 495 | Hesser | 05 11 70 | Field | ||||
1115 | 21 03 00 | - 51 27.5 | 30 m | 103a -O | GG 385 | Hesser | 05 11 70 | IC 5152 | ||||
1116 | 23 08 39 | - 35 36 | 30 m | 103a -O | GG 385 | Hesser | 05 11 70 | Field | ||||
1117 | 23 08 39 | - 35 36 | 30 m | 103a - D | GG 495 | Hesser | 05 11 70 | Field | ||||
1118 | 03 11 00 | - 55 23 | 30 m | 103a - D | GG 495 | Hesser | 05 11 70 | NGC 1261 | ||||
1119 | 23 08 39 | - 35 36 | 30 m | 103a - D | GG 495 | Hesser | 05 11 70 | Field | ||||
1120 | 23 08 39 | - 35 36 | 30 m | 103a -O | GG 385 | Hesser | 05 11 70 | Field | ||||
1121 | 22 00 54 | - 51 26 | 30 m | 103a -O | GG 385 | Hesser | 06 11 70 | IC 5152 | ||||
1122 | 22 00 54 | - 51 26 | 45 m | 103a -O | GG 385 | Hesser | 06 11 70 | IC 5152 | ||||
1123 | 22 00 54 | - 51 26 | 60 m | 103a -O | GG 385 | Hesser | 06 11 70 | IC 5152 | ||||
1124 | 05 36 00 | - 70 52 | 05 m | 103a -O | GG 385 | Hesser | 06 11 70 | L M C | ||||
1125 | 03 11 00 | - 55 23 | 30 m | 103a -O | GG 385 | Hesser | 06 11 70 | NGC 1261 | ||||
1126 | 03 11 00 | - 55 23 | 30 m | 103a - D | GG 495 | Hesser | 06 11 70 | NGC 1261 | ||||
1127 | 04 49 30 | - 83 59.3 | 30 m | 103a - D | GG 495 | Hesser | 06 11 70 | NGC 1841 | ||||
1128 | 04 49 30 | - 83 59.3 | 30 m | 103a -O | GG 385 | Hesser | 06 11 70 | NGC 1841 | ||||
1129 | 07 51 09 | - 38 27 | 30 m | 103a -O | GG 385 | Hesser | 06 11 70 | NGC 2477 | ||||
1130 | 07 51 09 | - 38 27 | 30 m | 103a - D | GG 495 | Hesser | 06 11 70 | NGC 2477 | ||||
1131 | 08 41 33 | - 47 06 | 30 m | 103a - D | GG 495 | Hesser | 06 11 70 | NGC 2660 | ||||
1132 | 08 41 33 | - 47 06 | 30 m | 103a -O | GG 385 | Hesser | 06 11 70 | NGC 2660 | ||||
1133 | 02 57 00 | - 71 41 | 40 m | 103a -O | nones | Gonzalez | 25 11 70 | NGC 121 | ||||
1134 | 01 02 00 | - 71 30 | 40 m | 103a -O | nones | Gonzalez | 25 11 70 | Gascoigne Field |
(1) al 1087 error de anotación
(2) debiera ser 1078 y no 1088
(*) corresponde a tubo imagen
Last Updated on 8/27/99
By Guerra & Marin
December 1970 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1135 | 05 58 24 | - 68 32.6 | 1 m | 103a - D | GG 495 | P. Lucke | 02 12 70 | NGC 2164 | ||||
1136 | 05 58 24 | - 68 32.6 | 10 m | 103a - D | GG 495 | P. Lucke | 02 12 70 | NGC 2164 | ||||
1137 | 05 58 24 | - 68 32.6 | 60 m | 103a - D | GG 495 | P. Lucke | 02 12 70 | NGC 2164 | ||||
1138 | 05 58 24 | - 68 32.6 | 10 m | 103a - D | GG 495 | P. Lucke | 02 12 70 | NGC 2164 | ||||
1139 | 05 58 24 | - 68 32.6 | 60 m | 103a - D | GG 495 | P. Lucke | 02 12 70 | NGC 2164 | ||||
1140 | 05 58 24 | - 68 32.6 | 2 m | 103a - D | GG 495 | P. Lucke | 02 12 70 | NGC 2164 | ||||
1141 | 05 58 24 | - 68 32.6 | 2 m | 103a - D | GG 495 | P. Lucke | 02 12 70 | NGC 2164 | ||||
1142 | 02 38 48 | - 34 41 | 60 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | Fornax | ||||
1143 | 05 58 24 | -68 32.6 | 1 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | NGC 2164 | ||||
1144 | 05 58 24 | -68 32.6 | 10 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | NGC 2164 | ||||
1145 | 05 58 24 | -68 32.6 | 60 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | NGC 2164 | ||||
1146 | 05 58 24 | -68 32.6 | 10 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | NGC 2164 | ||||
1147 | 05 58 24 | -68 32.6 | 1 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | NGC 2164 | ||||
1148 | 05 58 24 | -68 32.6 | 60 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | NGC 2164 | ||||
1149 | 05 58 24 | -68 32.6 | 1 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | NGC 2164 | ||||
1150 | 05 39 00 | - 69 06 | 15 m | 103a - O | GG 385 | P. Lucke | 03 12 70 | 30 Doradus | ||||
1151 | 05 58 24 | - 68 32.6 | 60 m | 103a - D | GG 495 | P. Lucke | 03 12 70 | NGC 2164 | ||||
1152 | al 1160 | (*) | ||||||||||
1161 | 05 26 06 | - 68 37.5 | 25 m | 103a - D | GG 495 | Demers | 26 12 70 | L M C | ||||
1162 | 05 26 06 | - 68 37.5 | 15 m | 103a - O | GG 385 | Demers | 26 12 70 | L M C | ||||
1163 | 00 15 48 | - 68 37.5 | 30 m | 103a - D | GG 495 | Demers | 26 12 70 | L M C | ||||
1164 | 00 15 48 | - 68 37.5 | 20 m | 103a - O | GG 385 | Demers | 26 12 70 | L M C | ||||
1165 | 05 06 42 | - 69 05 | 30 m | 103a - D | GG 495 | Demers | 26 12 70 | L M C | ||||
1166 | 05 06 42 | - 69 05 | 15 m | 103a - O | GG 385 | Demers | 26 12 70 | L M C | ||||
1167 | 04 57 00 | - 69 38 | 30 m | 103a - D | GG 495 | Demers | 26 12 70 | L M C | ||||
1168 | 04 57 00 | - 69 38 | 15 m | 103a - O | GG 385 | Demers | 26 12 70 | L M C | ||||
1169 | 05 08 12 | - 67 55 | 30 m | 103a - D | GG 495 | Demers | 26 12 70 | L M C | ||||
1170 | 05 08 12 | - 67 55 | 15 m | 103a - O | GG 385 | Demers | 26 12 70 | L M C | ||||
1171 | 05 10 00 | - 68 42 | 30 m | 103a - D | GG 495 | Demers | 26 12 70 | L M C | ||||
1172 | 05 26 06 | - 68 37.5 | 30 m | 103a - D | GG 495 | Demers | 27 12 70 | L M C | ||||
1173 | 05 26 06 | - 68 37.5 | 15 m | 103a - O | GG 385 | Demers | 27 12 70 | L M C | ||||
1174 | 05 15 42 | - 68 37.5 | 30 m | 103a - D | GG 495 | Demers | 27 12 70 | L M C | ||||
1175 | 05 15 42 | - 68 37.5 | 30 m | 103a - D | GG 495 | Demers | 27 12 70 | L M C | ||||
1176 | 05 15 42 | - 68 37.5 | 15 m | 103a - O | GG 385 | Demers | 27 12 70 | L M C | ||||
1177 | 05 08 12 | - 67 55 | 30 m | 103a - D | GG 495 | Demers | 27 12 70 | L M C | ||||
1178 | 05 08 12 | - 67 55 | 15 m | 103a - O | GG 385 | Demers | 27 12 70 | L M C | ||||
1179 | 05 10 00 | - 68 42 | 30 m | 103a - D | GG 495 | Demers | 27 12 70 | L M C | ||||
1180 | 05 10 00 | - 68 42 | 15 m | 103a - O | GG 385 | Demers | 27 12 70 | L M C | ||||
1181 | 05 10 00 | - 68 42 | 15 m | 103a - O | GG 385 | Demers | 27 12 70 | L M C | ||||
1182 | 05 32 12 | - 68 12 | 30 m | 103a - D | GG 495 | Demers | 27 12 70 | L M C | ||||
1183 | 05 32 12 | - 68 12 | 15 m | 103a - O | GG 385 | Demers | 27 12 70 | L M C | ||||
1184 | 05 06 42 | - 69 05 | 30 m | 103a - D | GG 495 | Demers | 27 12 70 | L M C | ||||
1185 | 05 06 42 | - 69 05 | 15 m | 103a - O | GG 385 | Demers | 27 12 70 | L M C | ||||
1186 | 04 57 00 | - 69 38 | 10 m | 103a - D | GG 495 | Demers | 27 12 70 | L M C |
(*) corresponde a tubo imagen
Last Updated on 8/27/99
By Jorge Marin
1971 Plate logs for 1.5-m telescope
January 1971 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1187 | 05 39 30 | - 69 20 | 30 m | 098 - 02 | RG 610 | Weedman / Smith | 02 01 71 | L M C | ||||
1188 | 04 51 00 | - 66 20 | 15 m | 098 - 02 | RG 610 | Weedman / Smith | 02 01 71 | L M C | ||||
1189 | 05 32 00 | - 67 20 | 30 m | 098 - 02 | RG 610 | Weedman / Smith | 02 01 71 | L M C | BROKEN OK" | CTIO | ||
1190 | 05 25 00 | - 67 40 | 30 m | 098 - 02 | RG 610 | Weedman / Smith | 02 01 71 | L M C | BROKEN OK" | CTIO | ||
1191 | 05 27 00 | - 68 50 | 30 m | 098 - 02 | RG 610 | Weedman / Smith | 02 01 71 | L M C | CTIO | |||
1192 | 05 10 00 | - 68 50 | 30 m | 098 - 02 | RG 610 | Weedman / Smith | 02 01 71 | L M C | CTIO | |||
1193 | 05 19 00 | - 69 30 | 30 m | 098 - 02 | RG 610 | Weedman / Smith | 02 01 71 | L M C | CTIO | |||
1194 | 02 38 18 | - 34 39 | 120 m | 103a - O | GG 385 | Kunkel / Bradt | 18 01 71 | Fornax | ||||
1195 | 11 20 00 | - 61 03 | 20 m | 103a - O | GG 385 | Kunkel / Bradt | 18 01 71 | Centaurus 3 | CTIO | |||
1196 | 11 20 00 | - 61 03 | 120 m | 103a - O | U G 2 | Kunkel / Bradt | 18 01 71 | Centaurus 3 | CTIO | |||
1197 | 15 19 18 | - 56 47 | 30 m | 103a - O | GG 385 | Kunkel / Bradt | 18 01 71 | Norman 2 | CTIO | |||
1198 | 02 38 18 | - 34 39 | 166 m | 103a - D | GG 495 | Kunkel / Bradt | 19 01 71 | Fornax | ||||
1199 | 07 52 25 | - 26 21.3 | 94 m | 098 - 02 | RG 610 | Kunkel / Bradt | 19 01 71 | Nebula | CTIO | |||
1200 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | J. Graham | 23 01 71 | NGC 1783 | ||||
1201 | 05 05 18 | - 69 26 | 20 m | 103a - O | nones | J. Graham | 23 01 71 | NGC 1835 | ||||
1202 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | J. Graham | 23 01 71 | NGC 1783 | ||||
1203 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | J. Graham | 23 01 71 | NGC 1835 | ||||
1204 | 00 25 42 | - 71 41 | 45 m | 103a - O | nones | J. Graham | 24 01 71 | NGC 121 | ||||
1205 | 06 30 12 | - 64 18 | 30 m | 103a - O | nones | J. Graham | 24 01 71 | NGC 2257 | ||||
1206 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | J. Graham | 24 01 71 | NGC 1783 | ||||
1207 | 05 36 00 | - 70 48 | 30 m | 103a - O | nones | J. Graham | 24 01 71 | Nova LMC | ||||
1208 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | J. Graham | 24 01 71 | NGC 1835 | ||||
1209 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | J. Graham | 24 01 71 | NGC 1783 | ||||
1210 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | J. Graham | 24 01 71 | NGC 1835 | ||||
1211 | 06 30 12 | - 64 18 | 30 m | 103a - O | nones | J. Graham | 24 01 71 | NGC 2257 | ||||
1212 | 06 20 54 | - 67 31 | 30 m | 103a - O | nones | J. Graham | 24 01 71 | NGC 2231 | ||||
1213 | 08 34 18 | - 45 04 | 10 m | 103a - O | GG 385 | J. Graham | 24 01 71 | Pulsar Field | ||||
1214 | 08 56 30 | - 28 41 | 10 m | 103a - O | GG 385 | J. Graham | 24 01 71 | K 1 - 2 | ||||
1215 | 00 25 42 | - 71 41 | 45 m | 103a - O | nones | J. Graham | 25 01 71 | NGC 121 | ||||
1216 | 04 59 00 | - 66 01 | 30 m | 103a - O | nones | J. Graham | 25 01 71 | NGC 1783 | ||||
1217 | 04 49 00 | - 68 50 | 2 m | 103a - O | nones | J. Graham | 25 01 71 | Schm plate defect | ||||
1218 | 05 05 18 | - 69 26 | 30 m | 103a - O | nones | J. Graham | 25 01 71 | NGC 1835 | ||||
1219 | 06 30 12 | - 64 18 | 30 m | 103a - O | nones | J. Graham | 25 01 71 | NGC 2257 | ||||
1220 | 06 20 54 | - 67 31 | 30 m | 103a - O | nones | J. Graham | 25 01 71 | NGC 2231 | ||||
1221 | 04 59 00 | - 66 01 | 40 m | 103a - O | nones | J. Graham | 25 01 71 | NGC 1783 | ||||
1222 | 05 05 18 | - 69 26 | 40 m | 103a - O | nones | J. Graham | 25 01 71 | NGC 1835 | ||||
1223 | 06 30 12 | - 64 18 | 40 m | 103a - O | nones | J. Graham | 25 01 71 | NGC 2257 | ||||
1224 | 08 56 30 | - 28 41 | 10 m | 103a - O | GG 385 | J. Graham | 25 01 71 | K 1 - 2 |
Last Updated on 8/27/99
By Guerra & Marin
March 1971 Plate logs for 1.5-m telescope
Plate | N. N | R . A | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1312 | al 1339 | (*) | ||||||||||
1340 | 10 26 33 | - 43 44 | 57 m | lla - O | nones | Burbigel | 25 03 71 | NGC 3256 | ||||
1341 | 12 41 39 | - 40 37 | 45 m | 103a - O | nones | Burbigel | 25 03 71 | Assoc. cent. | ||||
1342 | 12 47 13 | - 41 08.2 | 60 m | 103a - O | nones | Burbigel | 25 03 71 | NGC 4696 | ||||
1343 | 14 01 37 | - 41 16 | 60 m | 103a - O | nones | Burbigel | 25 03 71 | NGC 5408 | ||||
1344 | 18 10 42 | - 85 24 | 60 m | 103a - O | nones | Burbigel | 25 03 71 | NGC 6438 | ||||
1345 | 18 10 42 | - 85 24 | 20 m | 103a - O | nones | Burbigel | 25 03 71 | NGC 6438 | ||||
1346 | al 1350 | (*) | ||||||||||
1351 | 09 01 01 | - 40 26.4 | 72 m | 103a - O | UG 2 | Burbigel | 26 03 71 | SAO 220767 | CTIO | |||
1352 | 13 35 13 | - 33 49 | 60 m | 103a - O | nones | Burbigel | 26 03 71 | IC 4296 | ||||
1353 | 10 35 13 | - 42 45 | 60 m | 103a - D | nones | Burbigel | 26 03 71 | Klemola | ||||
1354 | 13 35 29 | - 29 43 | 5 m | 103a - O | nones | Burbigel | 26 03 71 | NGC 5236 | ||||
1355 | 13 38 17 | - 31 30 | 5 m | 103a - O | nones | Burbigel | 26 03 71 | NGC 5253 | ||||
1356 | 12 48 17 | - 41 07.3 | 60 m | 103a - D | nones | Burbigel | 26 03 71 | NGC 4696 | ||||
1357 | 14 01 56 | - 33 50 | 60 m | 103a - O | nones | Burbigel | 26 03 71 | NGC 5419 | ||||
1358 | al 1368 | (*) |
(*) corresponde a tubo imagen
Last Updated on 8/27/99
By Guerra & Marin
April 1971 Plate logs for 1.5-m telescope
Plate | N. N | R . A | Dec | Exp.Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1369 | 09 01 26 | - 40 25 | 180 m | 103a - O | U G 2 | Kunkel | 02 04 71 | Vela XR - 1 | ||||
1369 | 09 01 26 | - 40 25 | 36 m | 103a - O | GG 385 | Kunkel | 02 04 71 | Vela XR - 1 | CTIO | |||
1370a | 15 18 25 | - 57 03 | 36 m | 103a - O | GG 385 | Kunkel | 02 04 71 | Circinus X - 1 | BROKEN OK" | CTIO | ||
1370b | 15 18 25 | - 57 03 | 180 m | 103a - O | U G 2 | Kunkel | 02 04 71 | Circinus X - 1 | BROKEN OK" | CTIO | ||
1371 | 15 18 25 | - 57 03 | 36 m | 103a - O | GG 385 | Kunkel | 02 04 71 | Circinus X - 1 | CTIO | |||
1372 | 15 18 25 | - 57 03 | 36 m | 103a - O | GG 385 | Kunkel | 02 04 71 | Circinus X - 1 | CTIO | |||
1373 | 09 25 14 | - 52 42 | 45 m | lla - O | U G 2 | Bok | 03 04 71 | Vela 1 | ||||
1374 | 09 25 14 | - 52 42 | 45 m | 103a - O | U G 2 | Bok | 03 04 71 | Vela 1 | ||||
1374 | 09 25 14 | - 52 42 | 05 m | 103a - O | GG 385 | Bok | 03 04 71 | Vela 1 | ||||
1374 | 09 25 14 | - 52 42 | 08 m | 103a - O | GG 385 | Bok | 03 04 71 | Vela 1 | ||||
1374 | 09 25 14 | - 52 42 | 12 m | 103a - O | GG 385 | Bok | 03 04 71 | Vela 1 | ||||
1375 | 09 25 14 | - 52 42 | 07 m | lla - O | GG 385 | Bok | 03 04 71 | Vela 1 | ||||
1376 | 09 25 14 | - 52 42 | 10 m | 103a D | GG 495 | Bok | 03 04 71 | Vela 1 | ||||
1376 | 09 25 14 | - 52 42 | 01 m | 103a D | GG 495 | Bok | 03 04 71 | Vela 1 | ||||
1377 | 09 25 14 | - 52 42 | 45 m | 103a - O | U G 2 | Bok | 03 04 71 | Vela 1 | ||||
1377 | 09 25 14 | - 52 42 | 09 m | 103a - O | GG 385 | Bok | 03 04 71 | Vela 1 | ||||
1377 | 09 25 14 | - 52 42 | 03 m | 103a - O | GG 385 | Bok | 03 04 71 | Vela 1 | ||||
1378 | 13 26 06 | - 63 42 | 45 m | 103a - O | U G 2 | Bok | 03 04 71 | Centaurus ll | ||||
1378 | 13 26 06 | - 63 42 | 09 m | 103a - O | GG 385 | Bok | 03 04 71 | Centaurus ll | ||||
1378 | 13 26 06 | - 63 42 | 03 m | 103a - O | GG 385 | Bok | 03 04 71 | Centaurus ll | ||||
1379 | 13 26 06 | - 63 42 | 07 m | lla - O | GG 385 | Bok | 03 04 71 | Centaurus ll | ||||
1380 | 13 26 06 | - 63 42 | 10 m | 103a D | GG 495 | Bok | 03 04 71 | Centaurus ll | ||||
1381 | 15 23 48 | - 59 27 | 45 m | 103a - O | U G 2 | Bok | 03 04 71 | Circinus | ||||
1381 | 15 23 48 | - 59 27 | 06 m | 103a - O | GG 385 | Bok | 03 04 71 | Circinus | ||||
1381 | 15 23 48 | - 59 27 | 10 m | 103a - O | GG 385 | Bok | 03 04 71 | Circinus | ||||
1382 | 15 23 48 | - 59 27 | 07 m | lla - O | GG 385 | Bok | 03 04 71 | Circinus | ||||
1382 | 15 23 48 | - 59 27 | 45 seg | lla - O | GG 385 | Bok | 03 04 71 | Circinus | ||||
1383 | 15 23 48 | - 59 27 | 10 m | 103a D | GG 495 | Bok | 03 04 71 | Circinus | ||||
1384 | 09 25 39 | - 52 42 | 10 m | 103a D | GG 495 | Bok | 04 04 71 | Vela 1 | ||||
1384 | 09 25 39 | - 52 42 | 01 m | 103a D | GG 495 | 3 | Bok | 04 04 71 | Vela 1 | |||
1385 | 09 25 39 | - 52 42 | 10 m | lla - O | GG 385 | 3 | Bok | 04 04 71 | Vela 1 | |||
1385 | 09 25 39 | - 52 42 | 01 m | lla - O | GG 385 | 2.5 | Bok | 04 04 71 | Vela 1 | |||
1386 | 09 25 39 | - 52 42 | 20 m | lla - O | U G 2 | 3 | Bok | 04 04 71 | Vela 1 | |||
1386 | 09 25 39 | - 52 42 | 04 m | lla - O | GG 385 | 3 | Bok | 04 04 71 | Vela 1 | |||
1386 | 09 25 39 | - 52 42 | 02 m | lla - O | GG 385 | 4 | Bok | 04 04 71 | Vela 1 | |||
1387 | 09 25 39 | - 52 42 | 50 m | lla - O | U G 2 | 5 | Bok | 04 04 71 | Vela 1 | |||
1387 | 09 25 39 | - 52 42 | 05 m | lla - O | U G 2 | 4 | Bok | 04 04 71 | Vela 1 | |||
1388 | 09 25 39 | - 52 42 | 50 m | lla - O | U G 2 | 4 | Bok | 04 04 71 | Vela 1 | |||
1388 | 09 25 39 | - 52 42 | 15 m | lla - O | GG 385 | ´4 - 10 | Bok | 04 04 71 | Vela 1 | |||
1388 | 09 25 39 | - 52 42 | 07 m | lla - O | GG 385 | ´4 - 10 | Bok | 04 04 71 | Vela 1 | |||
1389 | 13 27 18 | - 63 42 | 10 m | lla - O | GG 385 | ´4 - 10 | Bok | 04 04 71 | Centaurus ll | |||
1389 | 13 27 18 | - 63 42 | 01 m | lla - O | GG 385 | ´4 - 10 | Bok | 04 04 71 | Centaurus ll | |||
1390 | 13 27 18 | - 63 42 | 10 m | 103a - D | GG 495 | ´4 - 10 | Bok | 04 04 71 | Centaurus ll | |||
1390 | 13 27 18 | - 63 42 | 01 m | 103a - D | GG 495 | 2 | Bok | 04 04 71 | Centaurus ll | |||
1391 | 13 27 18 | - 63 42 | 20 m | lla - O | U G 2 | 2 | Bok | 04 04 71 | Centaurus ll | |||
1391 | 13 27 18 | - 63 42 | 04 m | lla - O | GG 385 | 2 | Bok | 04 04 71 | Centaurus ll | |||
1391 | 13 27 18 | - 63 42 | 02 m | lla - O | GG 385 | 2.5 | Bok | 04 04 71 | Centaurus ll | |||
1392 | 13 27 18 | - 63 42 | 60 m | lla - O | U G 2 | 2.5 | Bok | 04 04 71 | Centaurus ll | |||
1392 | 13 27 18 | - 63 42 | 12 m | lla - O | GG 385 | 4 | Bok | 04 04 71 | Centaurus ll | |||
1392 | 13 27 18 | - 63 42 | 06 m | lla - O | GG 385 | 3 | Bok | 04 04 71 | Centaurus ll | |||
1393 | 15 18 25 | - 57 03 | 36 m | 103a - O | GG 385 | 3 | Bok | 04 04 71 | Circinus X - 1 | BROKEN OK" | CTIO | |
1394 | 15 23 43 | - 59 25 | 60 m | lla - O | U G 2 | 3 | Bok | 04 04 71 | Circinus | |||
1394 | 15 23 43 | - 59 25 | 10 m | lla - O | GG 385 | 3 | Bok | 04 04 71 | Circinus | |||
1395 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 3 | Bok | 05 04 71 | HD 95540 | |||
1395 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 4 | Bok | 05 04 71 | HD 95540 | |||
1396 | 10 58 48 | - 60 17 | 10 m | lla - O | GG 385 | 4 | Bok | 05 04 71 | HD 95540 | |||
1396 | 10 58 48 | - 60 17 | 01 m | lla - O | GG 385 | 4 | Bok | 05 04 71 | HD 95540 | |||
1397 | 10 58 48 | - 60 17 | 20 m | lla - O | U G 2 | 4 | Bok | 05 04 71 | HD 95540 | |||
1397 | 10 58 48 | - 60 17 | 05 m | lla - O | GG 385 | 4 | Bok | 05 04 71 | HD 95540 | |||
1397 | 10 58 48 | - 60 17 | 02 m | lla - O | GG 385 | 3 | Bok | 05 04 71 | HD 95540 | |||
1398 | 10 58 48 | - 60 17 | 10 m | lla - O | GG 385 | 3 | Bok | 05 04 71 | HD 95540 | |||
1398 | 10 58 48 | - 60 17 | 01 m | lla - O | GG 385 | 3 | Bok | 05 04 71 | HD 95540 | |||
1399 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 2 | Bok | 05 04 71 | HD 95540 | |||
1399 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 2 | Bok | 05 04 71 | HD 95540 | |||
1400 | 10 58 48 | - 60 17 | 60 m | lla - O | U G 2 | 2 | Bok | 05 04 71 | HD 95540 | |||
1400 | 10 58 48 | - 60 17 | 06 m | lla - O | U G 2 | 1.5 | Bok | 05 04 71 | HD 95540 | |||
1401 | 10 58 48 | - 60 17 | 60 m | lla - O | U G 2 | 1.5 | Bok | 05 04 71 | HD 95540 | |||
1401 | 10 58 48 | - 60 17 | 06 m | lla - O | U G 2 | 3 | Bok | 05 04 71 | HD 95540 | |||
1402 | 10 58 48 | - 60 17 | 60 m | lla - O | U G 2 | 1.5 | Bok | 05 04 71 | HD 95540 | |||
1402 | 10 58 48 | - 60 17 | 12 m | lla - O | GG 385 | 1.5 | Bok | 05 04 71 | HD 95540 | |||
1402 | 10 58 48 | - 60 17 | 01 m | lla - O | GG 385 | 1.5 | Bok | 05 04 71 | HD 95540 | |||
1403 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 05 04 71 | HD 95540 | |||
1403 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 1.5 | Bok | 05 04 71 | HD 95540 | |||
1404 | 15 18 25 | - 57 03 | 36 m | 103a - O | GG 385 | 3 | Bok | 05 04 71 | Circinus X - 1 | BROKEN OK" | CTIO | |
1405 | 15 23 43 | - 59 25 | 60 m | lla - O | U G 2 | 2.5 | Bok | 05 04 71 | Circinus | |||
1405 | 15 23 43 | - 59 25 | 12 m | lla - O | GG 385 | 2.5 | Bok | 05 04 71 | Circinus | |||
1405 | 15 23 43 | - 59 25 | 01 m | lla - O | GG 385 | 2.5 | Bok | 05 04 71 | Circinus | |||
1406 | 09 26 36 | - 52 50 | 60 m | lla - O | U G 2 | 4 | Bok | 06 04 71 | Vela 1 | |||
1406 | 09 26 36 | - 52 50 | 07 m | lla - O | GG 385 | 4 | Bok | 06 04 71 | Vela 1 | |||
1406 | 09 26 36 | - 52 50 | 02 m | lla - O | GG 385 | 4 | Bok | 06 04 71 | Vela 1 | |||
1407 | 09 26 36 | - 52 50 | 10 m | 103a - D | GG 495 | 4 | Bok | 06 04 71 | Vela 1 | |||
1407 | 09 26 36 | - 52 50 | 01 m | 103a - D | GG 495 | 4 | Bok | 06 04 71 | Vela 1 | |||
1408 | 10 58 48 | - 60 17 | 20 m | lla - O | U G 2 | 4 | Bok | 06 04 71 | HD 95540 | |||
1408 | 10 58 48 | - 60 17 | 20 m | lla - O | U G 2 | 4 | Bok | 06 04 71 | HD 95540 | |||
1408 | 10 58 48 | - 60 17 | 2.5 m | lla - O | GG 385 | 3 | Bok | 06 04 71 | HD 95540 | |||
1408 | 10 58 48 | - 60 17 | 2.5 m | lla - O | GG 385 | 1.5 | Bok | 06 04 71 | HD 95540 | |||
1408 | 10 58 48 | - 60 17 | 30 seg | lla - O | GG 385 | 1.5 | Bok | 06 04 71 | HD 95540 | |||
1409 | 10 58 48 | - 60 17 | 10 m | lla - O | GG 385 | 1.5 | Bok | 06 04 71 | HD 95540 | |||
1409 | 10 58 48 | - 60 17 | 01 m | lla - O | GG 385 | 2 | Bok | 06 04 71 | HD 95540 | |||
1410 | 10 58 48 | - 60 17 | 20 m | lla - O | U G 2 | 2 | Bok | 06 04 71 | HD 95540 | |||
1410 | 10 58 48 | - 60 17 | 2.5 m | lla - O | GG 385 | 1.5 | Bok | 06 04 71 | HD 95540 | |||
1410 | 10 58 48 | - 60 17 | 30 seg | lla - O | GG 385 | 1.5 | Bok | 06 04 71 | HD 95540 | |||
1411 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 06 04 71 | HD 95540 | |||
1411 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 1.5 | Bok | 06 04 71 | HD 95540 | |||
1412 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 3.5 | Bok | 06 04 71 | HD 95540 | |||
1412 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 2 | Bok | 06 04 71 | HD 95540 | |||
1413 | 13 26 06 | - 63 42 | 60 m | lla - O | U G 2 | 2 | Bok | 06 04 71 | Centaurus ll | |||
1413 | 13 26 06 | - 63 42 | 7.5 m | lla - O | GG 385 | 2 | Bok | 06 04 71 | Centaurus ll | |||
1413 | 13 26 06 | - 63 42 | 02 m | lla - O | GG 385 | 2 | Bok | 06 04 71 | Centaurus ll | |||
1414 | 13 26 06 | - 63 42 | 60 m | lla - O | U G 2 | 2 | Bok | 06 04 71 | Centaurus ll | |||
1414 | 13 26 06 | - 63 42 | 06 m | lla - O | U G 2 | 4 | Bok | 06 04 71 | Centaurus ll | |||
1415 | 13 26 06 | - 63 42 | 10 m | 103a - D | GG 495 | 4 | Bok | 06 04 71 | Centaurus ll | |||
1415 | 13 26 06 | - 63 42 | 01 m | 103a - D | GG 495 | 4 | Bok | 06 04 71 | Centaurus ll | |||
1416 | 15 18 25 | - 57 03 | 36 m | 103a - O | GG 385 | 4 | Bok | 06 04 71 | Centaurus ll | CTIO | ||
1417 | 15 55 30 | - 54 16 | 20 m | lla - O | U G 2 | 4 | Bok | 06 04 71 | Norma l | |||
1417 | 15 55 30 | - 54 16 | 03 m | lla - O | GG 385 | 4 | Bok | 06 04 71 | Norma l | |||
1417 | 15 55 30 | - 54 16 | 40 seg | lla - O | GG 385 | 4 | Bok | 06 04 71 | Norma l | |||
1418 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 3 | Bok | 07 04 71 | HD 95540 | |||
1418 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 3 | Bok | 07 04 71 | HD 95540 | |||
1419 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 2 | Bok | 07 04 71 | HD 95540 | |||
1419 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 2 | Bok | 07 04 71 | HD 95540 | |||
1420 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 07 04 71 | HD 95540 | |||
1420 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 1.5 | Bok | 07 04 71 | HD 95540 | |||
1421 | 15 18 25 | - 57 03 | 12 m | 103a - O | GG 385 | 2 | Bok | 07 04 71 | Cir. XR - 1 | |||
1421 | 15 18 25 | - 57 03 | 12 m | 103a - O | GG 385 | 2 | Bok | 07 04 71 | Cir. XR - 1 | |||
1421 | 15 18 25 | - 57 03 | 12 m | 103a - O | GG 385 | 2 | Bok | 07 04 71 | Cir. XR - 1 | CTIO | ||
1421 | 15 18 25 | - 57 03 | 12 m | 103a - O | GG 385 | 2 | Bok | 07 04 71 | Cir. XR - 1 | |||
1421 | 15 18 25 | - 57 03 | 12 m | 103a - O | GG 385 | 2 | Bok | 07 04 71 | Cir. XR - 1 | |||
1422 | 15 24 42 | - 59 33 | 20 m | lla - O | U G 2 | 2 | Bok | 07 04 71 | Circinus | |||
1422 | 15 24 42 | - 59 33 | 2.5 m | lla - O | GG 385 | 2 | Bok | 07 04 71 | Circinus | |||
1422 | 15 24 42 | - 59 33 | 30 seg | lla - O | GG 385 | 2 | Bok | 07 04 71 | Circinus | |||
1423 | 15 55 24 | - 54 15.8 | 50 m | lla - O | U G 2 | 3 | Bok | 07 04 71 | Norma l | |||
1423 | 15 55 24 | - 54 15.8 | 06 m | lla - O | GG 385 | 3 | Bok | 07 04 71 | Norma l | |||
1423 | 15 55 24 | - 54 15.8 | 01 m | lla - O | GG 385 | 3 | Bok | 07 04 71 | Norma l | |||
1424 | 10 58 48 | - 60 17 | 10 m | 103a - D | GG 495 | 2 | Bok | 08 04 71 | HD 95540 | |||
1424 | 10 58 48 | - 60 17 | 01 m | 103a - D | GG 495 | 2 | Bok | 08 04 71 | HD 95540 | |||
1425 | 11 30 12 | - 60 31 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1425 | 11 30 12 | - 60 31 | 01 m | 103a - D | GG 495 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1426 | 11 30 12 | - 60 31 | 10 m | lla - O | GG 385 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1426 | 11 30 12 | - 60 31 | 01 m | lla - O | GG 385 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1427 | 11 30 12 | - 60 31 | 60 m | lla - O | U G 2 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1427 | 11 30 12 | - 60 31 | 07.5 m | lla - O | GG 385 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1427 | 11 30 12 | - 60 31 | 01.5 m | lla - O | GG 385 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1428 | 11 30 12 | - 60 31 | 20 m | lla - O | U G 2 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1428 | 11 30 12 | - 60 31 | 02.5 m | lla - O | GG 385 | 1.5 | Bok | 08 04 71 | SA 193 | |||
1428 | 11 30 12 | - 60 31 | 30 seg | lla - O | GG 385 | 3 | Bok | 08 04 71 | SA 193 | |||
1429 | 15 24 42 | - 59 33 | 10 m | 103a - D | GG 495 | 3 | Bok | 08 04 71 | Circinus | |||
1429 | 15 24 42 | - 59 33 | 01 m | 103a - D | GG 495 | 3 | Bok | 08 04 71 | Circinus | |||
1430 | 15 24 42 | - 59 33 | 20 m | lla - O | U G 2 | 3 | Bok | 08 04 71 | Circinus | |||
1430 | 15 24 42 | - 59 33 | 02.5 m | lla - O | GG 385 | 3 | Bok | 08 04 71 | Circinus | |||
1430 | 15 24 42 | - 59 33 | 30 m | lla - O | GG 385 | 3 | Bok | 08 04 71 | Circinus | |||
1431 | 15 55 24 | - 54 15.8 | 60 m | lla - O | U G 2 | 3 | Bok | 08 04 71 | Norma l | |||
1431 | 15 55 24 | - 54 15.8 | 60 m | lla - O | U G 2 | 3 | Bok | 08 04 71 | Norma l | |||
1432 | 15 55 24 | - 54 15.8 | 20 m | lla - O | U G 2 | 2 | Bok | 08 04 71 | Norma l | |||
1432 | 15 55 24 | - 54 15.8 | 02.5 m | lla - O | GG 385 | 2 | Bok | 08 04 71 | Norma l | |||
1432 | 15 55 24 | - 54 15.8 | 30 seg | lla - O | GG 385 | 2 | Bok | 08 04 71 | Norma l | |||
1433 | 15 55 24 | - 54 15.8 | 10 m | 103a - D | GG 495 | 3 | Bok | 08 04 71 | Norma l | |||
1433 | 15 55 24 | - 54 15.8 | 01 m | 103a - D | GG 495 | 3 | Bok | 08 04 71 | Norma l | |||
1434 | 15 55 24 | - 54 15.8 | 10 m | lla - O | GG 385 | 3 | Bok | 08 04 71 | Norma l | |||
1434 | 15 55 24 | - 54 15.8 | 01 m | lla - O | GG 385 | 3 | Bok | 08 04 71 | Norma l | |||
1435 | 15 55 24 | - 54 15.8 | 10 m | 103a - D | GG 495 | 3 | Bok | 08 04 71 | Norma l | |||
1435 | 15 55 24 | - 54 15.8 | 01 m | 103a - D | GG 495 | 2.5 | Bok | 08 04 71 | Norma l | |||
1436 | 09 40 00 | - 54 00 | 20 m | lla - O | U G 2 | 2.5 | Bok | 09 04 71 | Vela 2 | |||
1436 | 09 40 00 | - 54 00 | 02.5 m | lla - O | GG 385 | 1.5 | Bok | 09 04 71 | Vela 2 | |||
1436 | 09 40 00 | - 54 00 | 30 seg | lla - O | GG 385 | 1.5 | Bok | 09 04 71 | Vela 2 | |||
1437 | 09 40 00 | - 54 00 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | Vela 2 | |||
1437 | 09 40 00 | - 54 00 | 01 m | 103a - D | GG 495 | 2 | Bok | 09 04 71 | Vela 2 | |||
1438 | 09 40 00 | - 54 00 | 10 m | lla - O | GG 385 | 3.5 | Bok | 09 04 71 | Vela 2 | |||
1438 | 09 40 00 | - 54 00 | 01 m | lla - O | GG 385 | 1.5 - 3 | Bok | 09 04 71 | Vela 2 | |||
1439 | 09 40 00 | - 54 00 | 60 m | lla - O | U G 2 | 1.5 - 3 | Bok | 09 04 71 | Vela 2 | |||
1439 | 09 40 00 | - 54 00 | 07.5 m | lla - O | GG 385 | 2.5 | Bok | 09 04 71 | Vela 2 | |||
1439 | 09 40 00 | - 54 00 | 01.5 m | lla - O | GG 385 | 2 | Bok | 09 04 71 | Vela 2 | |||
1440 | 09 40 00 | - 54 00 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | Vela 2 | |||
1440 | 09 40 00 | - 54 00 | 01 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | Vela 2 | |||
1441 | 11 30 12 | - 60 31 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | SA 193 | |||
1441 | 11 30 12 | - 60 31 | 01 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | SA 193 | |||
1442 | 15 24 42 | - 59 33 | 10 m | 103a - D | GG 495 | 1 | Bok | 09 04 71 | Circinus | |||
1442 | 15 24 42 | - 59 33 | 01 m | 103a - D | GG 495 | 1 | Bok | 09 04 71 | Circinus | |||
1443 | 16 22 54 | - 52 06 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1443 | 16 22 54 | - 52 06 | 01 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1444 | 16 22 54 | - 52 06 | 10 m | lla - O | GG 385 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1444 | 16 22 54 | - 52 06 | 01 m | lla - O | GG 385 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1445 | 16 22 54 | - 52 06 | 20 m | lla - O | U G 2 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1445 | 16 22 54 | - 52 06 | 02.5 m | lla - O | GG 385 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1445 | 16 22 54 | - 52 06 | 30 seg | lla - O | GG 385 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1446 | 16 22 54 | - 52 06 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1446 | 16 22 54 | - 52 06 | 1 m | 103a - D | GG 495 | 1.5 | Bok | 09 04 71 | Norma lV | |||
1447 | 16 22 54 | - 52 06 | 60 m | lla - O | U G 2 | 2 | Bok | 09 04 71 | Norma lV | |||
1447 | 16 22 54 | - 52 06 | 07.5 m | lla - O | GG 385 | 2 | Bok | 09 04 71 | Norma lV | |||
1447 | 16 22 54 | - 52 06 | 1.5 m | lla - O | GG 385 | 2 | Bok | 09 04 71 | Norma lV | |||
1448 | 14 18 18 | - 60 47 | 10 m | lla - O | GG 385 | 5 | Bok | 15 04 71 | Centaurus | |||
1448 | 14 18 18 | - 60 47 | 1 m | lla - O | GG 385 | 5 | Bok | 15 04 71 | Centaurus | |||
1449 | 14 18 18 | - 60 47 | 15 m | 103a - D | GG 495 | 6 | Bok | 15 04 71 | Centaurus | |||
1449 | 14 18 18 | - 60 47 | 1.5 m | 103a - D | GG 495 | 6 | Bok | 15 04 71 | Centaurus | |||
1450 | 14 18 18 | - 60 47 | 30 m | lla - O | U G 2 | 4 | Bok | 15 04 71 | Centaurus | |||
1450 | 14 18 18 | - 60 47 | 4 m | lla - O | GG 385 | 4 | Bok | 15 04 71 | Centaurus | |||
1450 | 14 18 18 | - 60 47 | 45 seg | lla - O | GG 385 | 6 | Bok | 15 04 71 | Centaurus | |||
1451 | 14 18 18 | - 60 47 | 75 m | lla - O | U G 2 | 4--6 | Bok | 15 04 71 | Centaurus | |||
1451 | 14 18 18 | - 60 47 | 2.5 m | lla - O | U G 2 | 4--6 | Bok | 15 04 71 | Centaurus | |||
1452 | 15 49 42 | - 56 16 | 15 m | 103a - D | GG 495 | 4--8 | Bok | 15 04 71 | Norma ll | |||
1452 | 15 49 42 | - 56 16 | 1.5 m | 103a - D | GG 495 | 4--8 | Bok | 15 04 71 | Norma ll | |||
1453 | 15 49 42 | - 56 16 | 12 m | lla - O | GG 385 | 3.5 | Bok | 15 04 71 | Norma ll | |||
1453 | 15 49 42 | - 56 16 | 1 m | lla - O | GG 385 | 3.5 | Bok | 15 04 71 | Norma ll | |||
1454 | 15 49 42 | - 56 16 | 60 m | lla - O | U G 2 | 3 | Bok | 15 04 71 | Norma ll | |||
1454 | 15 49 42 | - 56 16 | 6 m | lla - O | U G 2 | 6 | Bok | 15 04 71 | Norma ll | |||
1455 | 09 40 00 | - 53 57 | 75 m | lla - O | U G 2 | 8--10 | Bok | 15 04 71 | Vela ll | |||
1455 | 09 40 00 | - 53 57 | 7.5 m | lla - O | U G 2 | 12 | Bok | 15 04 71 | Vela ll | |||
1456 | 12 56 00 | - 61 30 | 75 m | lla - O | GG 385 | 3.5 | Bok | 16 04 71 | Saco de Carbon a | |||
1457 | 13 15 00 | - 61 30 | 75 m | lla - O | GG 385 | 4 | Bok | 16 04 71 | Saco de Carbon b | |||
1458 | 14 18 18 | - 60 47 | 60 m | lla - O | U G 2 | 3.5 | Bok | 16 04 71 | Centaurus l | |||
1458 | 14 18 18 | - 60 47 | 7.5 m | lla - O | GG 385 | 3.5 | Bok | 16 04 71 | Centaurus l | |||
1458 | 14 18 18 | - 60 47 | 1 5 m | lla - O | GG 385 | 3.5 | Bok | 16 04 71 | Centaurus l | |||
1459 | 16 23 24 | - 51 59.2 | 60 m | lla - O | U G 2 | 3 | Bok | 16 04 71 | Norma lV | |||
1459 | 16 23 24 | - 51 59.2 | 6 m | lla - O | U G 2 | 3 | Bok | 16 04 71 | Norma lV | |||
1460 | 11 30 12 | - 60 31 | 60 m | lla - O | U G 2 | 1 | Bok | 16 04 71 | SA 193 | |||
1460 | 11 30 12 | - 60 31 | 07.5 m | lla - O | GG 385 | 1.5 | Bok | 16 04 71 | SA 193 | |||
1460 | 11 30 12 | - 60 31 | 01.5 m | lla - O | GG 385 | 1.5 | Bok | 16 04 71 | SA 193 | |||
1460 | 11 30 12 | - 60 31 | 6 m | lla - O | U G 2 | 1.5 | Bok | 16 04 71 | SA 193 | |||
1461 | 12 56 00 | - 61 30 | 90 m | 098 - 0 2 | RG - 610 | 1.5 | Bok | 16 04 71 | Coal Sack a | |||
1462 | 13 15 00 | -61 29.7 | 90 m | 098 - 0 2 | RG - 610 | 1.5 | Bok | 17 04 71 | Coal Sack b | |||
1463 | 13 15 00 | -61 29.7 | 30 m | 103a - D | GG 495 | 1.5 | Bok | 17 04 71 | Coal Sack b | |||
1464 | 12 56 00 | - 61 30 | 30 m | 103a - D | GG 495 | 1 | Bok | 17 04 71 | Coal Sack a | |||
1465 | 14 18 18 | - 60 47 | 10 m | lla - O | GG 385 | 1.5 | Bok | 17 04 71 | Centaurus l | |||
1465 | 14 18 18 | - 60 47 | 01 m | lla - O | GG 385 | 1.5 | Bok | 17 04 71 | Centaurus l | |||
1466 | 15 49 42 | - 56 16 | 60 m | lla - O | U G 2 | 1.5 | Bok | 17 04 71 | Norma ll | |||
1466 | 15 49 42 | - 56 16 | 7.5 m | lla - O | GG 385 | 1.5 | Bok | 17 04 71 | Norma ll | |||
1466 | 15 49 42 | - 56 16 | 1.5 m | lla - O | GG 385 | 1.5 | Bok | 17 04 71 | Norma ll | |||
1466 | 15 49 42 | - 56 16 | 6 m | lla - O | U G 2 | 1.5 | Bok | 17 04 71 | Norma ll | |||
1467 | 15 49 42 | - 56 16 | 10 m | 103a - D | GG 495 | 1.5 | Bok | 17 04 71 | Norma ll | |||
1467 | 15 49 42 | - 56 16 | 01 m | 103a - D | GG 495 | 1.5 | Bok | 17 04 71 | Norma ll | |||
1468 | 15 49 42 | - 56 16 | 10 m | lla - O | GG 385 | 1.5 | Bok | 17 04 71 | Norma ll | |||
1468 | 15 49 42 | - 56 16 | 01 m | lla - O | GG 385 | 1.5 | Bok | 17 04 71 | Norma ll |
Last Updated on 8/27/99
By Jorge Marin
May 1971 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1469 | 08 25 18 | - 68 01 | 5 m | 103a - O | NO | 4--5 | Rubin, Smith | 01 05 71 | NGC 2601 | |||
1470 | 08 25 18 | - 68 01 | 60 m | 103a - O | NO | 4--5 | Rubin, Smith | 01 05 71 | NGC 2601 | |||
1471 | 08 25 18 | - 68 01 | 5 m | 103a - O | NO | 4--5 | Rubin, Smith | 01 05 71 | NGC 2601 | |||
1472 | 09 58 48 | - 31 24 | 5 m | 103a - O | NO | 2--3 | Rubin, Smith | 01 05 71 | NGC 3095 | |||
1473 | Focus | plate | Rubin, Smith | 01 05 71 | Focus Plate | |||||||
1474 | 11 52 30 | - 23 01 | 20 m | 103a - O | NO | 1 | Rubin, Smith | 01 05 71 | NGC 3955 | |||
1475 | 17 16 18 | - 39 17.5 | 60 m | 103a - O | NO | 1--2 | Rubin, Smith | 01 05 71 | H 2 - 6 | |||
1476 | 17 16 18 | - 39 17.5 | 20 m | 103a - O | NO | 2--3 | Rubin, Smith | 01 05 71 | H 2 - 6 | |||
1477 | 17 16 18 | - 39 17.5 | 44 m | 098 - 0 2 | RG - 610 | 2--3 | Rubin, Smith | 01 05 71 | H 2 - 6 | |||
1478 | 17 16 18 | - 39 17.5 | 60 m | 098 - 0 2 | RG - 610 | 3 | Rubin, Smith | 01 05 71 | H 2 - 6 | |||
1479 | 17 07 24 | - 41 33.9 | 60 m | 098 - 0 2 | RG - 610 | 3--4 | Rubin, Smith | 01 05 71 | M 2 | |||
1480 | 10 44 00 | - 59 33 | 60 m | 098 - 02 | RG - 610 | 2 | Blanco | 23 05 71 | Eta Carina | BROKEN OK" | CTIO | |
1481 | 13 04 06 | - 49 21 | 120 m | 103a - O | NO | 2 | Blanco | 23 05 71 | NGC 4945 | CTIO | ||
1482 | 12 52 06 | - 60 13 | 30 m | 103a - O | GG 385 | 3--2 | Landolt | 25 05 71 | K Crusis/ NGC 4755 | |||
1483 | 12 52 06 | - 60 13 | 30 m | 103a - D | GG 495 | 3--2 | Landolt | 25 05 71 | K Crusis/ NGC 4755 | |||
1484 | 13 36 36 | - 00 31.2 | 5 m | 103a - D | GG 495 | 3--2 | Landolt | 25 05 71 | SA 105 | |||
1485 | 12 33 00 | - 72 24 | 30 m | 103a - D | GG 495 | 3--2 | Landolt | 25 05 71 | NGC 4372 | |||
1486 | 12 33 00 | - 72 24 | 30 m | 103a - O | GG 385 | 3--2 | Landolt | 25 05 71 | NGC 4372 | |||
1487 | 16 21 48 | - 26 27 | 30 m | 103a - O | GG 385 | 3--2 | Landolt | 25 05 71 | NGC 6121 | |||
1488 | 16 21 48 | - 26 27 | 30 m | 103a - D | GG 495 | 3--2 | Landolt | 25 05 71 | NGC 6121 | |||
1489 | 16 21 48 | - 26 27 | 60 m | 103a - O | U G 2 | 3--2 | Landolt | 25 05 71 | NGC 6121 | |||
1490 | 16 21 48 | - 26 27 | 83 m | 103a - O | U G 2 | 3--2 | Landolt | 25 05 71 | NGC 6121 | |||
1491 | 12 52 30 | - 60 13 | 10 m | 103a - O | GG 385 | 3--2 | Landolt | 26 05 71 | K Crusis/ NGC 4755 | |||
1492 | 12 52 30 | - 60 13 | 30 m | 103a - O | GG 385 | 3--2 | Landolt | 26 05 71 | K Crusis/ NGC 4755 | |||
1493 | 12 52 30 | - 60 13 | 60 m | 103a - O | U G 2 | 3--2 | Landolt | 26 05 71 | K Crusis/ NGC 4755 | |||
1494 | 16 21 48 | - 26 27 | 60 m | 103a - O | U G 2 | 2.5 | Landolt | 26 05 71 | NGC 6121 | |||
1495 | 16 21 48 | - 26 27 | 30 m | 103a - O | U G 2 | 2.5 | Landolt | 26 05 71 | NGC 6121 | |||
1496 | 16 21 48 | - 26 27 | 12 m | 103a - O | GG 385 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1497 | 16 21 48 | - 26 27 | 12 m | 103a - O | GG 385 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1498 | 16 21 48 | - 26 27 | 12 m | 103a - O | GG 385 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1499 | 16 21 48 | - 26 27 | 60 m | 103a - D | GG 495 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1500 | 16 21 48 | - 26 27 | 15 m | 103a - D | GG 495 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1501 | 16 21 48 | - 26 27 | 15 m | 103a - D | GG 495 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1502 | 16 21 48 | - 26 27 | 15 m | 103a - D | GG 495 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1503 | 16 21 48 | - 26 27 | 30 m | 103a - D | GG 495 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1504 | 16 21 48 | - 26 27 | 12 m | 103a - O | GG 385 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1505 | 16 21 48 | - 26 27 | 30 m | 103a - D | GG 495 | 3.5 | Landolt | 26 05 71 | NGC 6121 | |||
1506 | 17 48 30 | - 37 02 | 30 m | 103a - D | GG 495 | 3.5 | Landolt | 26 05 71 | NGC 6441 | |||
1507 | 17 48 30 | - 37 02 | 15 m | 103a - O | GG 385 | 3.5 | Landolt | 26 05 71 | NGC 6441 | |||
1508 | 13 36 36 | - 00 31.2 | 5 m | 103a - D | GG 495 | 3 | Landolt | 27 05 71 | SA 105 | |||
1509 | 12 52 30 | - 60 13 | 30 m | 103a - D | GG 495 | 3 | Landolt | 27 05 71 | K Crusis/ NGC 4755 | |||
1510 | 12 52 30 | - 60 13 | 30 m | 103a - O | U G 2 | 3 | Landolt | 27 05 71 | K Crusis/ NGC 4755 | |||
1511 | 12 52 30 | - 60 13 | 30 m | 103a - O | U G 2 | 1.5 | Landolt | 27 05 71 | K Crusis/ NGC 4755 | |||
1512 | 12 52 30 | - 60 13 | 50 m | 103a - D | GG 495 | 3 | Landolt | 27 05 71 | K Crusis/ NGC 4755 | |||
1513 | 16 21 48 | - 26 27 | 60 m | 103a - D | GG 495 | 3 | Landolt | 27 05 71 | NGC 6121 | |||
1514 | 16 21 48 | - 26 27 | 60 m | 103a - D | GG 495 | 3 | Landolt | 27 05 71 | NGC 6121 | |||
1515 | 16 21 48 | - 26 27 | 30 m | 103a - O | GG 385 | 3 | Landolt | 27 05 71 | NGC 6121 | |||
1516 | 16 21 48 | - 26 27 | 30 m | 103a - O | GG 385 | 2--4 | Landolt | 27 05 71 | NGC 6121 | |||
1517 | 16 21 48 | - 26 27 | 60 m | 103a - O | GG 385 | 2--4 | Landolt | 27 05 71 | NGC 6121 | |||
1518 | 16 21 48 | - 26 27 | 60 | 103a - O | GG 385 | 3 | Landolt | 27 05 71 | NGC 6121 | |||
1519 | 16 21 48 | - 26 27 | 30 m | 103a - O | U G 2 | 3 | Landolt | 27 05 71 | NGC 6121 | |||
1520 | 16 21 48 | - 26 27 | 30 m | 103a - O | U G 2 | 3 | Landolt | 27 05 71 | NGC 6121 | |||
1521 | 17 48 30 | - 37 02 | 15 m | 103a - O | GG 385 | 3 | Landolt | 27 05 71 | NGC 6441 | |||
1522 | 17 48 30 | - 37 02 | 30 m | 103a - D | GG 495 | 3 | Landolt | 27 05 71 | NGC 6441 | |||
1523 | 12 52 30 | - 60 13 | 60 m | 103a - O | U G 2 | 3 | Landolt | 31 05 71 | NGC 4755 | |||
1524 | 12 52 30 | - 60 13 | 15 m | 103a - O | U G 2 | 3 | Landolt | 31 05 71 | NGC 4755 | |||
1525 | 12 52 30 | - 60 13 | 15 m | 103a - O | U G 2 | 3 | Landolt | 31 05 71 | NGC 4755 | |||
1526 | 12 52 30 | - 60 13 | 6 m | 103a - O | U G 2 | 3 | Landolt | 31 05 71 | NGC 4755 | |||
1527 | 12 52 30 | - 60 13 | 6 m | 103a - O | U G 2 | 3 | Landolt | 31 05 71 | NGC 4755 | |||
1528 | 12 52 30 | - 60 13 | 10 m | 103a - O | GG 385 | 3 | Landolt | 31 05 71 | NGC 4755 | |||
1529 | 12 52 30 | - 60 13 | 4 m | 103a - O | GG 385 | 3 | Landolt | 31 05 71 | NGC 4755 | |||
1530 | 12 52 30 | - 60 13 | 4 m | 103a - O | GG 385 | 3 | Landolt | 31 05 71 | NGC 4755 | |||
1531 | 12 52 30 | - 60 13 | 10 m | 103a - D | GG 495 | 4 | Landolt | 31 05 71 | NGC 4755 | |||
1532 | 12 52 30 | - 60 13 | 10 m | 103a - D | GG 495 | 4 | Landolt | 31 05 71 | NGC 4755 | |||
1533 | 12 52 30 | - 60 13 | 50 m | 103a - D | GG 495 | 4 | Landolt | 31 05 71 | NGC 4755 | |||
1534 | 12 52 30 | - 60 13 | 4 m | 103a - D | GG 495 | 4 | Landolt | 31 05 71 | NGC 4755 | |||
1535 | 12 52 30 | - 60 13 | 4 m | 103a - D | GG 495 | 4 | Landolt | 31 05 71 | NGC 4755 | |||
1536 | 12 52 30 | - 60 13 | 50 m | 103a - O | GG 385 | 4 | Landolt | 31 05 71 | NGC 4755 | |||
1537 | 12 52 30 | - 60 13 | 50 m | 103a - O | GG 385 | 4--6 | Landolt | 31 05 71 | NGC 4755 | |||
1538 | 16 21 48 | - 26 27 | 60 m | 103a - O | GG 385 | 4 | Landolt | 31 05 71 | NGC 6121 | |||
1539 | 16 21 48 | - 26 27 | 6 m | 103a - O | U G 2 | 4 | Landolt | 31 05 71 | NGC 6121 | |||
1540 | 16 21 48 | - 26 27 | 6 m | 103a - O | U G 2 | 4 | Landolt | 31 05 71 | NGC 6121 | |||
1541 | 16 21 48 | - 26 27 | 6 m | 103a - O | U G 2 | 4 | Landolt | 31 05 71 | NGC 6121 |
Last Updated on 8/27/99
By Guerra & Marin
June 1971 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1542 | 16 21 48 | - 26 27 | 4 m | 103a - O | GG 385 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1543 | 16 21 48 | - 26 27 | 4 m | 103a - O | GG 385 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1544 | 16 21 48 | - 26 27 | 5 m | 103a - D | GG 495 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1545 | 16 21 48 | - 26 27 | 5 m | 103a - D | GG 495 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1546 | 16 21 48 | - 26 27 | 60 m | 098 - 02 | RG 610 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1547 | 16 21 48 | - 26 27 | 2 m | 103a - O | GG 385 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1548 | 16 21 48 | - 26 27 | 2 m | 098 - 02 | GG 385 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1549 | 16 21 48 | - 26 27 | 2:30 m | 103a - D | GG 495 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1550 | 16 21 48 | - 26 27 | 2:30 m | 103a - D | GG 495 | 3 | Landolt | 01 06 71 | NGC 6121 | |||
1551 | 16 21 48 | - 26 27 | 18 m | 103a - O | U G 2 | 4 | Landolt | 01 06 71 | NGC 6121 | |||
1552 | 16 21 48 | - 26 27 | 18 m | 103a - O | U G 2 | 4 | Landolt | 01 06 71 | NGC 6121 | |||
1553 | 16 15 12 | - 22 55 | 30 m | 103a - D | GG 495 | 2--3 | Landolt | 01 06 71 | NGC 6093 | |||
1554 | 16 25 24 | - 25 59 | 20 m | 103a - O | GG 385 | 4 | Landolt | 01 06 71 | NGC 6144 | |||
1555 | 17 46 14 | - 24 45.9 | 60 m | 098 - 02 | RG 610 | 4 | Landolt | 01 06 71 | IRC 20385 | |||
1556 | (*) |
(*) Corresponde a Tubo Imagen
Last Updated on 8/27/99
By Guerra & Marin
August 1971 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1587 | 13 44 00 | - 47 06 | 01 seg | II a - D | GG 495 | 2--3 | Graham | 02 08 71 | NGC 5139 | |||
1588 | 13 44 00 | - 47 06 | 15 seg | II a - O | U G 2 | 2--3 | Graham | 02 08 71 | NGC 5139 | |||
1589 | 13 44 00 | - 47 06 | 7 seg | II a - O | U G 2 | 2--3 | Graham | 02 08 71 | NGC 5139 | |||
1590 | 13 44 00 | - 47 06 | 5 seg | II a - D | GG 495 | 2--3 | Graham | 02 08 71 | NGC 5139 | |||
1591 | (1) | |||||||||||
1602 | 05 40 06 | - 66 39 | 3 m | 103a - O | NO | 2 | Smith | 17 08 71 | Nova Graham 1971 b | |||
1603 | 05 40 06 | - 66 39 | 1 m | 103a - O | NO | 2 | Smith | 17 08 71 | Nova Graham 1971 b | |||
1604 | 15 25 06 | - 50 31 | 1 m | II a - D | GG 495 | ? | 27 08 71 | NGC 5927 | ||||
1605 | 15 25 06 | - 50 31 | 12 m | II a - O | U G 2 | ? | 27 08 71 | NGC 5927 | ||||
1606 | 15 32 30 | - 50 32 | 24 m | II a - O | U G 2 | ? | 27 08 71 | NGC 5946 | ||||
1607 | 15 32 30 | - 50 32 | 2 m | II a - D | GG 495 | ? | 27 08 71 | NGC 5946 | ||||
1608 | 17 22 24 | - 48 27 | 30 sec | II a - D | GG 495 | ? | 27 08 71 | NGC 6352 | ||||
1609 | 17 22 24 | - 48 27 | 6 m | II a - O | U G 2 | ? | 27 08 71 | NGC 6352 | ||||
1610 | 17 37 36 | - 53 39 | 2 m | II a - O | U G 2 | ? | 27 08 71 | NGC 6397 | ||||
1611 | 17 37 36 | - 53 39 | 10 sec | II a - D | GG 495 | ? | 27 08 71 | NGC 6397 | ||||
1612 | 00 25 42 | - 71 41 | 45 m | 103a - O | GG 385 | ? | 27 08 71 | NGC 121 | ||||
1613 | 01 00 00 | - 33 40 | 75 m | 103a - O | GG 385 | ? | 27 08 71 | Sculptor | ||||
1613 | 00 23 48 | - 72 56 | 75 m | 103a - O | GG 385 | ? | 27 08 71 | Kron 3 | ||||
1614 | 00 25 42 | - 71 41 | 50 m | 103a - O | GG 385 | ? | 27 08 71 | NGC 121 | ||||
1615 | 00 25 42 | - 71 41 | 50 m | 103a - O | GG 385 | ? | 27 08 71 | NGC 121 | ||||
1616 | 00 25 42 | - 71 41 | 0 | 103a - O | GG 385 | ? | 27 08 71 | NGC 121 | Bad plate | |||
1617 | 05 41 00 | - 66 40 | 5 m | 103a - O | GG 385 | ? | 27 08 71 | Nova Dor. 1971 l | ||||
1618 | 23 09 00 | - 35 42 | 15 m | 103a - O | GG 385 | Lasker | 28 08 71 | Stock Object | ||||
1619 | 23 09 00 | - 35 42 | 15 m | 103a - D | GG 495 | Lasker | 28 08 71 | Stock Object | ||||
1620 | 00 32 00 | - 07 29 | 60 m | 103a - O | GG 385 | Lasker | 28 08 71 | MP 00 31 | CTIO | |||
1621 | 04 51 00 | - 17 57 | 60 m | 103a - O | GG 385 | Lasker | 28 08 71 | MP 04 50 | CTIO | |||
1622 | 14 51 10 | - 64 37 | 60 m | 103a - O | GG 385 | Lasker | 29 08 71 | MP 14 49 | CTIO | |||
1623 | 14 51 10 | - 65 33 | 30 m | 103a - O | GG 385 | Lasker | 29 08 71 | MP 14 49 | CTIO | |||
1624 | 20 49 18 | - 69 21 | 60 m | 103a - D | GG 495 | Lasker | 29 08 71 | IC 5152 | ||||
1625 | 20 46 59 | - 16 22.7 | 30 m | 103a - O | GG 385 | Lasker | 29 08 71 | PSR 2045-16 | CTIO | |||
1626 | 00 53 30 | - 37 52 | 130 m | 103a - O | GG 385 | Lasker | 29 08 71 | NGC 300 | Bad plate | |||
1627 | 01 00 00 | - 33 40 | 45 m | 103a - O | GG 385 | ? | 27 08 71 | Sculptor | ||||
1627 | 00 23 48 | - 72 56 | 45 m | 103a - O | GG 385 | ? | 27 08 71 | Kron 3 |
(1) Al 1601 corresponde a Tubo Imagen
Last Updated on 8/27/99
By Jorge Marin
September 1971 Plate logs for 1.5-m telescope
Plate | N. N | R . A | Dec | Exp.Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1628 | (1) | |||||||||||
1630 | 17 11 00 | - 29 24 | 15 m | 103a - O | GG 385 | Smith | 17 09 71 | NGC 6304 | ||||
1631 | 17 11 00 | - 29 24 | 15 m | 103a - D | GG 495 | Smith | 17 09 71 | NGC 6304 | ||||
1632 | 17 48 06 | - 37 02 | 15 m | 103a - D | GG 495 | 3--4 | Smith | 17 09 71 | NGC 6441 | |||
1633 | 17 48 06 | - 37 02 | 15 m | 103a - D | GG 495 | 3 | Smith | 17 09 71 | NGC 6441 | |||
1634 | 17 23 00 | - 48 21 | 15 m | 103a - O | GG 385 | 3 | Smith | 17 09 71 | NGC 6352 | |||
1635 | 17 23 00 | - 48 21 | 15 m | 103a - D | GG 495 | 3 | Smith | 17 09 71 | NGC 6352 | |||
1636 | 17 11 24 | - 29 24 | 15 m | 103a - D | GG 495 | 3 | Smith | 17 09 71 | NGC 6304 | |||
1637 | 23 10 15 | - 35 29 | 15 m | 103a - D | GG 495 | 4 | Smith | 17 09 71 | Field JEM | |||
1638 | 23 10 15 | - 35 29 | 15 m | 103a - O | GG 385 | 4 | Graham | 21 09 71 | Field JEM | |||
1639 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | 4 | Graham | 21 09 71 | NGC 121 | |||
1640 | 00 25 42 | - 71 41 | 55 m | 103a - O | GG 385 | 4 | Graham | 21 09 71 | NGC 121 | |||
1641 | 00 25 42 | - 71 41 | 55 m | 103a - O | GG 385 | 2 | Graham | 21 09 71 | NGC 121 | |||
1642 | 00 25 42 | - 71 41 | 60 m | 103a - D | GG 495 | Graham | 21 09 71 | NGC 121 | ||||
1643 | 00 25 42 | - 71 41 | 55 m | 103a - O | GG 385 | Graham | 21 09 71 | NGC 121 | ||||
1644 | 00 25 42 | - 71 41 | 55 m | 103a - O | GG 385 | Graham | 21 09 71 | NGC 121 | ||||
1645 | 00 25 42 | - 71 41 | 55 m | 103a - O | GG 385 | Graham | 21 09 71 | NGC 121 | ||||
1646 | 00 25 42 | - 71 41 | 55 m | 103a - O | GG 385 | Graham | 21 09 71 | NGC 121 | ||||
1647 | 05 41 00 | - 66 40 | 10 m | 103a - O | GG 385 | Graham | 21 09 71 | Nova Dor 1971 b | ||||
1648 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 22 09 71 | NGC 121 | ||||
1649 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 22 09 71 | NGC 121 | ||||
1650 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 22 09 71 | NGC 121 | ||||
1651 | 00 25 42 | - 71 41 | 60 m | 103a - D | GG 495 | Graham | 22 09 71 | NGC 121 | ||||
1652 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 22 09 71 | NGC 121 | ||||
1653 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 22 09 71 | NGC 121 | ||||
1654 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 22 09 71 | NGC 121 | ||||
1655 | 02 00 00 | - 74 30 | 10 m | 103a - O | GG 385 | Graham | 22 09 71 | NGC 121 | ||||
1656 | 05 41 00 | - 66 40 | 10 m | 103a - O | GG 385 | Graham | 22 09 71 | Nova Dor 1971 b | ||||
1657 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 24 09 71 | NGC 121 | ||||
1658 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 24 09 71 | NGC 121 | ||||
1659 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 24 09 71 | NGC 121 | ||||
1660 | 00 25 42 | - 71 41 | 60 m | 103a - D | GG 495 | Graham | 24 09 71 | NGC 121 | ||||
1661 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 24 09 71 | NGC 121 | ||||
1662 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 24 09 71 | NGC 121 | ||||
1663 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 24 09 71 | NGC 121 | ||||
1664 | 02 00 00 | - 74 30 | 10 m | 103a - O | GG 385 | Graham | 24 09 71 | NGC 121 | ||||
1665 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 25 09 71 | NGC 121 | ||||
1666 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 25 09 71 | NGC 121 | ||||
1667 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 25 09 71 | NGC 121 | ||||
1668 | 00 25 42 | - 71 41 | 60 m | 103a - D | GG 495 | Graham | 25 09 71 | NGC 121 | ||||
1669 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 25 09 71 | NGC 121 | ||||
1670 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 25 09 71 | NGC 121 | ||||
1671 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 25 09 71 | NGC 121 | ||||
1672 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | Graham | 25 09 71 | NGC 121 |
(1) Al 1629 corresponde a Tubo Imagen
Last Updated on 8/27/99
By Guerra & Marin
October 1971 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1673 | 18 55 36 | - 62 09 | 10 m | 103a - O | GG 385 | 2 | Graham | 14 10 71 | Nova IC 4798 | |||
1674 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | NGC 121 | |||
1675 | 00 25 42 | - 71 41 | 10 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | NGC 121 | |||
1676 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | NGC 121 | |||
1677 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | NGC 1783 | |||
1678 | 04 58 24 | - 68 08 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | 1971 b Doradus | |||
1679 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | NGC 1783 | |||
1680 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | NGC 1783 | |||
1681 | 04 59 00 | - 66 01 | 35 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | 1971 b Doradus | |||
1682 | 04 59 00 | - 66 01 | 35 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | NGC 1783 | |||
1683 | - 90 00 | 5 m | 103a - O | GG 385 | 1.5 | Graham | 14 10 71 | Pole | ||||
1684 | 18 55 36 | - 62 09 | 60 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | Nova IC 4798 | |||
1685 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | NGC 121 | |||
1686 | 00 25 42 | - 71 41 | 60 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | NGC 121 | |||
1687 | 02 00 00 | - 74 30 | 10 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | NGC 1783 | |||
1688 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | NGC 1783 | |||
1689 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | NGC 121 | |||
1690 | 00 25 42 | - 71 41 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | NGC 121 | |||
1691 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | NGC 1783 | |||
1692 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 15 10 71 | NGC 1783 | |||
1693 | 17 38 00 | - 53 40 | 15 m | 103a - O | GG 385 | 3 | Hesser | 19 10 71 | NGC 6397 | |||
1694 | 17 38 00 | - 53 40 | 15 m | 103a - D | GG 495 | 3 | Hesser | 19 10 71 | NGC 6397 | |||
1695 | 22 00 54 | - 51 26 | 60 m | 103a - O | GG 385 | 2--3 | Hesser | 19 10 71 | IC 5152 | |||
1696 | 00 21 50 | - 72 09.7 | 60 m | 103a - D | GG 495 | 3 | Hesser | 19 10 71 | 47 Tucana | |||
1697 | 00 21 50 | - 72 09.7 | 15 m | 103a - D | GG 495 | 2 | Hesser | 19 10 71 | 47 Tucana | |||
1698 | 00 21 50 | - 72 09.7 | 60 m | 103a - O | GG 385 | 2 | Hesser | 19 10 71 | 47 Tucana | |||
1699 | 00 21 50 | - 72 09.7 | 15 m | 103a - O | GG 385 | 2 | Hesser | 19 10 71 | 47 Tucana | |||
1700 | 00 53 36 | - 37 51 | 60 m | 103a - O | GG 385 | 1.5 | Hesser | 19 10 71 | NGC 300 | CTIO | ||
1701 | 00 53 36 | - 37 51 | 60 m | 103a - D | GG 495 | 1.5 | Hesser | 19 10 71 | NGC 300 | CTIO | ||
1702 | 04 30 30 | - 27 43.6 | 15 m | 103a - D | GG 495 | 1.5 | Hesser | 19 10 71 | Field | |||
1703 | 04 30 30 | - 27 43.6 | 15 m | 103a - O | GG 385 | 1.5 | Hesser | 19 10 71 | Field | |||
1704 | 17 38 00 | - 53 40 | 30 m | 103a - D | GG 495 | 3 | Hesser | 20 10 71 | NGC 6397 | |||
1705 | 17 38 00 | - 53 40 | 15 m | 103a - O | GG 385 | 2.5 | Hesser | 20 10 71 | NGC 6397 | |||
1706 | 18 39 34 | - 49 07 | 10 m | 103a - O | GG 385 | 2.5 | Hesser | 20 10 71 | Field | |||
1707 | 18 39 34 | - 49 07 | 10 m | 103a - D | GG 495 | 2.5 | Hesser | 20 10 71 | Field | |||
1708 | 22 00 54 | - 51 26 | 60 m | 103a - O | GG 385 | 2.5 | Hesser | 20 10 71 | IC 5152 | |||
1709 | 00 53 36 | - 37 51 | 120 m | 103a - O | GG 385 | 2.5 | Hesser | 20 10 71 | NGC 300 | CTIO | ||
1710 | 00 21 50 | - 72 09.7 | 30 m | 103a - O | GG 385 | 2.5 | Hesser | 20 10 71 | 47 Tucana | |||
1711 | 00 21 50 | - 72 09.7 | 30 m | 103a - D | GG 495 | 2.5 | Hesser | 20 10 71 | 47 Tucana | |||
1712 | 00 21 50 | - 72 09.7 | 15 m | 103a - D | GG 495 | 2.5 | Hesser | 20 10 71 | 47 Tucana | |||
1713 | 00 21 50 | - 72 09.7 | 15 m | 103a - O | GG 385 | 2.5 | Hesser | 20 10 71 | 47 Tucana | |||
1714 | 00 21 50 | - 72 09.7 | 15 m | 103a - O | GG 385 | 2.5 | Hesser | 20 10 71 | 47 Tucana | |||
1715 | 00 21 50 | - 72 09.7 | 15 m | 103a - D | GG 495 | 2.5 | Hesser | 20 10 71 | 47 Tucana | |||
1716 | 05 00 00 | - 31 41 | 15 m | 103a - D | GG 495 | 2 | Hesser | 20 10 71 | Field | |||
1717 | 05 00 00 | - 31 41 | 15 m | 103a - O | GG 385 | 2 | Hesser | 20 10 71 | Field | |||
1718 | 23 42 30 | - 15 30 | 60 m | 098 - 02 | RG 610 | 1.5 | Blanco | 28 10 71 | R. Acuarium | CTIO | ||
1719 | 00 13 30 | - 39 21 | 30 m | 103a - O | GG 385 | 1.5 | Blanco | 28 10 71 | NGC 55 | |||
1720 | 00 53 54 | - 37 49 | 20 m | 103a - O | GG 385 | 1.5 | Blanco | 28 10 71 | NGC 300 | BROKEN OK" | CTIO | |
1721 | 00 46 18 | - 25 25 | 20 m | 103a - O | GG 385 | 1.5 | Blanco | 28 10 71 | NGC 253 | CTIO | ||
1722 | 06 35 30 | - 62 36.9 | 90 m | 098 - 02 | RG 610 | 1.5 | Blanco | 28 10 71 | Nova 1925 | CTIO | ||
1723 | 18 24 09 | - 31 42 | 12 m | 098 - 02 | RG 610 | 2 | Blanco | 29 10 71 | V455 Sagittarius | CTIO | ||
1724 | 21 25 47 | - 65 24 | 30 m | 098 - 02 | RG 610 | 2 | Blanco | 29 10 71 | AR Pavonis | CTIO | ||
1725 | 20 08 42 | - 53 12 | 30 m | 098 - 02 | RG 610 | 2 | Blanco | 29 10 71 | BL Telescopium | CTIO | ||
1726 | 23 42 30 | - 15 30 | 30 m | 098 - 02 | RG 610 | 2 | Blanco | 29 10 71 | R Aquarius | CTIO | ||
1727 | 00 24 00 | - 72 04 | 30 m | 098 - 02 | RG 610 | 3 | Blanco | 29 10 71 | VW Tucana | CTIO | ||
1728 | 04 24 40 | - 21 12 | 30 m | 098 - 02 | RG 610 | 3 | Blanco | 29 10 71 | UV Eridanus | CTIO | ||
1729 | 07 15 24 | - 26 53 | 21 m | 098 - 02 | RG 610 | 3.5 | Blanco | 29 10 71 | CG C.Ma | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
November 1971 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1730 | (1) | |||||||||||
1799 | 00 21 54 | - 72 21 | 10 m | IN + H2O | RG 695 | 3 | Spinrad | 17 11 71 | 47 Tucana | |||
1800 | 00 21 54 | - 72 21 | 20 m | IN + H2O | RG 695 | 2 | Spinrad | 17 11 71 | 47 Tucana | |||
1801 | 00 21 54 | - 72 21 | 6 m | 103a - D | GG 495 | 2 | Spinrad | 17 11 71 | 47 Tucana | |||
1802 | 00 21 54 | - 72 21 | 6 m | 098 - 02 | RG 610 | 2 | Spinrad | 17 11 71 | 47 Tucana | |||
1803 | 00 25 40 | - 71 41 | 120 m | 098 - 02 | RG 610 | 2--3 | Spinrad | 17 11 71 | NGC 121 | |||
1804 | 00 50 00 | - 73 10 | 90 m | 098 - 02 | RG 610 | 2 | Spinrad | 17 11 71 | LMC Center | |||
1805 | 05 24 40 | - 69 47 | 90 m | 098 - 02 | RG 610 | 1.5 | Spinrad | 17 11 71 | LMC Bar | |||
1806 | 05 24 40 | - 69 47 | 40 m | 103a - O | GG 385 | 1.5 | Spinrad | 17 11 71 | LMC Bar | |||
1807 | 04 19 19 | - 55 00 | 10 m | III a - J | GG 385 | 1 | Spinrad | 17 11 71 | NGC 1566 | |||
1808 | 05 38 00 | - 69 00 | 12 m | 098 - 02 | RG 610 | 3 | Spinrad | 17 11 71 | 30 Doradus | |||
1809 | 00 50 00 | - 73 10 | 40 m | 103a - O | GG 385 | 2 | Graham | 18 11 71 | SMC Center | |||
1810 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 2 | Graham | 18 11 71 | NGC 1783 | |||
1811 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 18 11 71 | NGC 1783 | |||
1812 | 04 59 00 | - 66 01 | 40 m | 103a - D | GG 495 | 1.5 | Graham | 18 11 71 | NGC 1783 | |||
1813 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 18 11 71 | NGC 1783 | |||
1814 | 05 05 00 | - 69 26 | 60 m | 103a - D | GG 495 | 1.5 | Graham | 18 11 71 | NGC 1835 | |||
1815 | 05 05 00 | - 69 26 | 30 m | 103a - O | GG 385 | 1.5 | Graham | 18 11 71 | NGC 1835 | |||
1816 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 18 11 71 | NGC 1783 | |||
1817 | 05 41 00 | - 66 40 | 15 m | 103a - O | GG 385 | 1.5 | Graham | 18 11 71 | Nova 1971b |
(1) Al 1798 corresponde a Tubo Imagen
Last Updated on 8/27/99
By Guerra & Marin
December 1971 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1818 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 11 12 71 | NGC 1783 | ||||
1819 | 05 07 06 | - 69 14 | 40 m | 103a - O | GG 385 | Graham | 11 12 71 | Bok | ||||
1820 | 05 07 06 | - 69 14 | 60 m | 103a - D | GG 495 | Graham | 11 12 71 | Bok | ||||
1821 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 11 12 71 | NGC 1783 | ||||
1822 | 05 05 00 | - 69 26 | 40 m | 103a - O | GG 385 | Graham | 11 12 71 | NGC 1835 | ||||
1823 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 11 12 71 | NGC 1783 | ||||
1824 | 05 05 00 | - 69 26 | 40 m | 103a - O | GG 385 | Graham | 11 12 71 | NGC 1835 | ||||
1825 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 11 12 71 | NGC 1783 | ||||
1826 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 12 12 71 | NGC 1783 | ||||
1827 | 05 07 06 | - 69 14 | 40 m | 103a - O | GG 385 | Graham | 12 12 71 | Bok | ||||
1828 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 12 12 71 | NGC 1783 | ||||
1829 | 04 59 00 | - 66 01 | 60 m | 103a - D | GG 495 | Graham | 12 12 71 | NGC 1783 | ||||
1830 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 12 12 71 | NGC 1783 | ||||
1831 | 05 07 06 | - 69 14 | 10 m | 103a - D | GG 495 | Graham | 12 12 71 | Bok | ||||
1832 | 05 07 06 | - 69 14 | 40 m | 103a - O | GG 385 | Graham | 12 12 71 | Bok | ||||
1833 | 05 07 06 | - 69 14 | 10 m | 103a - O | GG 385 | Graham | 12 12 71 | Bok | ||||
1834 | 04 59 00 | - 66 01 | 30 m | 103a - O | GG 385 | Graham | 12 12 71 | NGC 1783 | ||||
1835 | 05 07 06 | - 69 14 | 30 m | 103a - O | GG 385 | Graham | 12 12 71 | Bok | ||||
1836 | 05 07 06 | - 69 14 | 13 m | 103a - O | GG 385 | Graham | 13 12 71 | Bok | ||||
1837 | 05 07 06 | - 69 14 | 40 m | 103a - O | GG 385 | Graham | 13 12 71 | Bok | ||||
1838 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 13 12 71 | NGC 1783 | ||||
1839 | 05 07 06 | - 69 14 | 40 m | 103a - O | GG 385 | Graham | 13 12 71 | Bok | ||||
1840 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 13 12 71 | NGC 1783 | ||||
1841 | 05 07 06 | - 69 14 | 40 m | 103a - O | GG 385 | Graham | 13 12 71 | Bok | CTIO | |||
1842 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | Graham | 13 12 71 | NGC 1783 | ||||
1843 | 05 07 06 | - 69 14 | 40 m | 103a - O | GG 385 | Graham | 13 12 71 | Bok | ||||
1844 | 00 06 00 | - 41 48 | 60 m | 103a - O | GG 385 | 1.5 | Buarbidge | 16 12 71 | Anon Trio | |||
1845 | 01 17 48 | - 41 31 | 60 m | 103a - O | GG 385 | 1.5 | Buarbidge | 16 12 71 | Anon Group | |||
1846 | 03 16 18 | - 41 13 | 60 m | 103a - O | GG 385 | 1.5 | Buarbidge | 16 12 71 | NGC 1291 | |||
1847 | 03 54 50 | - 42 27 | 60 m | 103a - O | GG 385 | 1.5 | Buarbidge | 16 12 71 | NGC 1487 | |||
1848 | 04 28 24 | - 53 53.4 | 60 m | 103a - O | GG 385 | 1.5 | Buarbidge | 16 12 71 | IC 2082 | |||
1849 | 06 17 29 | - 48 44.1 | 65 m | 103a - O | GG 385 | 1.5 | Buarbidge | 16 12 71 | PKS 0616 - 48 | |||
1850 | 05 19 00 | - 72 33 | 90 m | 098 - 02 | RG 610 | 1.5 | Graham | 25 12 71 | LMC X2 | |||
1851 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 25 12 71 | NGC 1783 | |||
1852 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 25 12 71 | NGC 1783 | |||
1853 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 25 12 71 | NGC 1783 | |||
1854 | 04 59 00 | - 66 01 | 60 m | 103a - O | GG 385 | 1.5 | Graham | 25 12 71 | NGC 1783 | |||
1855 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 26 12 71 | NGC 1783 | |||
1856 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1.5 | Graham | 26 12 71 | NGC 1783 | |||
1857 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1--2 | Graham | 26 12 71 | NGC 1783 | |||
1858 | 04 59 00 | - 66 01 | 50 m | 103a - O | GG 385 | 1--2 | Graham | 26 12 71 | NGC 1783 | |||
1859 | 05 38 00 | - 64 06 | 90 m | 098 - 02 | RG 610 | 1 | Graham | 26 12 71 | LMC X3 | |||
1860 | 04 59 00 | - 66 01 | 90 m | 098 - 02 | RG 610 | 1--3 | Graham | 26 12 71 | NGC 1783 | |||
1861 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1 | Graham | 26 12 71 | NGC 1783 | |||
1862 | 04 59 00 | - 66 01 | 40 m | 103a - O | GG 385 | 1--3 | Graham | 26 12 71 | NGC 1783 | |||
1863 | 04 59 00 | - 66 01 | 50 m | 103a - O | GG 385 | 2--3 | Graham | 26 12 71 | NGC 1783 |
Last Updated on 8/27/99
By Jorge Marin
1972 Plate logs for 1.5-m telescope
February 1972 Plate logs for 1.5-m telescope
Plate | N.N. | R.A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
1997 | (1) | |||||||||||
(2) | ||||||||||||
2018 | 1918 | 08 34 23 | - 45 05 | 10 m | 103a - O | GG 385 | 1.5 | Lasker Hilther | 15 02 72 | PSR 0833 - 45 | ||
2019 | 1919 | 11 20 00 | - 60 26 | 15 m | II a - O | GG 385 | 1.5 | Lasker Hilther | 15 02 72 | 2ASE 1119 - 60 | Broken | CTIO |
2020 | 1920 | 11 20 00 | - 60 26 | 60 m | II a - O | GG 385 | 1.5 | Lasker Hilther | 15 02 72 | 2ASE 1119 - 60 | Broken | CTIO |
2021 | 1921 | 15 45 25 | - 47 39 | 12 m | II a - O | GG 385 | 1.5 | Lasker Hilther | 15 02 72 | 2ASE 1543 - 47 | CTIO | |
2022 | 1922 | 15 45 25 | - 47 39 | 60 m | II a - O | GG 385 | 1.5 | Lasker Hilther | 15 02 72 | 2ASE 1543 - 47 | Broken | CTIO |
2023 | 1923 | 05 39 00 | - 69 10 | 10 m | II a - O | GG 385 | 1.5 | Graham | 15 02 72 | 30 Doradus | ||
2024 | 1924 | 05 39 00 | - 69 10 | 10 m | 098 - 02 | GG 385 | 1.5 | Graham | 19 02 72 | 30 Doradus | ||
2025 | 1925 | 04 59 00 | - 66 02 | 30 m | 103a - O | GG 385 | 1.5 | Graham | 19 02 72 | NGC 1783 | ||
2026 | 1926 | 10 46 00 | - 59 29 | 5 m | 103a - O | GG 385 | 1.5 | Graham | 19 02 72 | Eta Carina | ||
2027 | 1927 | 10 46 00 | - 59 29 | 5 m | 103a - O | GG 385 | 1.5 | Graham | 19 02 72 | Eta Carina | ||
2028 | 1928 | 13 23 00 | - 42 52 | 60 m | 103a - O | GG 385 | 1.5 | Graham | 19 02 72 | NGC 5128 | ||
2029 | 1929 | 13 25 00 | - 47 20 | 45 m | 103a - O | GG 385 | Graham | 19 02 72 | Omega Cen. | |||
2030 | 1930 | 13 25 00 | - 47 20 | 12 m | 103a - O | GG 385 | Graham | 19 02 72 | Omega Cen. | |||
2031 | 1931 | 05 39 00 | - 69 10 | 20 m | 103a - O | GG 385 | Graham | 20 02 72 | 30 Doradus | |||
2032 | 1932 | 05 09 00 | - 69 00 | 30 m | 103a - O | GG 385 | Graham | 20 02 72 | Bok Tifft | |||
2033 | 1933 | 05 22 00 | - 68 00 | 30 m | 103a - O | GG 385 | Graham | 20 02 72 | Constellation I | |||
2034 | 1934 | 06 30 00 | - 64 18 | 60 m | 103a - O | GG 385 | Graham | 20 02 72 | NGC 2257 | |||
2035 | 1935 | 10 59 30 | - 60 00 | 30 m | 103a - O | GG 385 | Graham | 20 02 72 | Carina arm | |||
2036 | 1936 | 10 34 06 | - 58 05 | 10 m | 103a - O | GG 385 | Graham | 20 02 72 | NGC 3293 | |||
2037 | 1937 | 11 12 00 | - 61 05 | 30 m | 103a - O | GG 385 | Graham | 20 02 72 | NGC 3603 | |||
2038 | 1938 | 11 12 00 | - 61 05 | 30 m | 103a - O | GG 385 | Graham | 20 02 72 | NGC 3603 | |||
2039 | 1939 | 10 59 30 | - 60 00 | 30 m | 103a - O | GG 385 | Graham | 20 02 72 | Carina arm | |||
2040 | 1940 | 13 25 00 | - 47 20 | 45 m | 103a - O | GG 385 | Graham | 20 02 72 | Omega Cen. | |||
2041 | 1941 | 15 54 00 | - 54 40 | 30 m | 103a - O | GG 385 | Graham | 20 02 72 | Norma Field | |||
2042 | 1942 | 15 54 00 | - 54 40 | 30 m | 103a - O | GG 385 | Graham | 20 02 72 | Norma Field | |||
2043 | 1943 | 17 37 36 | - 53 39 | 5 m | 103a - O | GG 385 | Graham | 20 02 72 | NGC 6397 | |||
2044 | 1944 | 04 36 18 | - 08 51 | 10 m | 103a - O | GG 385 | Graham | 21 02 72 | EG 41 | |||
2045 | 1945 | 07 53 36 | - 14 41 | 10 m | 103a - O | GG 385 | Graham | 21 02 72 | EG 57 | |||
2046 | 1946 | 06 57 00 | - 04 30 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Monoceros | |||
2047 | 1947 | 07 52 00 | - 28 22 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Puppis | |||
2048 | 1948 | 09 25 42 | - 52 56 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Vela | |||
2049 | 1949 | 12 14 00 | - 62 50 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Crux | CTIO | ||
2050 | 1950 | 13 27 00 | - 63 45 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Centaurus | |||
2051 | 1951 | 09 25 42 | - 52 56 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Vela | |||
2052 | 1952 | 12 14 00 | - 62 50 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Crux | |||
2053 | 1953 | 13 27 00 | - 63 45 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Centaurus | |||
2054 | 1954 | 15 54 00 | - 54 40 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | Norma Field | |||
2055 | 1955 | 17 37 36 | - 53 39 | 30 m | 103a - O | GG 385 | Graham | 21 02 72 | NGC 6397 | |||
2056 | 1956 | 02 45 12 | - 30 24 | 25 m | 103a - O | GG 385 | Smith | 22 02 72 | NGC 1097 | |||
2057 | 1957 | 05 35 29 | - 49 45 | 30 m | 103a - O | GG 385 | Smith | 22 02 72 | PKS 0535 - 49 | CTIO | ||
2058 | 1958 | 05 35 29 | - 49 45 | 60 m | 103a - O | GG 385 | Smith | 22 02 72 | PKS 0535 - 49 | CTIO | ||
2059 | 1959 | 07 43 26 | - 67 22 | 120 m | 103a - O | GG 385 | Smith | 22 02 72 | PKS 0744 - 67 | CTIO | ||
2060 | 1960 | 11 17 10 | - 46 25 | 100 m | II a -O | GG 385 | Smith | 22 02 72 | PKS 1116 - 46 | CTIO |
(1) Al 2017 Corresponde a Tubo Imagen
(2) Nueva numeracion por error por tanto desde el Nº 1990 a el Nº 1999 estan repetidos
Last Updated on 8/27/99
By Guerra & Marin
March 1972 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2061 | 1961 | (1) | ||||||||||
2063 | 1963 | 10 03 30 | - 58 32 | 90 m | 098 - 02 | RG 610 | 2 | Henize | 17 03 72 | HD 87643 | ||
2064 | 1964 | 11 07 00 | - 77 30 | 120 m | 103a - O | GG 385 | 2 | Henize | 17 03 72 | HD 97048 | ||
2065 | 1965 | 11 07 00 | - 76 27 | 120 m | 103a - O | GG 385 | 2 | Henize | 17 03 72 | HD 97300 | ||
2066 | 1966 | 11 07 00 | - 77 30 | 120 m | 103a - D | GG 495 | 2 | Henize | 17 03 72 | HD 97048 | ||
2067 | 1967 | 18 59 00 | - 37 00 | 58 m | 103a - O | GG 385 | 2 | Henize | 17 03 72 | R Corona Australis | ||
2068 | 1968a | 08 35 00 | - 26 17 | 4 m | 098 - 02 | RG 610 | 2 | Henize | 18 03 72 | He -2 - 10 | ||
2068 | 1968b | 08 35 00 | - 26 17 | 15 m | 098 - 02 | RG 610 | 2 | Henize | 18 03 72 | He -2 - 10 | ||
2068 | 1968c | 08 35 00 | - 26 17 | 60 m | 098 - 02 | RG 610 | 2 | Henize | 18 03 72 | He -2 - 10 | ||
2069 | 1969 | 11 07 00 | - 77 30 | 100 m | 098 - 02 | RG 610 | 2 | Henize | 18 03 72 | HD 97048 | ||
2070 | 1970 | 11 07 00 | - 76 27 | 100 m | 098 - 02 | RG 610 | 2 | Henize | 18 03 72 | HD 97300 | ||
2071 | 1971 | 11 07 00 | - 76 27 | 120 m | 103a - D | GG 495 | 2 | Henize | 18 03 72 | HD 97300 | ||
2072 | 1972 | 11 07 00 | - 77 30 | 94 m | 103a - D | GG 495 | 2 | Henize | 18 03 72 | HD 97048 |
(1) Al 1962 corresponde a Tubo Imagen
Last Updated on 8/27/99
By Guerra & Marin
May 1972 Plate logs for 1.5-m telescope
Plate | N. N | R . A | Dec | Exp.Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2073 | 1973 | 07 52 00 | - 38 26 | 15 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | NGC 2477 | ||
2074 | 1974 | 07 52 00 | - 38 26 | 15 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | NGC 2477 | ||
2075 | 1975 | 07 52 00 | - 38 26 | 15 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 10 05 72 | NGC 2477 | ||
2076 | 1976 | 10 42 00 | - 71 00 | 15 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 10 05 72 | Field | ||
2077 | 1977 | 10 42 00 | - 71 00 | 15 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | Field | ||
2078 | 1978 | 10 42 00 | - 71 00 | 15 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | Field | ||
2079 | 1979 | 10 42 00 | - 71 00 | 15 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 10 05 72 | Field | ||
2080 | 1980 | 17 13 00 | - 29 26 | 30 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 10 05 72 | NGC 6304 | ||
2081 | 1981 | 17 13 00 | - 29 26 | 30 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | NGC 6304 | ||
2082 | 1982 | 17 13 00 | - 29 26 | 30 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | NGC 6304 | ||
2083 | 1983 | 17 13 00 | - 29 26 | 30 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 10 05 72 | NGC 6304 | ||
2084 | 1984 | 17 48 00 | - 37 02 | 30 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2085 | 1985 | 17 48 00 | - 37 02 | 30 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2086 | 1986 | 17 48 00 | - 37 02 | 30 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2087 | 1987 | 17 48 00 | - 37 02 | 30 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2088 | 1988 | 17 48 00 | - 37 02 | 15 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2089 | 1989 | 17 48 00 | - 37 02 | 30 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2090 | 1990 | 17 48 00 | - 37 02 | 45 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2091 | 1991 | 17 48 00 | - 37 02 | 10 m | 103a - D | GG 495 | 2.5 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2092 | 1992 | 17 48 00 | - 37 02 | 10 m | 103a - D | GG 495 | 2.5 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2093 | 1993 | 17 48 00 | - 37 02 | 5 m | 103a - D | GG 495 | 2.5 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2094 | 1994 | 17 48 00 | - 37 02 | 5 m | 103a - D | GG 495 | 2.5 | Hesser Hartwich | 10 05 72 | NGC 6441 | ||
2095 | 1995 | 07 52 00 | - 38 10 | 15 m | 103a - O | GG 385 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 2477 | ||
2096 | 1996 | 07 52 00 | - 38 10 | 15 m | 103a - D | GG 495 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 2477 | ||
2097 | 1997 | 07 52 00 | - 38 10 | 15 m | 103a - D | GG 495 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 2477 | ||
2098 | 1998 | 07 52 00 | - 38 10 | 15 m | 103a - O | GG 385 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 2477 | ||
2099 | 1999 | 10 42 00 | - 71 00 | 15 m | 103a - O | GG 385 | 1.5 | Hesser Hartwich | 11 05 72 | Field | ||
2100 | 2000 | 10 42 00 | - 71 00 | 15 m | 103a - D | GG 495 | 1.5 | Hesser Hartwich | 11 05 72 | Field | ||
2101 | 2001 | 13 25 00 | - 47 09 | 5 m | 103a - D | GG 495 | 1.5 | Hesser Hartwich | 11 05 72 | Omega Cen. | ||
2102 | 2002 | 13 25 00 | - 47 09 | 5 m | 103a - O | GG 385 | 1.5 | Hesser Hartwich | 11 05 72 | Omega Cen. | ||
2103 | 2003 | 17 24 00 | - 48 24 | 30 m | 103a - O | GG 385 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 6352 | ||
2104 | 2004 | 17 24 00 | - 48 24 | 30 m | 103a - D | GG 495 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 6352 | ||
2105 | 2005 | 17 24 00 | - 48 24 | 30 m | 103a - D | GG 495 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 6352 | ||
2106 | 2006 | 17 24 00 | - 48 24 | 30 m | 103a - O | GG 385 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 6352 | ||
2107 | 2007 | 17 48 00 | - 37 02 | 45 m | 103a - O | GG 385 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 6441 | ||
2108 | 2008 | 17 48 00 | - 37 02 | 45 m | 103a - O | GG 385 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 6441 | ||
2109 | 2009 | 17 48 00 | - 37 02 | 7 m | 103a - D | GG 495 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 6441 | ||
2110 | 2010 | 17 13 00 | - 29 13 | 30 m | 103a - D | GG 495 | 1.5 | Hesser Hartwich | 11 05 72 | NGC 6304 | ||
2111 | 2011 | 17 13 00 | - 29 13 | 30 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 11 05 72 | NGC 6304 | ||
2112 | 2012 | 17 13 00 | - 29 13 | 20 m | 103a - O | GG 385 | 2 | Hesser Hartwich | 11 05 72 | NGC 6304 | ||
2113 | 2013 | 17 13 00 | - 29 13 | 20 m | 103a - D | GG 495 | 2 | Hesser Hartwich | 11 05 72 | NGC 6304 | ||
2114 | 2014 | Al 2075? (1) | ||||||||||
2176 | 2076 | 17 03 48 | -36 24 | 1.5m | lla - D | Spinad | Liller / Forman / Gomez | 14 05 72 | 1702 - 36 | |||
2177 | 2077 | 17 45 48 | -26 33 | 8m | lla - D | Spinad | Liller / Forman / Gomez | 14 05 72 | 1744 - 26 | |||
2178 | 2078 | 17 45 48 | -26 33 | 1.5m | lla - D | Spinad | Liller / Forman / Gomez | 14 05 72 | 1744 - 26 | |||
2179 | 2079 | 17 59 06 | -25 05 | 8m | lla - D | Spinad | Liller / Forman / Gomez | 14 05 72 | 1757 - 25 | |||
2180 | 2080 | 17 59 06 | -25 05 | 1.5m | lla - D | Spinad | Liller / Forman / Gomez | 14 05 72 | 1757 - 25 | |||
2181 | 2081 | 17 59 48 | -20 32 | 8m | lla - D | Spinad | Liller / Forman / Gomez | 14 05 72 | 1758 - 20 | |||
2182 | 2082 | 17 59 48 | -20 32 | 1.5m | lla - D | Spinad | Liller / Forman / Gomez | 14 05 72 | 1758 - 20 | |||
2183 | 2083 | 11 37 36 | -37 28 | 3m | lla - D | l | 4 | Smith / Gomez | 18 05 72 | NGC 3783 | ||
2184 | 2084 | 12 34 00 | -39 45 | 3m | lla - D | l | 3 | Smith / Gomez | 18 05 72 | NGC 4507 | ||
2185 | 2085 | 13 03 48 | -49 21 | 3m | lla - D | l | 3 | Smith / Gomez | 18 05 72 | NGC 4945 | ||
2186 | 2086 | 13 03 48 | -49 21 | 9m | lla - D | l | 2" - 3 | Smith / Gomez | 18 05 72 | NGC 4945 | ||
2187 | 2087 | 11 37 36 | -37 28 | 9m | lla - D | l | 2" - 3 | Smith / Gomez | 18 05 72 | NGC 3783 | ||
2188 | 2088 | 11 37 40 | -37 36 | 9m | lla - D | l | 2" - 3 | Smith / Gomez | 18 05 72 | NGC 3783 | ||
2189 | 2089 | 12 34 00 | -39 45 | 9m | lla - D | l | 2" - 3 | Smith / Gomez | 18 05 72 | NGC 4507 | ||
2190 | 2090 | 13 07 24 | -49 22 | 15m | lla - D | l | 2" - 3 | Smith / Gomez | 18 05 72 | NGC 4976 | ||
2191 | 2091 | 17 46 12 | -24 45 | 3m | lla - D | l | 2" - 3 | Smith / Gomez | 18 05 72 | IRC 20385 | ||
2192 | 2092 | 17 46 12 | -24 45 | 9m | lla - D | l | 2" - 3 | Smith / Gomez | 18 05 72 | IRC 20385 | ||
2193 | 2093 | 13 37 08 | -64 53 42 | 10m | lla - O | 2" - 3 | Smith / Gomez | 18 05 72 | Field Landolt | |||
2194 | 2094 | 12 34 00 | -39 45 | 60m | lla - O | 2" - 3 | Smith / Gomez | 18 05 72 | NGC 4507 | |||
2195 | 2095 | 14 30 42 | -44 04 | 60m | lla - O | 2" - 3 | Smith / Gomez | 18 05 72 | NGC 5643 | |||
2196 | 2096 | 20 16 12 | -44 54 | 123m | lla - O | 2" - 3 | Smith / Gomez | 18 05 72 | NGC 6890 |
(1) ( faltan hojas ) Corresponde a Tubo Imagen
Last Updated on 8/27/99
By Guerra & Marin
June 1972 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2197 | 2097 | 17 13 52 | -29 26 | 30m | 103a - O | GG 13 | 3 | Hesser / Zemelman | 16 06 72 | NGC 6304 | ||
2198 | 2098 | 17 13 52 | -29 26 | 30m | 103a - D | GG 14 | 3 | Hesser / Zemelman | 16 06 72 | NGC 6304 | ||
2199 | 2099 | 17 48 22 | -37 03 | 30m | 103a - D | GG 14 | 2" - 3 | Hesser / Zemelman | 16 06 72 | NGC 6441 | ||
2200 | 2100 | 17 48 22 | -37 03 | 90m | 103a - O | GG 13 | 3 | Hesser / Zemelman | 16 06 72 | NGC 6441 | ||
2201 | 2101 | 17 48 22 | -37 03 | 90m | 103a - O | GG 13 | 3 | Hesser / Zemelman | 16 06 72 | NGC 6441 | ||
2202 | 2102 | 17 48 22 | -37 03 | 30m | 103a - D | GG 14 | 3 | Hesser / Zemelman | 16 06 72 | NGC 6441 | ||
2203 | 2103 | 17 48 22 | -37 03 | 60m | 103a - O | GG 13 | 2" - 3 | Hesser / Zemelman | 16 06 72 | NGC 6441 | ||
2204 | 2104 | 17 48 22 | -37 03 | 60m | 103a - O | GG 13 | 2" - 3 | Hesser / Zemelman | 16 06 72 | NGC 6441 | ||
2205 | 2105 | 17 48 22 | -37 03 | 15m | 103a - D | GG 14 | 2" - 3 | Hesser / Zemelman | 16 06 72 | NGC 6441 | ||
2206 | 2106 | 17 48 22 | -37 03 10 | 15m | 103a - D | GG 14 | 2" - 3" | Hesser / Zemelman | 16 06 72 | NGC 6441 | ||
2207 | 2107 | 13 18 17 | - 31 30 | 30 m | 103a - D | GG 495 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | Nova en NGC 5253 | CTIO | |
2208 | 2108 | 17 12 54 | -29 26 30 | 30m | 103a - O | GG 13 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2209 | 2109 | 17 12 54 | -29 26 30 | 30m | 103a - O | GG 13 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2210 | 2110 | 17 12 54 | -29 26 30 | 30m | 103a - O | GG 13 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2211 | 2111 | 17 12 54 | -29 27 00 | 30m | 103a - D | GG 14 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2212 | 2112 | 17 12 54 | -29 27 00 | 30m | 103a - O | GG 13 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2213 | 2113 | 17 48 00 | -37 03 00 | 30m | 103a - O | GG 13 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | NGC 6441 | ||
2214 | 2114 | 17 48 00 | -37 03 00 | 30m | 103a - D | GG 14 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | NGC 6441 | ||
2215 | 2115 | 17 12 54 | -29 26 52 | 30m | 103a - O | GG 13 | 1.5" - 2" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2216 | 2116 | 17 12 54 | -29 26 52 | 30m | 103a - O | GG 13 | 2" - 3" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2217 | 2117 | 17 12 54 | -29 26 52 | 30m | 103a - D | GG 14 | 2" - 3" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2218 | 2118 | 17 12 54 | -29 26 52 | 30m | 103a - O | GG 13 | 2" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2219 | 2119 | 17 12 54 | -29 26 52 | 30m | 103a - O | GG 13 | 2" - 3" | Hesser / Zemelman | 17 06 72 | NGC 6304 | ||
2220 | 2120 | 17 12 54 | -29 26 52 | 52m | 103a - O | GG 13 | 2" - 3" | Hesser / Zemelman | 17 06 72 | NGC 6304 |
Last Updated on 8/27/99
By Guerra & Marin
July 1972 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2221 | 2121 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 2" - 1" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2222 | 2122 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 1.5" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2223 | 2123 | 17 12 54 | -29 24 30 | 30m | 103a - D | GG 14 | 1" - 2" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2224 | 2124 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 1" - 2" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2225 | 2125 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2226 | 2126 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2227 | 2127 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2228 | 2128 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2229 | 2129 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2230 | 2130 | 17 12 54 | -29 24 30 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 17 07 72 | NGC 6304 | ||
2231 | 2131 | 00 21 15 | -72 15 30 | 60m | 103a - D | GG 14 | 1" - 2" | Hesser / Gonzalez | 17 07 72 | 47 Tuc | ||
2232 | 2132 | 17 12 54.5 | -29 24 32 | 30m | 103a - O | GG 13 | 2" - 3" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2233 | 2133 | 17 12 54.5 | -29 24 32 | 30m | 103a - O | GG 13 | 1" - 2" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2234 | 2134 | 17 12 54.5 | -29 24 32 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2235 | 2135 | 30m | 103a - O | GG 13 | Hesser / Gonzalez | 18 07 72 | NGC 6441 | |||||
2236 | 2136 | 17 12 54 | -29 24 32 | 12m | 103a - D | GG 14 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | NGC 6441 | ||
2237 | 2137 | 17 12 54 | -29 24 32 | 30m | 103a - D | GG 14 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | NGC 6441 | ||
2238 | 2138 | 17 12 54 | -29 24 32 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2239 | 2139 | 17 12 54 | -29 24 32 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2240 | 2140 | 17 12 54 | -29 24 32 | 30m | 103a - D | GG 14 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2241 | 2141 | 17 12 54 | -29 24 32 | 30m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2242 | 2142 | 17 12 54 | -29 24 32 | 60m | 103a - D | GG 14 | 1" - 5" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2243 | 2143 | 17 12 54 | -29 24 32 | 30m | 103a - O | GG 13 | 1" - 5" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2244 | 2144 | 17 12 54 | -29 24 32 | 30m | 103a - O | GG 13 | 1" - 5" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2245 | 2145 | 17 12 54 | -29 24 32 | 30m | 103a - O | GG 13 | 3" - 5" | Hesser / Gonzalez | 18 07 72 | NGC 6304 | ||
2246 | 2146 | 00 21 15 | -72 15 30 | 60m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | 47 Tuc | ||
2247 | 2147 | 00 21 15 | -72 15 30 | 60m | 103a - O | GG 13 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | 47 Tuc | ||
2248 | 2148 | 00 21 15 | -72 15 30 | 20m | 103a - D | GG 14 | 1" - 3" | Hesser / Gonzalez | 18 07 72 | 47 Tuc |
Last Updated on 8/27/99
By Guerra & Marin
August 1972 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2249 | 2149 | 17 46 21 | -24 45 | 6m | lla - D | I | 3" | Smith / Gomez | 14 08 72 | IRC 20385 | image tube | |
2250 | 2150 | 17 46 21 | -24 45 | 4m | lla - D | I | 3" | Smith / Gomez | 14 08 72 | IRC 20385 | image tube | |
2251 | 2151 | 17 46 21 | -24 45 | 4m | lla - D | I | 2" | Smith / Gomez | 14 08 72 | IRC 20385 | image tube | |
2252 | 2152 | 17 46 21 | -24 45 | 4m | lla - D | I | 2" | Smith / Gomez | 14 08 72 | IRC 20385 | image tube |
Last Updated on 8/27/99
By Jorge Marin
October 1972 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2274 | 2174 | 00 25 36 | -71 39 30 | 60m | 103a - O | GG 13 | J.Graham / R.Gonzalez | 07 10 72 | NGC 121 | |||
2275 | 2175 | 00 25 36 | -71 39 30 | 60m | 103a - O | GG 13 | J.Graham / R.Gonzalez | 07 10 72 | NGC 121 | |||
2276 | 2176 | 00 25 36 | -71 39 30 | 25m | 103a - O | GG 13 | J.Graham / R.Gonzalez | 07 10 72 | NGC 121 | |||
2277 | 2177 | 00 25 36 | -71 39 30 | 60m | 103a - O | GG 13 | J.Graham / Czuia | 16 10 72 | NGC 121 | |||
2278 | 2178 | 19 59 18 | -47 07 36 | 60m | 098 - 02 | RG 2 | J.Graham / Czuia | 16 10 72 | K 30 | |||
2279 | 2179 | 00 25 36 | -71 39 36 | 60m | 103a - O | GG 13 | J.Graham / Czuia | 16 10 72 | NGC 121 | |||
2280 | 2180 | 00 07 18 | -33 59 30 | 30m | 103a - O | GG 13 | J.Graham / Czuia | 16 10 72 | SCI 3 | |||
2281 | 2181 | 00 25 36 | -71 39 30 | 60m | 103a - O | GG 13 | J.Graham / Czuia | 16 10 72 | NGC 121 | |||
2282 | 2182 | 05 28 36 | -68 50 | 10m | 103a - O | GG 13 | J.Graham / Czuia | 16 10 72 | LMC nova 72/1 | |||
2283 | 2183 | 00 25 36 | -71 39 30 | 60m | 103a - O | GG 13 | J.Graham / Czuia | 16 10 72 | NGC 121 | |||
2284 | 2184 | 00 25 36 | -71 39 30 | 60m | 103a - O | GG 13 | J.Graham / Czuia | 16 10 72 | NGC 121 | |||
2285 | 2185 | 19 59 18 | -47 08 | 120m | llla - J baked | J.Graham / Gomez | 29 10 72 | Klemola 30 | ||||
2286 | 2186 | 23 22 00 | -58 05 | 36m | 103a - O | J.Graham / Gomez | 29 10 72 | NGC 7650 | ||||
2287 | 2187 | 19 59 00 | -47 09 | 120m | 103a - O | 1.5" | J.Graham / Gomez | 30 10 72 | Klemola 30 | |||
2288 | 2188 | 23 22 00 | -58 05 | 120m | 103a - O | 2" | J.Graham / Gomez | 30 10 72 | NGC 7650 | |||
2289 | 2189 | 03 29 36 | -52 40 | 60m | 103a - O | 2" | J.Graham / Gomez | 30 10 72 | Klemola 8 | |||
2290 | 2190 | 05 28 36 | -68 50 | 5m | 103a - O | GG 13 | 2" | J.Graham / Gomez | 30 10 72 | LMC nova 1972/1 | ||
2291 | 2191 | 05 40 36 | -66 41 | 5m | 103a - O | GG 13 | 2" | J.Graham / Gomez | 30 10 72 | LMC nova 1971/2 | ||
2292 | 2192 | 04 59 00 | -66 01 | 5m | 103a - O | GG 13 | J.Graham / Gomez | 30 10 72 | NGC 1783 | |||
2293 | 2193 | 05 22 00 | -68 00 | 60m | 098 - 02 | RG 2 | 2.5" | J.Graham / Gomez | 30 10 72 | constellation l LMC |
Last Updated on 8/27/99
By Guerra & Marin
November 1972 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2294 | 2194 | 00 22 36 | -72 14 | 2m | 103a - O | J.Graham / Gomez | 19 11 72 | 47 Tuc | ||||
2295 | 2195 | 05 38 00 | -01 58 | 30m | 098 - 02 | RG 1 | R.Gonzalez | 19 11 72 | epsillon Orion | |||
2296 | 2196 | 05 39 48 | -02 26 | 90m | 098 - 02 | RG 1 | J.Graham / R.Gonzalez | 19 11 72 | epsillon Orion | |||
2297 | 2197 | 05 33 54 | -05 24 | 5m | 098 - 02 | RG 2 | J.Graham / R.Gonzalez | 19 11 72 | M 42 | |||
2298 | 2198 | 05 33 54 | -05 24 | 5m | 103a - O | GG 13 | J.Graham / R.Gonzalez | 19 11 72 | M 42 | |||
2299 | 2199 | 00 23 00 | -72 20 | 2m | 103a - D | GG 14 | 3" | Hesser / R.Gonzalez | 22 11 72 | Nova | ||
2300 | 2200 | 00 23 00 | -72 20 | 2m | lla - O | GG 13 | 3" | Hesser / R.Gonzalez | 22 11 72 | Nova | ||
2301 | 2201 | 07 50 30 | -38 25 | 10m | 103a - D | GG 14 | 2" | Hesser / R.Gonzalez | 23 11 72 | NGC 2477 | ||
2302 | 2202 | 07 50 30 | -38 25 | 10m | lla - O | GG 13 | 2" | Hesser / R.Gonzalez | 23 11 72 | NGC 2477 | ||
2303 | 2203 | 03 07 30 | -20 46 | 100m | lla - O | GG 13 | 3" | R.Gonzalez | 24 11 72 | NGC 1232 | ||
2304 | 2204 | 06 29 36 | +04 40 | 180m | 098 - 02 | RG 1 | 3" | R.Gonzalez | 24 11 72 | NGC 2237 |
Last Updated on 8/27/99
By Guerra & Marin
1973 Plate logs for 1.5-m telescope.
January 1973 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2314 | 2214 | 04 28 30 | -53 59 | 60m | 103a - D | GG 14 | 1.5" | Sersic / Czuia | 13 01 73 | IC 2082 | ||
2315 | 2215 | 07 36 24 | -69 28 06 | 90m | 098 - 02 | RG 2 | Sersic / Czuia | 13 01 73 | NGC 2442 | |||
2316 | 2216 | 07 36 24 | -69 28 06 | 80m | 103a - D | GG 14 | Sersic / Czuia | 13 01 73 | NGC 2442 | |||
2317 | 2217 | 07 36 24 | -69 28 06 | 80m | 103a - O | GG 13 | Sersic / Czuia | 13 01 73 | NGC 2442 | |||
2318 | 2218 | 13 38 12 | -31 29 | 55m | 103a - D | GG 14 | Sersic / Czuia | 13 01 73 | NGC 5253 |
Last Updated on 8/27/99
By Guerra & Marin
February 1973 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2319 | 2219 | 07 24 12 | -21 07 36 | 15m | 103a - D | GG 13 | Miller / Zemelman | 08 02 73 | Vela F | |||
2320 | 2220 | 07 24 12 | -20 54 | 15m | 103a - D | GG 13 | Miller / Zemelman | 08 02 73 | Vela F | |||
2321 | 2221 | 07 24 12 | -20 54 | 40m | 103a - O | UG 2 | Miller / Zemelman | 08 02 73 | Vela F | |||
2322 | 2222 | 07 24 12 | -20 54 | 8m | 103a - O | GG 13 | Miller / Zemelman | 08 02 73 | Vela F | |||
2323 | 2223 | 07 24 12 | -20 54 | 15m | 103a - D | GG 14 | Miller / Zemelman | 08 02 73 | Vela F | |||
2324 | 2224 | 07 44 36 | -34 08 | 15m | 103a - D | GG 14 | Miller / Zemelman | 08 02 73 | Vela D | |||
2325 | 2225 | 07 44 36 | -34 08 | 40m | 103a - O | UG 2 | Miller / Zemelman | 08 02 73 | Vela D | |||
2326 | 2226 | 07 44 36 | -34 08 | 8m | 103a - O | GG 13 | 1" | Miller / Zemelman | 08 02 73 | Vela D | ||
2327 | 2227 | 07 57 48 | -28 23 | 8m | 103a - O | GG 13 | 1" | Miller / Zemelman | 08 02 73 | Vela B | ||
2328 | 2228 | 07 57 48 | -28 23 | 40m | 103a - O | UG 2 | 1" | Miller / Zemelman | 08 02 73 | Vela B | ||
2329 | 2229 | 07 57 48 | -28 23 | 15m | 103a - D | GG 14 | 1" | Miller / Zemelman | 08 02 73 | Vela B | ||
2330 | 2230 | 10 59 00 | -60 10 | 60m | 098 - 02 | RG 2 | 1" | Miller / Zemelman | 08 02 73 | HD 95540 | ||
2331 | 2231 | 10 59 00 | -60 10 | 10m | 103a - O | GG 13 | 1" | Miller / Zemelman | 08 02 73 | HD 95540 | ||
2332 | 2232 | 10 59 00 | -60 10 | 5m | 103a - D | GG 14 | 1" | Miller / Zemelman | 08 02 73 | HD 95540 | ||
2333 | 2233 | 07 45 42 | -34 09 | 30m | 103a - O | UG 2 | 2" | Miller / Bolelli | 09 02 73 | Vela D | ||
2334 | 2234 | 07 45 42 | -34 09 | 10m | 103a - O | GG 13 | 2" | Miller / Bolelli | 09 02 73 | Vela D | ||
2335 | 2235 | 07 45 42 | -34 09 | 10m | 103a - D | GG 14 | 2" | Miller / Bolelli | 09 02 73 | Vela D | ||
2336 | 2236 | 07 57 48 | -28 23 | 10m | 103a - D | GG 14 | 2" | Miller / Bolelli | 09 02 73 | Vela B | ||
2337 | 2237 | 07 57 48 | -28 23 | 30m | 103a - O | UG 2 | 2" | Miller / Bolelli | 09 02 73 | Vela B | ||
2338 | 2238 | 07 57 48 | -28 23 | 8m | 103a - O | GG 13 | 2" | Miller / Bolelli | 09 02 73 | Vela B | ||
2339 | 2239 | 07 24 06 | -21 07 | 10m | 103a - D | GG 14 | 2" | Miller / Bolelli | 09 02 73 | Vela F | ||
2340 | 2240 | 07 24 06 | -21 07 | 10m | 103a - D | GG 14 | 2" | Miller / Bolelli | 09 02 73 | Vela F | ||
2341 | 2241 | 07 24 06 | -21 07 | 8m | 103a - O | GG 13 | 2" | Miller / Bolelli | 09 02 73 | Vela F | ||
2342 | 2242 | 07 24 06 | -21 07 | 30m | 103a - O | UG 2 | 2" | Miller / Bolelli | 09 02 73 | Vela F | ||
2343 | 2243 | 07 43 54 | -31 50 | 10m | 103a - D | GG 14 | 2" | Miller / Bolelli | 09 02 73 | Vela A | ||
2344 | 2244 | 07 43 54 | -31 50 | 8m | 103a - O | GG 13 | 2" | Miller / Bolelli | 09 02 73 | Vela A | ||
2345 | 2245 | 07 43 54 | -31 50 | 30m | 103a - O | UG 2 | 2" | Miller / Bolelli | 09 02 73 | Vela A | ||
2346 | 2246 | 08 57 00 | -46 58 | 10m | 103a - D | GG 14 | 2" | Miller / Bolelli | 09 02 73 | RCW 38 | ||
2347 | 2247 | 08 57 00 | -46 58 | 8m | 103a - O | GG 13 | 2" | Miller / Bolelli | 09 02 73 | RCW 38 | ||
2348 | 2248 | 08 57 00 | -46 58 | 30m | 103a - O | UG 2 | 2" | Miller / Bolelli | 09 02 73 | RCW 38 | ||
2349 | 2249 | 14 19 54 | -60 48 | 10m | 103a - D | GG 14 | 2" | Miller / Bolelli | 09 02 73 | Cen l | ||
2350 | 2250 | 14 19 54 | -60 48 | 10m | 103a - D | GG 14 | 2" | Miller / Bolelli | 09 02 73 | Cen l | ||
2351 | 2251 | 07 43 54 | -31 50 | 10m | 103a - D | GG 14 | 2" | Miller / Zemelman | 09 02 73 | Vela A | ||
2352 | 2252 | 07 43 54 | -31 50 | 30m | 103a - O | UG 2 | 2" | Miller / Zemelman | 10 02 73 | Vela A | ||
2353 | 2253 | 07 43 54 | -31 50 | 30m | 103a - O | UG 2 | 2" | Miller / Zemelman | 10 02 73 | Vela A | ||
2354 | 2254 | 07 43 54 | -31 50 | 10m | 103a - D | GG 14 | 2" | Miller / Zemelman | 10 02 73 | Vela A | ||
2355 | 2255 | 07 43 54 | -31 50 | 8m | 103a - O | GG 13 | 2" | Miller / Zemelman | 10 02 73 | Vela A | ||
2356 | 2256 | 07 43 54 | -31 50 | 8m | 103a - O | GG 13 | 2" - 3" | Miller / Zemelman | 10 02 73 | Vela A | ||
2357 | 2257 | 07 58 00 | -28 32 | 8m | 103a - O | GG 13 | 3" - 4" | Miller / Zemelman | 10 02 73 | Vela B | ||
2358 | 2258 | 07 58 00 | -28 32 | 8m | 103a - O | GG 13 | 3" - 4" | Miller / Zemelman | 10 02 73 | Vela B | ||
2359 | 2259 | 07 58 00 | -28 32 | 40m | 103a - O | UG 2 | 3" - 4" | Miller / Zemelman | 10 02 73 | Vela B | ||
2360 | 2260 | 07 58 00 | -28 32 | 10m | 103a - D | GG 14 | 3" - 4" | Miller / Zemelman | 10 02 73 | Vela B | ||
2361 | 2261 | 08 56 12 | -47 40 | 10m | 103a - D | GG 14 | 3" - 4" | Miller / Zemelman | 10 02 73 | RCW 38 | ||
2362 | 2262 | 08 56 12 | -47 40 | 8m | 103a - O | GG 13 | 3" - 4" | Miller / Zemelman | 10 02 73 | RCW 38 | ||
2363 | 2263 | 08 56 12 | -47 40 | 20m | 103a - O | UG 2 | 3" - 4" | Miller / Zemelman | 10 02 73 | RCW 38 | ||
2364 | 2264 | 07 24 06 | -21 07 36 | 10m | 103a - D | GG 14 | 3" - 4" | Miller / Zemelman | 10 02 73 | Vela F | ||
2365 | 2265 | 10 59 00 | -60 10 | 8m | 103a - O | GG 13 | 3" - 4" | Miller / Zemelman | 10 02 73 | HD 95540 | ||
2366 | 2266 | 10 59 00 | -60 10 | 10m | 103a - O | UG 2 | 3" - 4" | Miller / Zemelman | 10 02 73 | HD 95540 | ||
2367 | 2267 | 14 19 54 | -60 48 | 5m | 103a - O | GG 13 | 3" - 4" | Miller / Zemelman | 10 02 73 | Cen I | ||
2368 | 2268 | 14 19 54 | -60 48 | 30m | 103a - D | GG 14 | 3" - 4" | Miller / Zemelman | 10 02 73 | Cen I | ||
2369 | 2269 | 07 45 00 | -34 42 | 5m | lla - O | 2" | Miller / Zemelman | 11 02 73 | Vela D | |||
2370 | 2270 | 07 45 00 | -34 42 | 40m | lla - O | 2" | Miller / Zemelman | 11 02 73 | Vela D | |||
2371 | 2271 | 07 45 00 | -34 42 | 32m | lla - O | 2" | Miller / Zemelman | 11 02 73 | Vela D | |||
2372 | 2272 | 07 24 06 | -21 07 36 | 30m | 103a - O | 2" | Miller / Zemelman | 11 02 73 | Vela F | |||
2373 | 2273 | 07 58 00 | -28 31 | 30m | 103a - O | 2" | Miller / Zemelman | 11 02 73 | Vela F | |||
2374 | 2274 | 07 43 54 | -31 50 | 30m | 103a - O | 2" | Miller / Zemelman | 11 02 73 | Vela A | |||
2375 | 2275 | 08 56 12 | -47 40 | 30m | 103a - O | 2" | Miller / Zemelman | 11 02 73 | RCW 38 | |||
2376 | 2276 | 14 19 54 | -60 48 | 30m | 103a - O | 2" | Miller / Zemelman | 11 02 73 | Cen I | |||
2377 | 2277 | 11 00 25 | -59 35 | 30m | 103a - O | 2" | Miller / Zemelman | 11 02 73 | HD 95540 | |||
2378 | 2278 | 10 59 54 | -60 05 | 35m | 098 - 02 | 2" | Miller / Zemelman | 11 02 73 | HD 95540 | |||
2379 | 2279 | 11 02 54 | -60 33 | 10m | 098 - 02 | 2" | Miller / Zemelman | 11 02 73 | HD 95540 | |||
2380 | 2280 | 04 20 00 | -48 20 | 60m | 103a - O | UG 2 | 2" | Graham / Elicer / Gonzalez | 11 02 73 | galaxy | ||
2381 | 2281 | 06 43 00 | -74 20 | 60m | 103a - O | 2" | Graham / Elicer / Gonzalez | 11 02 73 | galaxy ring type | |||
2382 | 2282 | 06 43 00 | -74 20 | 120m | 098 - 02 | GG 13 | 2" | Graham / Elicer / Gonzalez | 11 02 73 | galaxy ring type | ||
2383 | 2283 | 13 19 00 | -43 31 | 15m | 098 - 02 | RG 1 | 2" | Graham / Elicer / Gonzalez | 11 02 73 | NGC 5090 | ||
2384 | 2284 | 04 20 00 | -48 20 | 10m | 103a - D | GG 14 | 2" | Graham / Czuia / Elicer | 25 02 73 | galaxy | ||
2385 | 2285 | 04 20 00 | -48 20 | 30m | 103a - O | GG 13 | Graham / Czuia / Elicer | 25 02 73 | galaxy | |||
2386 | 2286 | 04 20 00 | -48 20 | 6m | 103a - O | GG 13 | Graham / Czuia / Elicer | 25 02 73 | galaxy | |||
2387 | 2287 | 10 07 48 | -38 15 | 90m | 103a - O | Graham / Czuia / Elicer | 25 02 73 | Anom 10 07 - 38 | ||||
2388 | 2288 | 10 07 48 | -38 15 | 120m | 098 - 02 | GG 14 | Graham / Czuia / Elicer | 25 02 73 | Anom 10 07 - 38 | |||
2389 | 2289 | 13 19 00 | +43 31 | 40m | 103a - O | GG 13 | Graham / Czuia / Elicer | 25 02 73 | NGC 5090 |
Last Updated on 8/27/99
By Guerra & Marin
April 1973 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2396 | 2296 | 09 44 00 | -31 04 | 60m | lla - O | 1.5" | Sersic / Czuia | 10 04 73 | N 2997 | |||
2397 | 2297 | 10 26 42 | -39 48 | 60m | lla - O | 1.5" | Sersic / Czuia | 10 04 73 | N 3256 | |||
2398 | 2298 | 13 20 30 | -38 13 | 59m | lla - O | GG 13 | 2" | Sersic / Czuia | 10 04 73 | N 5102 | ||
2399 | 2299 | 13 20 30 | -38 13 | 7m | lla - D | GG 14 | 2" | Sersic / Czuia | 10 04 73 | N 5102 | ||
2400 | 2300 | 13 38 24 | -31 31 | 60m | lla - D | GG 14 | 2" | Sersic / Czuia | 10 04 73 | N 5253 | ||
2401 | 2301 | 13 38 24 | -31 31 | 61m | lla - D | GG 13 | 2" | Sersic / Czuia | 10 04 73 | N 5253 | ||
2402 | 2302 | 56m | lla - D | GG 13 | 2.5" | Sersic / Czuia | 10 04 73 | N 6438 | ||||
2403 | 2303 | 09 44 30 | -31 04 | 61m | lla - D | GG 14 | 1.5" | Sersic / Czuia | 11 04 73 | N 2997 | ||
2404 | 2304 | 10 26 42 | -43 45 | 60m | lla - D | GG 14 | Sersic / Czuia | 11 04 73 | N 3256 | |||
2405 | 2305 | 10 26 42 | -43 45 | 60m | lla - O | GG 13 | 1.5" | Sersic / Czuia | 11 04 73 | N 3256 | ||
2406 | 2306 | 13 38 24 | -31 31 | 60m | 098 - 02 | RG 2 | Sersic / Czuia | 11 04 73 | N 5253 | |||
2407 | 2307 | 13 19 30 | -36 19 | 60m | lla - O | GG 13 | Sersic / Czuia | 11 04 73 | N 5102 | |||
2408 | 2308 | 13 19 30 | -36 19 | 60m | lla - D | GG 13 | Sersic / Czuia | 11 04 73 | N 5102 | |||
2409 | 2309 | 13 23 48 | -42 52 | 120m | 103a - D | GG 5 | Sersic / Czuia | 11 04 73 | N 5128 | |||
2410 | 2310 | 13 34 48 | -33 39 | 60m | lla - D | GG 14 | 1.5" | Sersic / Czuia | 12 04 73 | IC 4296 | ||
2411 | 2311 | 13 34 48 | -33 39 | 60m | lla - O | GG 13 | Sersic / Czuia | 12 04 73 | IC 4296 | |||
2412 | 2312 | 13 19 30 | -36 19 | 60m | lla - O | GG 13 | Sersic / Czuia | 12 04 73 | N 5102 | |||
2413 | 2313 | 13 19 30 | -36 19 | 60m | lla - D | GG 14 | Sersic / Czuia | 12 04 73 | N 5102 | |||
2414 | 2314 | 20 12 06 | -71 01 | 150m | 103a - D | Sersic / Czuia | 12 04 73 | T P |
Last Updated on 8/27/99
By Jorge Marin
June 1973 Plate logs for 1.5-m telescope
December 1973 Plate logs for 1.5-m telescope
1974 Plate logs for 1.5-m telescope
January 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2553 | 2453 | 04 20 18 | -68 20 | 17m | RG 2 | 08 01 74 | NGC 1567 | |||||
2554 | 2454 | 05 33 48 | -05 25 | 15m | RG 2 | 08 01 74 | Orion nebulae | |||||
2555 | 2455 | 03 59 24 | -67 42 | 60m | 098 - 02 | RG 1 | Graham / Gonzalez /Elicer | 08 01 74 | NGC 1511 | |||
2556 | 2456 | 06 27 00 | -47 05 | 45m | 098 - 02 | RG 1 | Graham / Gonzalez / Elicer | 08 01 74 | peculiar niple | |||
2557 | 2457 | 08 25 24 | -68 02 | 45m | 098 - 02 | RG 1 | Graham / Gonzalez / Elicer | 08 01 74 | NGC 2601 | |||
2558 | 2458 | 09 26 06 | -76 37 | 45m | 098 - 02 | RG 1 | Graham / Gonzalez / Elicer | 08 01 74 | NGC 2915 | |||
2559 | 2459 | 04 20 18 | -48 20 | 15m | 098 - 02 | RG 1 | Graham / Gomez / Elicer | 09 01 74 | NGC 1567 ecliptical galaxy | |||
2560 | 2460 | 06 27 00 | -47 05 | 90m | 098 - 02 | RG 1 | Graham / Gomez / Elicer | 09 01 74 | peculiar niple | |||
2561 | 2461 | 09 26 06 | -76 37 | 90m | 098 - 02 | RG 1 | Graham / Gomez / Elicer | 09 01 74 | NGC 2915 | |||
2562 | 2462 | 06 28 50 | -28 34 | 120 m | lla - O | GG 385 | 2" | R.Gonzalez | 22 01 74 | BSR 0628 - 28 | CTIO | |
2563 | 2463 | 08 18 06 | -13 41 | 90 m | lla - O | GG 385 | 2" | R.Gonzalez | 22 01 74 | BSR 0818 - 13 | CTIO | |
2564 | 2464 | 07 36 51 | -40 34 30 | 90 m | lla - O | GG 385 | 2" | R.Gonzalez | 22 01 74 | BSR 0736 - 40 | CTIO | |
2565 | 2465 | 07 24 06 | -21 07 36 | 40m | 103a - O | UG 2 | 2" | Miller / R.Gonzalez | 23 01 74 | HD 58510 | ||
2566 | 2466 | 07 24 06 | -21 07 36 | 40m | 103a - O | UG 2 | 2" | Miller / R.Gonzalez | 23 01 74 | HD 58510 | ||
2567 | 2467 | 07 24 06 | -21 07 36 | 10m | 103a - O | GG 13 | 2" | Miller / R.Gonzalez | 23 01 74 | HD 58510 | ||
2568 | 2468 | 07 24 06 | -21 07 36 | 10m | 103a - O | GG 13 | 2" | Miller / R.Gonzalez | 23 01 74 | HD 58510 | ||
2569 | 2469 | 07 24 06 | -21 07 36 | 15m | 103a - O | GG 13 | 2" | Miller / R.Gonzalez | 23 01 74 | HD 58510 | ||
2570 | 2470 | 07 24 06 | -21 07 36 | 15m | 103a - D | GG 14 | 2" | Miller / R.Gonzalez | 23 01 74 | HD 58510 | ||
2571 | 2471 | 07 24 06 | -21 07 36 | 40m | 103a - D | GG 14 | 2" | Miller / R.Gonzalez | 23 01 74 | HD 58510 | ||
2572 | 2472 | 07 57 48 | -28 30 | 40m | 103a - O | UG 2 | Miller / R.Gonzalez | 23 01 74 | Vela B | |||
2573 | 2473 | 07 57 48 | -28 30 | 40m | 103a - O | UG 2 | Miller / R.Gonzalez | 23 01 74 | Vela B | |||
2574 | 2474 | 07 57 48 | -28 30 | 15m | 103a - D | GG 14 | Miller / R.Gonzalez | 23 01 74 | Vela B | |||
2575 | 2475 | 08 57 48 | -47 36 | 40m | 103a - O | UG 2 | Miller / R.Gonzalez | 23 01 74 | RCW 38 | |||
2576 | 2476 | 08 57 48 | -47 36 | 15m | 103a - D | GG 14 | Miller / R.Gonzalez | 23 01 74 | RCW 38 | |||
2577 | 2477 | 07 24 06 | -21 07 36 | 40m | 103a - O | UG 2 | Miller / R.Gonzalez | 23 01 74 | HD 58510 | |||
2578 | 2478 | 07 24 06 | -21 07 36 | 10m | 103a - O | GG 13 | Miller / R.Gonzalez | 24 01 74 | HD 58510 | |||
2579 | 2479 | 07 57 48 | -28 30 | 40m | 103a - O | UG 2 | Miller / R.Gonzalez | 24 01 74 | Vela B | |||
2580 | 2480 | 07 57 48 | -28 30 | 10m | 103a - O | GG 13 | Miller / R.Gonzalez | 24 01 74 | Vela B | |||
2581 | 2481 | 08 57 48 | -47 36 | 40m/10m | 103a - O | UG 2 / GG 13 | 3" | Miller / R.Gonzalez | 24 01 74 | RCW 38 | ||
2582 | 2482 | 08 57 48 | -47 36 | 40m/10m | 103a - O | UG 2 / GG 13 | 3" | Miller / R.Gonzalez | 24 01 74 | RCW 38 | ||
2583 | 2483 | 08 57 48 | -47 36 | 10m/40m | 103a - O | GG 13 / UG 2 | 3" | Miller / R.Gonzalez | 24 01 74 | RCW 38 | ||
2584 | 2484 | 08 36 24 | -45 07 | 40m/10m | 103a - O | UG 2 / GG 13 | 3" | Miller / R.Gonzalez | 24 01 74 | HD 73568 | ||
2585 | 2485 | 08 36 24 | -45 07 | 10m/40m | 103a - O | GG 13 / UG 2 | 3" | Miller / R.Gonzalez | 24 01 74 | HD 73568 |
Last Updated on 8/27/99
By Guerra & Marin
February 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2586 | 2486 | 03 59 24 | -67 42 | 60m | 103a - O | Graham / Saá / Elicer | 22 02 74 | NGC 1511 | ||||
2587 | 2487 | 06 27 00 | -47 05 | 90m | 103a - O | Graham / Saá / Elicer | 22 02 74 | faint group of galaxies | ||||
2588 | 2488 | 06 25 54 | -53 40 | 30m | 103a - O | Graham / Saá / Elicer | 22 02 74 | PKS 625 - 53 | ||||
2589 | 2489 | 09 25 00 | -76 51 | 90m | 103a - O | Graham / Saá / Elicer | 22 02 74 | NGC 2915 | ||||
2590 | 2490 | 09 25 00 | -76 51 | 60m | 103a - O | Graham / Saá / Elicer | 22 02 74 | NGC 2915 | ||||
2591 | 2491 | 15 16 12 | -24 15 | 75m | 103a - O | Graham / Saá / Elicer | 22 02 74 | AP Librae |
Last Updated on 8/27/99
By Guerra & Marin
March 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2592 | 2492 | 06 27 00 | -47 05 | 3m | llla - J | Graham / Richer / Czuia | 22 03 74 | grupo de galaxias | ||||
2593 | 2493 | 13 04 42 | -37 26 | llla - J | Graham / Richer / Czuia | 22 03 74 | NGC 4953 | |||||
2594 | 2494 | 18 41 00 | -48 39 | 118m | llla - J | Graham / Richer / Czuia | 22 03 74 | PKS 1839 - 48 | ||||
2595 | 2495 | 10 36 12 | -27 18 | 33m | lla - O | GG 13 | Smith / Weedman / Czuia | 25 03 74 | Hydra l cluster of galaxies | |||
2596 | 2496 | 12 48 24 | -41 08 | 30m | lla - O | GG 13 | Smith / Weedman / Czuia | 25 03 74 | Centaurus cluster | |||
2597 | 2497 | 12 48 24 | -41 08 | 90m | lla - O | GG 13 | Smith / Weedman / Czuia | 25 03 74 | Centaurus cluster | |||
2598 | 2498 | 10 36 12 | -27 18 | 30m | lla - O | Smith / Weedman / Czuia | 26 03 74 | Hydra l cluster | ||||
2599 | 2499 | 10 36 12 | -27 18 | 180m | llla - J | Smith / Weedman / Czuia | 26 03 74 | Hydra l cluster | ||||
2600 | 2500 | 12 48 50 | -41 15 48 | 180m | llla - J | Smith / Weedman / Czuia | 26 03 74 | Centaurus cluster | ||||
2601 | 2501 | 12 43 54 | -40 36 22 | 30m | lla - O | Smith / Weedman / Czuia | 26 03 74 | Centaurus cluster | ||||
2602 | 2502 | 18 17 12 | -13 47 47 | 32m | llla - J | Smith / Weedman / Czuia | 26 03 74 | M 16 |
Last Updated on 8/27/99
By Guerra & Marin
April 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2603 | 2503 | 12 38 06 | -26 36 54 | 10m | 103a - D | GG 14 | 1" | Hesser / Gonzalez | 25 04 74 | NGC 4590 | ||
2604 | 2504 | 12 38 06 | -26 36 54 | 13m | 103a - O | GG 385 | 1" | Hesser / Gonzalez | 25 04 74 | NGC 4590 | ||
2605 | 2505 | 12 38 06 | -26 36 54 | 60m | 103a - D | GG 14 | 1" | Hesser / Gonzalez | 25 04 74 | NGC 4590 | ||
2606 | 2506 | 12 38 06 | -26 36 54 | 60m | 103a - O | GG 385 | 1" | Hesser / Gonzalez | 25 04 74 | NGC 4590 | ||
2607 | 2507 | 13 44 30 | -51 14 | 60m | 103a - D | GG 14 | 1" | Hesser / Gonzalez | 25 04 74 | NGC 5286 | ||
2608 | 2508 | 13 44 30 | -51 14 | 60m | 103a - O | GG 385 | < 1" | Hesser / Gonzalez | 25 04 74 | NGC 5286 | ||
2609 | 2509 | 17 23 30 | -48 27 | 120m | 103a - D | GG 14 | 1" - 1.5" | Hesser / Gonzalez | 25 04 74 | NGC 6352 | ||
2610 | 2510 | 17 23 30 | -48 27 | 56m | 103a - O | GG 385 | 1" - 2" | Hesser / Gonzalez | 25 04 74 | NGC 6352 | ||
2611 | 2511 | 12 38 06 | -26 36 54 | 20m | 103a - O | GG 385 | 1.5" - 2" | Hesser / Gonzalez | 26 04 74 | NGC 4590 | ||
2612 | 2512 | 12 38 06 | -26 36 54 | 20m | 103a - O | GG 385 | 2" | Hesser / Gonzalez | 26 04 74 | NGC 4590 | ||
2613 | 2513 | 12 38 06 | -26 36 54 | 60m | 103a - D | GG 14 | 1.5" | Hesser / Gonzalez | 26 04 74 | NGC 4590 | ||
2614 | 2514 | 12 38 06 | -26 36 54 | 40m | 103a - O | GG 385 | 1" - 2" | Hesser / Gonzalez | 26 04 74 | NGC 4590 | ||
2615 | 2515 | 14 57 00 | -82 08 | 120m | 103a - D | GG 14 | 2" - 2.5" | Hesser / Gonzalez | 26 04 74 | IC 4499 | ||
2616 | 2516 | 17 23 30 | -48 27 | 115m | 103a - D | GG 14 | 1.5" | Hesser / Gonzalez | 26 04 74 | NGC 6352 | ||
2617 | 2517 | 17 23 30 | -48 27 | 120m | 103a - O | GG 385 | 1.5" - 2" | Hesser / Gonzalez | 26 04 74 | NGC 6352 |
Last Updated on 8/27/99
By Jorge Marin
May 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2618 | 2518 | 18 34 48 | -23 57 | 20m | 103a - D | GG 14 | 2" - 3" | Hesser / Czuia / Poblete | 25 05 74 | M 22 | ||
2619 | 2519 | 18 34 48 | -23 57 | 20m | 103a - O | GG 385 | 3" | Hesser / Czuia / Poblete | 25 05 74 | M 22 | ||
2620 | 2520 | 18 34 48 | -23 57 | 60m | 103a - D | GG 14 | 3" | Hesser / Czuia / Poblete | 25 05 74 | M 22 | ||
2621 | 2521 | 13 44 00 | -51 14 | 60m | 103a - D | GG 14 | 3" | Hesser / Czuia / Poblete | 26 05 74 | NGC 5286 | ||
2622 | 2522 | 13 44 00 | -51 14 | 0.5m | 103a - O | GG 385 | 2" | Hesser / Czuia / Poblete | 26 05 74 | NGC 5286 | ||
2623 | 2523 | 13 44 00 | -51 14 | 0.5m | 103a - O | GG 385 | 2.5" | Hesser / Czuia / Poblete | 26 05 74 | NGC 5286 | ||
2624 | 2524 | 13 44 00 | -51 14 | 0.5m | 103a - O | GG 385 | 2.5" | Hesser / Czuia / Poblete | 26 05 74 | NGC 5286 | ||
2625 | 2525 | 13 44 00 | -51 14 | 0.5m | 103a - D | GG 14 | 2.5" | Hesser / Czuia / Poblete | 26 05 74 | NGC 5286 | ||
2626 | 2526 | 13 44 00 | -51 14 | 0.5m | 103a - D | GG 14 | 2.5" | Hesser / Czuia / Poblete | 26 05 74 | NGC 5286 | ||
2627 | 2527 | 13 44 00 | -51 14 | 0.5m | 103a - D | GG 14 | 2.5" | Hesser / Czuia / Poblete | 26 05 74 | NGC 5286 | ||
2628 | 2528 | 13 44 00 | -51 14 | 0.5m | 103a - O | GG 385 | 2.5" | Hesser / Czuia / Poblete | 26 05 74 | NGC 5286 | ||
2629 | 2529 | 17 23 00 | -48 27 | 60m | 103a - D | GG 14 | 2.5" | Hesser / Czuia / Poblete | 26 05 74 | NGC 6352 | ||
2630 | 2530 | 17 23 00 | -48 27 | 60m | 103a - O | GG 385 | 2.5" | Hesser / Czuia / Poblete | 26 05 74 | NGC 6352 | ||
2631 | 2531 | 17 23 00 | -48 27 | 120m | 103a - O | GG 385 | 2" | Hesser / Czuia / Poblete | 26 05 74 | NGC 6352 | ||
2632 | 2532 | 17 23 00 | -48 27 | 120m | 103a - D | GG 14 | 1.5" - 2" | Hesser / Czuia / Poblete | 26 05 74 | NGC 6352 | ||
2633 | 2533 | 18 34 48 | -23 57 | 20m | 103a - D | GG 14 | 1.5" - 2" | Hesser / Czuia / Poblete | 26 05 74 | M 22 | ||
2634 | 2534 | 18 34 48 | -23 57 | 20m | 103a - O | GG 385 | 1.5" - 2" | Hesser / Czuia / Poblete | 26 05 74 | M 22 | ||
2635 | 2535 | 18 34 48 | -23 57 | 5m | 103a - O | GG 385 | 1.5" - 2" | Hesser / Czuia / Poblete | 26 05 74 | M 22 | ||
2636 | 2536 | 18 34 48 | -23 57 | 5m | 103a - O | GG 385 | 1.5" | Hesser / Czuia / Poblete | 26 05 74 | M 22 | ||
2637 | 2537 | 18 34 48 | -23 57 | 5m | 103a - D | GG 14 | 1.5" | Hesser / Czuia / Poblete | 26 05 74 | M 22 | ||
2638 | 2538 | 18 34 48 | -23 57 | 5m | 103a - D | GG 14 | 1.5" | Hesser / Czuia / Poblete | 26 05 74 | M 22 |
Last Updated on 8/27/99
By Guerra & Marin
June 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2639 | 2539 | 18 05 42 | -24 40 | 25m | lla - O | UG 2 | 2" - 3" | Racine / R.Gonzalez | 29 06 74 | NGC 6544 | ||
2640 | 2540 | 18 05 42 | -24 40 | 15m | lla - O | UG 2 | 2" - 3" | Racine / R.Gonzalez | 29 06 74 | NGC 6544 | ||
2641 | 2541 | 18 05 42 | -24 40 | 3m | lla - D | GG 14 | 2" - 5" | Racine / R.Gonzalez | 29 06 74 | NGC 6544 | ||
2642 | 2542 | 18 05 42 | -24 40 | 1m | lla - D | GG 14 | 2" - 5" | Racine / R.Gonzalez | 29 06 74 | NGC 6544 | ||
2643 | 2543 | 18 07 36 | -25 35 | 6m | lla - O | GG 14 | 2" - 5" | Racine / R.Gonzalez | 29 06 74 | NGC 6553 | ||
2644 | 2544 | 18 07 36 | -25 35 | 20m | lla - D | UG 2 | 2" - 5" | Racine / R.Gonzalez | 29 06 74 | NGC 6553 | ||
2645 | 2545 | 18 08 24 | -31 26 | 30m | lla - O | UG 2 | 2" - 20" | Racine / R.Gonzalez | 30 06 74 | NGC 6558 | ||
2646 | 2546 | 18 08 24 | -31 26 | 8m | lla - D | GG 14 | 2" - 20" | Racine / R.Gonzalez | 30 06 74 | NGC 6558 | ||
2647 | 2547 | 21 44 54 | -21 22 | 4m | lla - D | GG 14 | 2" - 20" | Racine / R.Gonzalez | 30 06 74 | Pal 12 | ||
2648 | 2548 | 21 44 54 | -21 22 | 25m | lla - O | UG 2 | 2" - 20" | Racine / R.Gonzalez | 30 06 74 | Pal 12 | ||
2649 | 2549 | 19 43 42 | -07 46 | 3m | lla - D | GG 14 | 2" - 4" | Racine / R.Gonzalez | 30 06 74 | Pal 11 | ||
2650 | 2550 | 19 43 42 | -07 46 | 20m | lla - O | UG 2 | 2" - 4" | Racine / R.Gonzalez | 30 06 74 | Pal 11 | ||
2651 | 2551 | 21 31 54 | -00 58 | 3m | lla - O | UG 2 | 3" - 10" | Racine / R.Gonzalez | 30 06 74 | NGC 7089 | ||
2652 | 2552 | 21 31 54 | -00 58 | 15m | lla - O | UG 2 | 3" - 10" | Racine / R.Gonzalez | 30 06 74 | NGC 7089 | ||
2653 | 2553 | 21 31 54 | -00 58 | 40s | lla - D | GG 14 | 3" - 10" | Racine / R.Gonzalez | 30 06 74 | NGC 7089 | ||
2654 | 2554 | 21 31 54 | -00 58 | 3m | lla - D | GG 14 | 3" - 10" | Racine / R.Gonzalez | 30 06 74 | NGC 7089 |
Last Updated on 8/27/99
By Guerra & Marin
July 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2655 | 2555 | 16 25 48 | -38 25 | 10m | lla - D | GG 14 | 5" | Racine / R.Gonzalez | 01 07 74 | NGC 6139 | ||
2656 | 2556 | 16 25 48 | -38 25 | 5m | lla - O | GG 385 | 5" | Racine / R.Gonzalez | 01 07 74 | NGC 6139 | ||
2657 | 2557 | 17 14 42 | -27 46 | 10m | lla - D | GG 14 | 6" - 10" | Racine / R.Gonzalez | 01 07 74 | NGC 6316 | ||
2658 | 2558 | 17 14 42 | -27 46 | 5m | lla - O | GG 385 | 8" - 10" | Racine / R.Gonzalez | 01 07 74 | NGC 6316 | ||
2659 | 2559 | 17 19 30 | -19 13 | 10m | lla - D | GG 14 | 4" | Racine / R.Gonzalez | 01 07 74 | NGC 6342 | ||
2660 | 2560 | 17 19 30 | -19 13 | 5m | lla - O | GG 385 | Racine / R.Gonzalez | 01 07 74 | NGC 6342 | |||
2661 | 2561 | 17 22 12 | -25 59 | 10m | lla - D | GG 14 | 4" | Racine / R.Gonzalez | 01 07 74 | NGC 6355 | ||
2662 | 2562 | 17 22 12 | -25 59 | 5m | lla - O | GG 385 | Racine / R.Gonzalez | 01 07 74 | NGC 6355 | |||
2663 | 2563 | 17 36 54 | -23 33 | 10m | lla - D | GG 14 | 3" | Racine / R.Gonzalez | 01 07 74 | NGC 6401 | ||
2664 | 2564 | 17 36 54 | -23 33 | 5m | lla - O | GG 385 | Racine / R.Gonzalez | 01 07 74 | NGC 6401 | |||
2564 | 13 04 00 | -49 21 | 60m | 103a - O | 1" | Racine / R.Gonzalez | 21 07 74 | NGC 4945 | ||||
2665 | 2565 | 13 29 00 | -86 24 | 115m | 103a - O | 1" | Racine / R.Gonzalez | 21 07 74 | cumulo de galaxias | |||
2666 | 2566 | 20 43 00 | -55 10 | 90m | 103a - O | 1" | Racine / R.Gonzalez | 21 07 74 | grupo de galaxias | |||
2667 | 2567 | 22 46 00 | -58 04 | 120m | llla - J | 2" | Racine / R.Gonzalez | 21 07 74 | galaxy chain | |||
2668 | 2568 | 22 35 00 | -61 32 | 120m | llla - J | 2" | Racine / R.Gonzalez | 21 07 74 | interacting galaxies | |||
2669 | 2569 | 18 35 00 | -30 00 | 10s each | lla - O | V.Blanco / Saá / Czuia | 30 07 74 | focus plate |
Last Updated on 8/27/99
By Guerra & Marin
October 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2670 | 2570 | 18 01 12 | -24 24 | 20m | llla - J | GG 13 | 2" | Dufour / Ríos | 10 10 74 | M 8 | ||
2671 | 2571 | 00 46 20 | -73 24 | 30m | 127 - 02 | RG 2 | 2" | Dufour / Ríos | 10 10 74 | SMC N 19 | ||
2672 | 2572 | 00 46 20 | -73 24 | 60m | 127 - 02 | RG 2 | 3" | Dufour / Ríos | 10 10 74 | SMC N 19 | ||
2673 | 2573 | 00 46 20 | -73 24 | 30m | llla - J | GG 13 | 2.5" | Dufour / Ríos | 10 10 74 | SMC N 19 | ||
2674 | 2574 | 00 46 20 | -73 24 | 45m | llla - J | UG 2 | 2" | Dufour / Ríos | 10 10 74 | SMC N 19 | ||
2675 | 2575 | 00 58 27 | -72 18 | 30m | llla - J | UG 2 | 2" | Dufour / Ríos | 10 10 74 | SMC N 66A | ||
2676 | 2576 | 00 58 27 | -72 18 | 20m | llla - J | GG 385 | 2" | Dufour / Ríos | 10 10 74 | SMC N 66A | ||
2677 | 2577 | 00 58 27 | -72 18 | 15m | 127 - 02 | RG 2 | 2" | Dufour / Ríos | 10 10 74 | SMC N 66A | ||
2678 | 2578 | 05 40 00 | -69 45 | 30m | llla - J | UG 2 | 2" | Dufour / Ríos | 10 10 74 | LMC X - 1 | ||
2679 | 2579 | 05 38 40 | -64 06 | 180m | llla - J | UG 2 | 2" | Dufour / Ríos | 10 10 74 | LMC X - 3 | ||
2680 | 2580 | 05 38 40 | -64 06 | 60m | llla - J | UG 2 | 2" | Dufour / Ríos | 10 10 74 | LMC X - 3 | ||
2681 | 2581 | 00 58 30 | -33 50 | 180m | 103a - D | 2" - 5" | Demers / R.Gonzalez | 14 10 74 | Sculptor galaxy | |||
2682 | 2582 | 04 34 24 | -58 59 | 180m | 103a - O | 3" | Demers / R.Gonzalez | 14 10 74 | Reticulum galaxy | |||
2683 | 2583 | 04 34 24 | -58 59 | 75m | 103a - D | 5" | Demers / R.Gonzalez | 14 10 74 | Reticulum galaxy | |||
2684 | 2584 | 00 58 30 | -33 50 | 180m | 103a - D | 3" | Demers / Kunkel / R.Gonzalez | 15 10 74 | Sculptor galaxy | |||
2685 | 2585 | 04 34 24 | -58 59 | 62m | 103a - O | 3" | Demers / Kunkel / R.Gonzalez | 15 10 74 | Reticulum galaxy | |||
2686 | 2586 | 04 34 24 | -58 59 | 40m | 103a - D | Demers / Kunkel / R.Gonzalez | 15 10 74 | Reticulum galaxy | ||||
2687 | 2587 | 04 34 24 | -58 59 | 40m | 103a - O | Demers / Kunkel / R.Gonzalez | 15 10 74 | Reticulum galaxy |
Last Updated on 8/27/99
By Guerra & Marin
December 1974 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2688 | 2588 | 04 58 48 | -66 02 | 40m | 103a - O | 1.5" | Graham / Poblete / Rojas | 17 12 74 | NGC 1783 | |||
2689 | 2589 | 04 58 48 | -66 02 | 40m | 103a - O | 1.5" | Graham / Poblete / Rojas | 17 12 74 | NGC 1783 | |||
2690 | 2590 | 04 58 48 | -66 02 | 40m | 103a - O | 1.5" | Graham / Poblete / Rojas | 17 12 74 | NGC 1783 | |||
2691 | 2591 | 04 58 48 | -66 02 | 40m | 103a - O | 1" | Graham / Poblete / Rojas | 17 12 74 | NGC 1783 | |||
2692 | 2592 | 04 58 48 | -66 02 | 40m | 103a - O | 1" | Graham / Poblete / Rojas | 17 12 74 | NGC 1783 | |||
2693 | 2593 | 04 58 48 | -66 02 | 40m | 103a - O | 1" - 1.5" | Graham / Poblete / Rojas | 17 12 74 | NGC 1783 | |||
2694 | 2594 | 04 58 48 | -66 02 | 40m | 103a - O | GG 385 | 1" | Graham / Poblete / Rojas | 17 12 74 | NGC 1783 | ||
2695 | 2595 | 04 58 48 | -66 02 | 40m | 103a - O | GG 385 | > 1" | Graham / Poblete / Rojas | 18 12 74 | NGC 1783 | ||
2696 | 2596 | 04 58 48 | -66 02 | 40m | 103a - O | GG 385 | > 1" | Graham / Poblete / Rojas | 18 12 74 | NGC 1783 | ||
2697 | 2597 | 04 58 48 | -66 02 | 40m | 103a - O | GG 385 | < 1" | Graham / Poblete / Rojas | 18 12 74 | NGC 1783 | ||
2698 | 2598 | 04 58 48 | -66 02 | 60m | 103a - D | GG 495 | > 1" | Graham / Poblete / Rojas | 18 12 74 | NGC 1783 | ||
2699 | 2599 | 04 58 48 | -66 02 | 40m | 103a - O | GG 385 | > 1.5" | Graham / Poblete / Rojas | 18 12 74 | NGC 1783 | ||
2700 | 2600 | 04 58 48 | -66 02 | 40m | 103a - O | GG 385 | 1.5" | Graham / Poblete / Rojas | 18 12 74 | NGC 1783 | ||
2701 | 2601 | 04 58 48 | -66 02 | 40m | 103a - O | GG 385 | 1.5" | Graham / Poblete / Rojas | 18 12 74 | NGC 1783 | ||
2702 | 2602 | cenit | -30 00 | 12s each | 103a - D | GG 385 | 5" | Cosgrove | 27 12 74 | focus plate | ||
2703 | 2603 | 08 36 12 | -30 00 | 12s each | 103a - D | 5" | Cosgrove | 27 12 74 | focus plate | |||
2704 | 2604 | 01 26 36 | -30 00 | 12s each | 103a - D | 5" | Cosgrove | 27 12 74 | focus plate | |||
2705 | 2605 | 05 42 30 | +20 00 | 12s each | 103a - D | 5" | Cosgrove | 27 12 74 | focus plate | |||
2706 | 2606 | 06 12 42 | -75 00 | 12s each | 103a - D | 5" | Cosgrove | 27 12 74 | focus plate | |||
2707 | 2607 | 09 35 12 | -30 00 | 12s each | lla - O | 3" | Cosgrove | 27 12 74 | focus plate | |||
2708 | 2608 | 10 57 36 | -75 00 | 12s each | lla - O | 3" | Cosgrove | 27 12 74 | focus plate | |||
2709 | 2609 | 04 02 48 | -30 00 | 12s each | 103a - O | 2" | Cosgrove | 28 12 74 | focus plate | |||
2710 | 2610 | 08 17 00 | -30 00 | 12s each | 103a - O | 2" | Cosgrove | 28 12 74 | focus plate | |||
2711 | 2611 | 01 25 00 | -30 00 | 12s each | 103a - O | 2" | Cosgrove | 28 12 74 | focus plate | |||
2712 | 2612 | 06 01 12 | -75 00 | 12s each | 103a - O | 2" | Cosgrove | 28 12 74 | focus plate | |||
2713 | 2613 | 07 06 06 | +20 00 | 12s each | 103a - O | 2" | Cosgrove | 28 12 74 | focus plate |
Last Updated on 8/27/99
By Jorge Marin
1975 Plate logs for 1.5-m telescope
January 1975 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2714 | 2614 | 05 37 36 | -70 12 | 20m | 103a - D | GG 14 | 2" | Flower / Pinto | 21 01 75 | focus plate | ||
2715 | 2615 | 05 37 36 | -70 12 | 20m | 103a - O | GG 13 | 3" | Flower / Pinto | 21 01 75 | focus plate | ||
2716 | 2616 | 05 37 36 | -70 12 | 60m | 103a - D | GG 14 | 3" | Flower / Pinto | 21 01 75 | focus plate | ||
2717 | 2617 | 05 37 36 | -70 12 | 60m | 103a - O | 3" | Flower / Pinto | 21 01 75 | focus plate | |||
2718 | 2618 | 05 37 36 | -70 12 | 90m | 103a - D | 3" | Flower / Pinto | 21 01 75 | focus plate | |||
2719 | 2619 | 05 37 36 | -70 12 | 20m | 103a - O | 3" | Flower / Pinto | 21 01 75 | focus plate | |||
2720 | 2620 | 05 37 36 | -70 12 | 20m | 103a - D | 3" | Flower / Pinto | 21 01 75 | focus plate |
Last Updated on 8/27/99
By Guerra & Marin
February 1975 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2721 | 2621 | 05 13 12 | -40 03 | 10m | 103a - O | GG 385 | 5" | Mrs.Liller / Ríos | 03 02 75 | NGC 1851 | ||
2722 | 2622 | 06 15 42 | +09 08 | 20m | 103a - O | GG 385 | 4" - 5" | Mrs.Liller / Ríos | 03 02 75 | 0614 + 09 | ||
2723 | 2623 | 09 11 24 | -64 45 | 10m | 103a - O | GG 385 | 5" - 6" | Mrs.Liller / Ríos | 03 02 75 | 2808 | ||
2724 | 2624 | 06 48 06 | -35 59 | 10m | 103a - O | GG 385 | 5" - 6" | Mrs.Liller / Ríos | 03 02 75 | NGC 2298 | ||
2725 | 2625 | 09 11 24 | -64 45 | 10m | 103a - O | GG 385 | 5" - 6" | Mrs.Liller / Ríos | 03 02 75 | 2808 | ||
2726 | 2626 | 15 18 43 | -57 04 | 60m | 098 - 04 | RG 1 | 4" - 5" | Mrs.Liller / Ríos | 03 02 75 | Cir X - 1 | ||
2727 | 2627 | 15 37 33 | -52 15 | 30m | 098 - 04 | RG 1 | 4" - 5" | Mrs.Liller / Ríos | 03 02 75 | Nova Normae | ||
2728 | 2628 | 05 13 12 | -40 03 | 10m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Ríos | 04 02 75 | NGC 1851 | ||
2729 | 2629 | 06 48 06 | -35 59 | 10m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Ríos | 04 02 75 | NGC 2298 | ||
2730 | 2630 | 09 11 24 | -64 45 | 10m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Ríos | 04 02 75 | NGC 2808 | ||
2731 | 2631 | 06 15 42 | +09 08 | 30m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Ríos | 04 02 75 | 0614 + 09 | ||
2732 | 2632 | 05 38 06 | -44 06 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Ríos | 04 02 75 | 537 - 44 | ||
2733 | 2633 | 12 24 30 | -72 32 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Ríos | 04 02 75 | NGC 4372 | ||
2734 | 2634 | 05 13 12 | -40 03 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Ríos | 04 02 75 | NGC 1851 | ||
2735 | 2635 | 06 48 06 | -35 59 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Ríos | 04 02 75 | NGC 2298 | ||
2736 | 2636 | 08 30 30 | +04 35 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Ríos | 04 02 75 | MA 0829 + 04 | ||
2737 | 2637 | 09 11 24 | -64 45 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Ríos | 04 02 75 | NGC 2808 | ||
2738 | 2638 | 12 24 30 | -72 32 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Ríos | 04 02 75 | NGC 4372 | ||
2739 | 2639 | 13 23 54 | -42 53 | 30m | 098 - 04 | RG 1 | 2" | Mrs.Liller / Ríos | 04 02 75 | Cent A | ||
2740 | 2640 | 15 18 43 | -57 04 | 60m | 098 - 04 | RG 1 | 2" | Mrs.Liller / Ríos | 04 02 75 | Cir X - 1 | ||
2741 | 2641 | 05 09 00 | -69 00 | 40m | 103a - D | GG 14 | 3" | Ríos | 08 02 75 | -69º 5:09 | ||
2742 | 2642 | 05 09 00 | -69 00 | 40m | 103a - D | GG 14 | 3" | Ríos | 08 02 75 | -69º 5:09 | ||
2743 | 2643 | 05 09 00 | -69 00 | 40m | 1 N | RG 8 | 3" - 5" | Ríos | 08 02 75 | -69º 5:09 | ||
2744 | 2644 | cenit | -30 00 | 10s each | 103a - D | 3" | Ríos | 08 02 75 | focus plate | |||
2745 | 2645 | 07 50 44 | -40 00 | 10s each | 103a - D | 3" | Ríos | 08 02 75 | focus plate | |||
2746 | 2646 | 16 22 57 | -40 00 | 10s each | 103a - D | 3" | Ríos | 08 02 75 | focus plate | |||
2747 | 2647 | 12 55 50 | -70 00 | 10s each | 103a - D | 3" | Ríos | 08 02 75 | focus plate | |||
2748 | 2648 | 03 11 42 | -55 23 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Pinto | 17 02 75 | NGC 1261 | ||
2749 | 2649 | 09 11 24 | -64 45 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Pinto | 17 02 75 | NGC 2808 | ||
2750 | 2650 | 06 15 42 | +09 08 | 30m | 103a - O | GG 385 | 2" | Mrs.Liller / Pinto | 17 02 75 | 3U 0614 | ||
2751 | 2651 | 05 13 12 | -40 03 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Pinto | 17 02 75 | NGC 1851 | ||
2752 | 2652 | 06 48 06 | -35 59 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Pinto | 17 02 75 | NGC 2298 | ||
2753 | 2653 | 09 11 24 | -64 45 | 10m | 103a - O | GG 385 | 2" | Mrs.Liller / Pinto | 17 02 75 | NGC 2808 | ||
2754 | 2654 | 12 24 30 | -72 32 | 10m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Pinto | 17 02 75 | NGC 4372 | ||
2755 | 2655 | 05 13 12 | -40 03 | 10m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Pinto | 17 02 75 | NGC 1851 | ||
2756 | 2656 | 06 48 06 | -35 59 | 10m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Pinto | 17 02 75 | NGC 2298 | ||
2757 | 2657 | 13 23 54 | -42 53 | 30m | 098 - 04 | RG 1 | 2" - 3" | Mrs.Liller / Pinto | 17 02 75 | Cent A | ||
2758 | 2658 | 14 28 18 | -55 12 | 15m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Pinto | 17 02 75 | NGC 5634 | ||
2759 | 2659 | 15 18 42 | -57 04 | 60m | 098 - 04 | RG 1 | 2" - 3" | Mrs.Liller / Pinto | 17 02 75 | Cir X - 1 | ||
2760 | 2660 | 14 28 18 | -55 02 | 15m | 103a - O | GG 385 | 2" - 3" | Mrs.Liller / Pinto | 17 02 75 | NGC 5634 | ||
2761 | 2661 | 03 11 42 | -55 23 | 10m | 103a - D | GG 14 | Mrs.Liller / Pinto | 18 02 75 | NGC 1261 | |||
2762 | 2662 | 03 11 42 | -55 23 | 10m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 1261 | |||
2763 | 2663 | 06 48 06 | -35 59 | 10m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 2298 | |||
2764 | 2664 | 09 11 24 | -64 45 | 10m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 2808 | |||
2765 | 2665 | 06 15 42 | +09 08 | 30m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | 3U 0614 | |||
2766 | 2666 | 05 13 12 | -40 03 | 10m | 103a - D | GG 14 | Mrs.Liller / Pinto | 18 02 75 | NGC 1851 | |||
2767 | 2667 | 05 13 12 | -40 03 | 10m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 1851 | |||
2768 | 2668 | 06 48 06 | -35 59 | 10m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 2298 | |||
2769 | 2669 | 09 11 24 | -64 45 | 10m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 2808 | |||
2770 | 2670 | 12 24 30 | -72 32 | 10m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 4372 | |||
2771 | 2671 | 14 28 18 | -05 52 | 15m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 5634 | |||
2772 | 2672 | 15 18 42 | -57 04 | 60m | 098 - 4 | RG 1 | Mrs.Liller / Pinto | 18 02 75 | Cir X - 1 | |||
2773 | 2673 | 15 45 36 | -47 47 | 25m | 098 - 4 | RG 1 | Mrs.Liller / Pinto | 18 02 75 | 3U 1543 | |||
2774 | 2674 | 14 28 18 | -05 52 | 15m | 103a - O | GG 385 | Mrs.Liller / Pinto | 18 02 75 | NGC 5634 |
Last Updated on 8/27/99
By Guerra & Marin
April 1975 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2775 | 2675 | 10 44 00 | -59 32 | 20m | lla - O | 1.5" | J.Hesser / Pinto | 20 04 75 | eta Carina | |||
2776 | 2676 | 10 44 00 | -59 32 | 10m | lla - O | 1.5" | J.Hesser / Pinto | 20 04 75 | eta Carina | |||
2777 | 2677 | 13 25 24 | -47 32 | 5m | lla - O | 1.5" | J.Hesser / Pinto | 20 04 75 | omega Centauri | |||
2778 | 2678 | 13 25 24 | -47 32 | 10m | lla - O | 1.5" | J.Hesser / Pinto | 20 04 75 | omega Centauri | |||
2779 | 2679 | 13 25 24 | -47 32 | 20m | lla - O | 1.5" | J.Hesser / Pinto | 20 04 75 | omega Centauri | |||
2780 | 2680 | 13 25 24 | -47 32 | 20m | llla - J baked | 1.5" | J.Hesser / Pinto | 20 04 75 | omega Centauri | |||
2781 | 2681 | 17 13 18 | -29 38 | 20m | llla - J baked | 1.5" | J.Hesser / Pinto | 20 04 75 | NGC 6304 | |||
2782 | 2682 | 17 13 18 | -29 38 | 30m | llla - J baked | 1.5" | J.Hesser / Pinto | 20 04 75 | NGC 6304 | |||
2783 | 2683 | 17 23 48 | -48 25 | 15m | llla - J baked | 1.5" | J.Hesser / Pinto | 20 04 75 | NGC 6352 | |||
2784 | 2684 | 17 23 48 | -48 25 | 30m | llla - J baked | 2" | J.Hesser / Pinto | 20 04 75 | NGC 6352 | |||
2785 | 2685 | 17 48 48 | -37 05 | 15m | llla - J baked | 2" | J.Hesser / Pinto | 20 04 75 | NGC 6441 | |||
2786 | 2686 | 17 48 48 | -37 05 | 30m | llla - J baked | 2" | J.Hesser / Pinto | 20 04 75 | NGC 6441 | |||
2787 | 2687 | 18 02 00 | -30 04 | 30m | llla - J baked | 2" | J.Hesser / Pinto | 20 04 75 | NGC 6522 | |||
2788 | 2688 | 18 02 00 | -30 04 | 15m | llla - J baked | 2" | J.Hesser / Pinto | 20 04 75 | NGC 6522 | |||
2789 | 2689 | 18 02 00 | -30 04 | 7.5m | llla - J baked | 2" | J.Hesser / Pinto | 20 04 75 | NGC 6522 |
Last Updated on 8/27/99
By Jorge Marin
June 1975 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2790 | 2690 | 22 28 00 | -20 57 | 180m | 098 - 02 | RG 610 | 2" | V.Blanco / Czuia | 30 06 75 | NGC 7293 | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
October 1975 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2791 | 2691 | 19 43 54 | -08 05 | 120m | 103a - D | GG 14 | 2" | R.W.C / R.Gonzalez | 06 10 75 | Pal 11 | ||
2792 | 2692 | 21 45 00 | -21 21 | 120m | 103a - D | R.W.C / R.Gonzalez | 06 10 75 | Pal 12 | ||||
2793 | 2693 | 21 45 00 | -21 21 | 60m | 103a - O | GG 13 | R.W.C / R.Gonzalez | 06 10 75 | Pal 12 | |||
2794 | 2694 | 00 52 00 | -26 44 | 60m | 103a - O | R.W.C / R.Gonzalez | 06 10 75 | NGC 298 | ||||
2795 | 2695 | 05 23 00 | -24 32 | 75m | 103a - D | GG 14 | R.W.C / R.Gonzalez | 06 10 75 | NGC 1904 | |||
2796 | 2696 | 19 43 54 | -08 05 | 80m | 103a - O | GG 385 | R.W.C / R.Gonzalez | 07 10 75 | Pal 11 | |||
2797 | 2697 | 19 43 54 | -08 05 | 35m | 103a - D | GG 14 | R.W.C / R.Gonzalez | 07 10 75 | Pal 11 | |||
2798 | 2698 | 21 45 00 | -21 21 | 60m | 103a - D | GG 14 | R.W.C / R.Gonzalez | 07 10 75 | Pal 12 | |||
2799 | 2699 | 21 45 00 | -21 21 | 60m | 103a - O | GG 385 | R.W.C / R.Gonzalez | 07 10 75 | Pal 12 | |||
2800 | 2700 | 05 23 00 | -24 32 | 60m | 103a - O | GG 385 | R.W.C / R.Gonzalez | 07 10 75 | NGC 1904 | |||
2801 | 2701 | 05 23 00 | -24 32 | 70m | 103a - D | GG 14 | R.W.C / R.Gonzalez | 07 10 75 | NGC 1904 |
Last Updated on 8/27/99
By Guerra & Marin
December 1975 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2802 | 2702 | 00 51 24 | -26 44 | 30m | 103a - D | GG 14 | McClure / Pinto | 13 12 75 | NGC 288 | |||
2803 | 2703 | 00 51 24 | -26 44 | 34m | 103a - D | GG 14 | McClure / Pinto | 13 12 75 | NGC 288 | |||
2804 | 2704 | 00 51 24 | -26 44 | 40m | 103a - D | GG 14 | McClure / Pinto | 13 12 75 | NGC 288 | |||
2805 | 2705 | 00 51 24 | -26 44 | 40m | 103a - D | GG 14 | McClure / Pinto | 13 12 75 | NGC 288 | |||
2806 | 2706 | 07 58 42 | -10 43 | 45m | 103a - D | GG 14 | McClure / Pinto | 13 12 75 | NGC 2506 | |||
2807 | 2707 | 07 58 42 | -10 43 | 45m | 103a - D | GG 14 | McClure / Pinto | 13 12 75 | NGC 2506 | |||
2808 | 2708 | 07 58 42 | -10 43 | 45m | 103a - D | GG 14 | McClure / Pinto | 13 12 75 | NGC 2506 | |||
2809 | 2709 | 07 58 42 | -10 43 | 76m | llla - J | GG 385 | McClure / Pinto | 13 12 75 | NGC 2506 |
Last Updated on 8/27/99
By Guerra & Marin
1976 Plate logs for 1.5-m telescope
July 1976 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2810 | 2710 | 18 03 50 | -29 30 | 10s each | 103a - D | O.Saá | 13 07 76 | focus Nº1 | ||||
2811 | 2711 | 20 05 30 | -35 40 | 10s each | 103a - D | O.Saá | 13 07 76 | focus Nº2 | ||||
2812 | 2712 | 19 48 00 | +08 46 | 5m | 103a - D | O.Saá | 13 07 76 | alpha Aql | ||||
2813 | 2713 | 22 56 00 | -29 45 | 5m | 103a - D | O.Saá | 13 07 76 | alpha PsA | ||||
2814 | 2714 | 22 56 00 | -29 45 | 10m | 103a - D | O.Saá | 14 07 76 | alpha PsA |
Last Updated on 8/27/99
By Guerra & Marin
August 1976 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2815 | 2715 | 18 56 42 | -08 44 | 2m | llla - J | 1.5" | Carney / Czuia | 20 08 76 | NGC 6712 | |||
2816 | 2716 | 18 56 42 | -08 44 | 10m | llla - J | 1.5" | Carney / Czuia | 20 08 76 | NGC 6712 | |||
2817 | 2717 | 18 56 42 | -08 44 | 0.3m | llla - J | 1.5" | Carney / Czuia | 20 08 76 | NGC 6712 | |||
2818 | 2718 | 19 08 00 | -60 02 | 30m | 103a - O | GG 385 | 3" | Carney / Czuia | 21 08 76 | NGC 6752 | ||
2819 | 2719 | 19 08 00 | -60 02 | 35m | 103a - D | GG 14 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 6752 | ||
2820 | 2720 | 00 55 24 | -72 37 | 30m | 103a - D | GG 14 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2821 | 2721 | 00 55 24 | -72 37 | 30m | 103a - D | GG 14 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2822 | 2722 | 00 55 24 | -72 37 | 40m | 103a - O | UG 2 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2823 | 2723 | 00 55 24 | -72 37 | 6m | 103a - O | UG 2 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2824 | 2724 | 00 55 24 | -72 37 | 10m | 103a - O | UG 2 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2825 | 2725 | 00 55 24 | -72 37 | 15m | 103a - O | GG 385 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2826 | 2726 | 00 55 24 | -72 37 | 10m | 103a - O | GG 385 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2827 | 2727 | 00 55 24 | -72 37 | 5m | 103a - O | GG 385 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2828 | 2728 | 00 55 24 | -72 37 | 5m | 103a - O | GG 385 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2829 | 2729 | 00 55 24 | -72 37 | 5m | 103a - D | GG 14 | 3" - 4" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2830 | 2730 | 00 55 24 | -72 37 | 5m | 103a - D | GG 14 | 3" | Carney / Czuia | 21 08 76 | NGC 330 | ||
2831 | 2731 | 00 23 06 | -72 11 | 10m | 103a - D | GG 14 | Carney / Czuia | 21 08 76 | NGC 104 (47 Tuc) |
Last Updated on 8/27/99
By Jorge Marin
September 1976 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2832 | 2732 | 00 51 12 | -26 46 | 15m | 103a - D | GG 14 | 3" - 4" | Canterna | 02 09 76 | NGC 288 | ||
2833 | 2733 | 00 51 12 | -26 46 | 90m | 103a - D | GG 14 | 3" - 4" | Canterna | 02 09 76 | NGC 288 |
Last Updated on 8/27/99
By Guerra & Marin
1977 Plate logs for 1.5-m telescope
June 1977 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2834 | 2734 | 15:05:00 | -30:00 | 10s each | 103a - D | GG 495 | 1.5" | V.Blanco / Czuia | 07 06 77 | Focus plate | Broken Ok" | CTIO |
2835 | 2735 | 15 05 00 | -30 00 | 10s each | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 07 06 77 | Focus plate | Broken Ok" | CTIO |
2836 | 2736 | 18 02 18 | -30 01 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | Broken Ok" | CTIO |
2837 | 2737 | 18 02 18 | -30 01 | 30m | 103a - D | GG 495 | 2" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | Broken Ok" | CTIO |
2838 | 2738 | 18 02 18 | -30 01 53 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | ||
2839 | 2739 | 18 02 18 | -30 01 53 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | CTIO | |
2840 | 2740 | 18 02 18 | -30 01 53 | 15m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | CTIO | |
2841 | 2741 | 18 02 18 | -30 01 53 | 20m | 103a - D | GG 495 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | Broken Ok" | CTIO |
2842 | 2742 | 18 02 18 | -30 01 53 | 15m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | CTIO | |
2843 | 2743 | 18 02 18 | -30 01 53 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | CTIO | |
2844 | 2744 | 18 02 18 | -30 01 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | Broken Ok" | CTIO |
2845 | 2745 | 18 02 18 | -30 01 | 30m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 07 06 77 | NGC 6522 | CTIO | |
2846 | 2746 | 18 02 18 | -30 01 | 30m | IN | RG 695 | 1.5" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2847 | 2747 | 18 02 22 | -30 01 33 | 20m | 103a - O | GG 385 | 1.3" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2848 | 2748 | 18 02 22 | -30 01 33 | 30m | 103a - D | GG 495 | 1.3" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2849 | 2749 | 18 02 22 | -30 01 33 | 20m | 098 - O4 | RG 610 | 1.3" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2850 | 2750 | 18 02 22 | -30 01 33 | 20m | 103a - O | GG 385 | 1.3" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2851 | 2751 | 18 02 22 | -30 01 33 | 30m | 103a - D | GG 495 | 1.3" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2852 | 2752 | 18 02 22 | -30 01 33 | 20m | 103a - O | GG 385 | 1" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | Broken Ok" ??? | CTIO |
2853 | 2753 | 18 02 22 | -30 01 33 | 30m | 103a - D | GG 495 | 1" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | Broken Ok" | CTIO |
2854 | 2754 | 18 02 22 | -30 01 33 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2855 | 2755 | 18 02 22 | -30 01 33 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2856 | 2756 | 18 02 22 | -30 01 33 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2857 | 2757 | 18 02 22 | -30 01 33 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2858 | 2758 | 18 02 22 | -30 01 33 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2859 | 2759 | 18 02 22 | -30 01 33 | 30m | 103a - D | GG 495 | 2" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2860 | 2760 | 18 02 22 | -30 01 33 | 20m | 103a - O | GG 385 | 2" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2861 | 2761 | 18 02 22 | -30 01 33 | 20m | 103a - D | GG 495 | 2.5" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO | |
2862 | 2762 | 18 02 22 | -30 01 33 | 20m | 103a - O | GG 385 | 2" | V.Blanco / Czuia | 08 06 77 | NGC 6522 | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
July 1977 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2863 | 2763 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2864 | 2764 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2865 | 2765 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2866 | 2766 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 2" - 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2867 | 2767 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2868 | 2768 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 2" - 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2869 | 2769 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2870 | 2770 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 2" - 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2871 | 2771 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2872 | 2772 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 2" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2873 | 2773 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2874 | 2774 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" - 2" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2875 | 2775 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2876 | 2776 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2877 | 2777 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 3" | Blanco / Zemelman | 09 07 77 | NGC 6522 | CTIO | |
2878 | 2778 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Zemelman / M.N | 10 07 77 | NGC 6522 | CTIO | |
2879 | 2779 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" | Blanco / Zemelman / M.N | 10 07 77 | NGC 6522 | CTIO | |
2880 | 2780 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 2" - 3" | Blanco / Zemelman / M.N | 10 07 77 | NGC 6522 | Broken Ok" | CTIO |
2881 | 2781 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 2" - 3" | Blanco / Zemelman / M.N | 10 07 77 | NGC 6522 | Broken Ok" | CTIO |
2882 | 2782 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 16 07 77 | NGC 6522 | Broken Ok" | CTIO |
2883 | 2783 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 16 07 77 | NGC 6522 | Broken Ok" | CTIO |
2884 | 2784 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | Broken Ok" | CTIO |
2885 | 2785 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2886 | 2786 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2887 | 2787 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2888 | 2788 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2889 | 2789 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2890 | 2790 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 2.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2891 | 2791 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 2.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2892 | 2792 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 1.5" - 3" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2893 | 2793 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" - 3" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2894 | 2794 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 1.5" - 3" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | Broken Ok" | CTIO |
2895 | 2795 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 2" - 4" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | Broken Ok" | CTIO |
2896 | 2796 | 18 02 00 | -30 14 | 20m | 103a - O | GG 495 | 2" - 6" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2897 | 2797 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | Broken Ok" | CTIO |
2898 | 2798 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 17 07 77 | NGC 6522 | CTIO | |
2899 | 2799 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | Broken Ok" | CTIO |
2900 | 2800 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | Broken Ok" | CTIO |
2901 | 2801 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2902 | 2802 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2903 | 2803 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2904 | 2804 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2905 | 2805 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2906 | 2806 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2907 | 2807 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | Broken Ok" | CTIO |
2908 | 2808 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2909 | 2809 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 1.5" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2910 | 2810 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 1.5" - 3" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2911 | 2811 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 2" - 3" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | Broken Ok" | CTIO |
2912 | 2812 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 1" - 2" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2913 | 2813 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 2" | V.Blanco / R.Gonzalez | 18 07 77 | NGC 6522 | CTIO | |
2914 | 2814 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 3" | V.Blanco / R.Gonzalez | 19 07 77 | NGC 6522 | CTIO | |
2915 | 2815 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 3" | V.Blanco / R.Gonzalez | 19 07 77 | NGC 6522 | CTIO | |
2916 | 2816 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 3" - 4" | V.Blanco / R.Gonzalez | 19 07 77 | NGC 6522 | CTIO | |
2917 | 2817 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 3" - 4" | V.Blanco / R.Gonzalez | 19 07 77 | NGC 6522 | CTIO | |
2918 | 2818 | 18 02 00 | -30 14 | 20m | 103a - O | GG 385 | 3" - 4" | V.Blanco / R.Gonzalez | 19 07 77 | NGC 6522 | CTIO | |
2919 | 2819 | 18 02 00 | -30 14 | 30m | 103a - D | GG 495 | 5" | V.Blanco / R.Gonzalez | 19 07 77 | NGC 6522 | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
1978 Plate logs for 1.5-m telescope
March 1978 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2920 | 2820 | 05 32 44 | -66 23 03 | 30m | llla - J baked | 2" | D.Crampton / A.Cowley / D.Maturana | 10 03 78 | LMC X - 1 | |||
2921 | 2821 | 09 19 40 | -55 05 39 | 90m | llla - J baked | 2" | D.Crampton / A.Cowley / D.Maturana | 10 03 78 | 250918 - 549 | |||
2922 | 2822 | 09 24 20 | -31 35 06 | 90m | llla - J baked | 2" | D.Crampton / A.Cowley / D.Maturana | 10 03 78 | 400923 - 31 | |||
2923 | 2823 | 12 40 31 | -60 03 30 | 105m | llla - J baked | 2" | D.Crampton / A.Cowley / D.Maturana | 10 03 78 | 251239 - 599 | |||
2924 | 2824 | 15 40 28 | -52 18 10 | 72m | llla - J baked | 2" | D.Crampton / A.Cowley / D.Maturana | 10 03 78 | 251538 - 522 | |||
2925 | 2825 | 05 39 52 | -69 46 52 | 30m | llla - J baked | 2" | D.Crampton / A.Cowley / D.Maturana | 11 03 78 | LMC X - 1 | |||
2926 | 2826 | 05 20 45.2 | -71 59 46 | 60m | llla - J baked | 2" | D.Crampton / A.Cowley / D.Maturana | 11 03 78 | LMC X - 2 | |||
2927 | 2827 | 09 19 40 | -55 05 39 | 120m | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 11 03 78 | 250918 - 549 | |||
2928 | 2828 | 11 23 54 | -59 11 40 | 90m | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 11 03 78 | #1122 - 59 | |||
2929 | 2829 | 14 09 05 | -62 02 06 | 90m | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 11 03 78 | MX 1406 - 61 | |||
2930 | 2830 | 16 34 13.4 | -64 27 59 | 90m | llla - J baked | 3" - 4" | D.Crampton / A.Cowley / D.Maturana | 11 03 78 | 2A 1631 - 644 | |||
2931 | 2831 | 05 39 04.9 | -64 06 58 | 90m | llla - J baked | 3" - 4" | D.Crampton / A.Cowley / D.Maturana | 12 03 78 | LMC X - 3 | |||
2932 | 2832 | 08 37 02 | -42 42 00 | 90m | llla - J baked | 3" - 4" | D.Crampton / A.Cowley / D.Maturana | 12 03 78 | 4U 0836 - 42 | |||
2933 | 2833 | 12 55 55 | -69 09 05 | 90m | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 12 03 78 | 251254 - 690 | |||
2934 | 2834 | 13 29 13 | -08 29 32 | 5m | llla - J baked | 4" | D.Crampton / A.Cowley / D.Maturana | 12 03 78 | W 485 | |||
2935 | 2835 | 15 45 46 | -62 29 02 | 90m | llla - J baked | 4" | D.Crampton / A.Cowley / D.Maturana | 12 03 78 | 251553 - 624 | |||
2936 | 2836 | 15 55 48 | -54 20 20 | 120m | llla - J baked | D.Crampton / A.Cowley / D.Maturana | 12 03 78 | 251553 - 542 | ||||
2937 | 2837 | 09 36 14 | -37 14 50 | 15m | llla - J baked | 4" - 5" | D.Crampton / A.Cowley / D.Maturana | 13 03 78 | LDS 275 AB | |||
2938 | 2838 | 08 37 02 | -42 42 00 | 90m | llla - J baked | 4" - 5" | D.Crampton / A.Cowley / D.Maturana | 13 03 78 | 4 U 0836 - 42 | |||
2939 | 2839 | 10 37 10 | -56 41 00 | 90m | llla - J baked | 4" - 5" | D.Crampton / A.Cowley / D.Maturana | 13 03 78 | 4 U 1036 - 56 | |||
2940 | 2840 | 12 55 55 | -69 09 05 | 120m | llla - J baked | 4" | D.Crampton / A.Cowley / D.Maturana | 13 03 78 | 251254 - 690 | |||
2941 | 2841 | 15 58 55 | -60 39 55 | 90m | llla - J baked | 4" | D.Crampton / A.Cowley / D.Maturana | 13 03 78 | 251556 - 605 | |||
2942 | 2842 | 16 26 29 | -49 08 53 | 100m | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 13 03 78 | 251624 - 490 | |||
2843 | 17 02 23 | -37 49 16 | 90s / 30s | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 13 03 78 | 3 U 1700 - 37 | ||||
2844 | 09 24 20 | -31 35 06 | 90m | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 14 03 78 | 4 U 0923 - 31 | ||||
2845 | 11 38 44 | -65 15 47 | 90m | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 14 03 78 | 4 U 1137 - 65 | ||||
2846 | 12 10 22 | -64 38 24 | 90m | llla - J baked | 3" | D.Crampton / A.Cowley / D.Maturana | 14 03 78 | 4 U 1210 - 64 | ||||
2847 | 15 58 55 | -60 39 54 | 90m | llla - J baked | 3" - 4" | D.Crampton / A.Cowley / D.Maturana | 14 03 78 | 251556 - 605 | ||||
2848 | 16 26 30 | -49 08 40 | 75m | llla - J baked | D.Crampton / A.Cowley / D.Maturana | 14 03 78 | 251624 - 490 | |||||
2849 | 17 04 18.9 | -36 23 35 | 70m | llla - J baked | D.Crampton / A.Cowley / D.Maturana | 14 03 78 | 251702 - 363 | |||||
2850 | 17 51 32.3 | -34 48 04 | 5m | llla - J baked | D.Crampton / A.Cowley / D.Maturana | 14 03 78 | NGC 6475 | |||||
2851 | 17 51 32.3 | -34 48 04 | 0.5m | llla - J baked | D.Crampton / A.Cowley / D.Maturana | 14 03 78 | NGC 6475 |
Last Updated on 8/27/99
By Guerra & Marin
May 1978 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2852 | 10 44 43 | -64 12 52 | 40m | 103a - D | GG 14 | 4" - 10" | A.Twarog / Poblete | 07 05 78 | theta Car cluster, IC 2602 | |||
2853 | 10 44 43 | -64 12 52 | 45m | 103a - O | GG 385 | A.Twarog / Poblete | 07 05 78 | theta Car cluster, IC 2602 | ||||
2854 | 10 44 43 | -64 12 52 | 45m | 103a - O | GG 385 | A.Twarog / Poblete | 07 05 78 | theta Car cluster, IC 2602 | ||||
2855 | 17 38 39 | -32 11 55 | 120m | 103a - O | UG 2 | 2" -3" | A.Twarog / Poblete | 07 05 78 | NGC 6405 | |||
2856 | 17 52 21 | -34 46 30 | 120m | 103a - O | UG 2 | 1.5" | A.Twarog / Poblete | 07 05 78 | NGC 6475 | |||
2857 | 17 52 21 | -34 46 30 | 30m | 103a - O | GG 385 | 1.5" | A.Twarog / Poblete | 07 05 78 | NGC 6475 | |||
2858 | 10 44 43 | -64 12 52 | 60m | 103a - D | GG 495 | 1.5" | A.Twarog / Poblete | 08 05 78 | IC 2602 | |||
2859 | 10 44 43 | -64 12 52 | 120m | 103a - O | UG 2 | 4" | A.Twarog / Poblete | 08 05 78 | IC 2602 | |||
2860 | 10 44 43 | -64 12 52 | 120m | 103a - O | UG 2 | 3" - 4" | A.Twarog / Poblete | 08 05 78 | IC 2602 | |||
2861 | 17 38 39 | -32 11 55 | 60m | 103a - D | GG 495 | 3" - 4" | A.Twarog / Poblete | 08 05 78 | NGC 6405 | |||
2862 | 17 38 39 | -32 11 55 | 40m | 103a - O | GG 385 | 3" - 4" | A.Twarog / Poblete | 08 05 78 | NGC 6405 | |||
2863 | 17 52 21 | -34 46 30 | 75m | 103a - D | GG 495 | 3" - 4" | A.Twarog / Poblete | 08 05 78 | NGC 6475 | |||
2864 | 17 52 21 | -34 46 30 | 75m | 103a - D | GG 14 | 2.5" | A.Twarog / Poblete | 08 05 78 | NGC 6475 | |||
2865 | 10 35 15 | -64 17 34 | 60m | 103a - D | GG 14 | 2" | A.Twarog / Poblete | 09 05 78 | IC 2602 | |||
2866 | 10 35 21 | -64 17 30 | 120m | 103a - O | UG 2 | 2" | A.Twarog / Poblete | 09 05 78 | IC 2602 | |||
2867 | 17 38 39 | -32 11 55 | 40m | 103a - O | GG 385 | 2" | A.Twarog / Poblete | 09 05 78 | IC 2602 | |||
2868 | 17 38 39 | -32 11 55 | 40m | 103a - O | GG 385 | 3" | A.Twarog / Poblete | 09 05 78 | NGC 6405 | |||
2869 | 17 38 39 | -32 11 55 | 120m | 103a - O | UG 2 | A.Twarog / Poblete | 09 05 78 | NGC 6405 | ||||
2870 | 17 52 21 | -34 46 30 | 120m | 103a - O | UG 2 | 1.5" | A.Twarog / Poblete | 09 05 78 | NGC 6475 | |||
2871 | 17 52 21 | -34 46 30 | 30m | 103a - O | GG 385 | 1.5" | A.Twarog / Poblete | 09 05 78 | NGC 6475 | |||
2872 | 10 35 16 | -64 17 34 | 60m | 103a - D | GG 14 | 2" | A.Twarog / Poblete | 10 05 78 | IC 2602 | |||
2873 | 10 35 16 | -64 17 34 | 120m | 103a - O | UG 2 | 1.5" - 4" | A.Twarog / Poblete | 10 05 78 | IC 2602 | |||
2874 | 10 35 16 | -64 17 34 | 40m | 103a - O | GG 385 | A.Twarog / Poblete | 10 05 78 | IC 2602 | ||||
2875 | 17 38 39 | -32 11 55 | 60m | 103a - D | GG 14 | A.Twarog / Poblete | 10 05 78 | NGC 6405 |
Last Updated on 8/27/99
By Guerra & Marin
August 1978 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2876 | 17 38 39 | -32 11 55 | 60m | lla - O | GG 385 | 1.5" | A.Twarog / Poblete | 02 08 78 | Sagitarius I | CTIO | ||
2877 | 17 52 21 | -34 46 30 | 120m | 103a - O | UG 2 | A.Twarog / Poblete | 10 05 78 | NGC 6475 | ||||
2878 | 17 57 31 | -29 08 47 | 30m | lla - O | GG 385 | 3" - 5" | J.Ríos | 03 08 78 | Sagitarius I | CTIO | ||
2879 | 17 57 31 | -29 08 47 | 20m | lla - D | GG 495 | 3" - 5" | J.Ríos | 03 08 78 | Sagitarius I | CTIO | ||
2880 | 17 57 31 | -29 08 47 | 30m | lla - O | GG 385 | 3" - 5" | J.Ríos | 03 08 78 | Sagitarius I | CTIO | ||
2881 | 17 57 31 | -29 08 47 | 20m | lla - D | GG 495 | 3" - 5" | J.Ríos | 03 08 78 | Sagitarius I | CTIO | ||
2882 | 17 57 31 | -29 08 47 | 30m | lla - O | GG 385 | 3" - 5" | J.Ríos | 03 08 78 | Sagitarius I | CTIO | ||
2883 | 17 57 31 | -29 08 47 | 20m | lla - D | GG 495 | 3" - 5" | J.Ríos | 03 08 78 | Sagitarius I | CTIO | ||
2884 | 17 57 31 | -29 08 47 | 30m | lla - O | GG 385 | 3" - 5" | J.Ríos | 03 08 78 | Sagitarius I | CTIO | ||
2885 | 17 57 31 | -29 08 47 | 20m | lla - D | GG 495 | 3" - 5" | J.Ríos | 03 08 78 | Sagitarius I | CTIO | ||
2886 | 22 56 12 | -41 09 40 | 90m | 103a - D | GG 495 | 3" | Elmegreen / R.Gonzalez | 31 08 78 | NGC 7424 | |||
2887 | 22 56 12 | -41 09 40 | 60m | 103a - O | GG 385 | 3" | Elmegreen / R.Gonzalez | 31 08 78 | NGC 7424 | |||
2888 | 22 56 12 | -41 09 40 | 180m | 103a - O | UG 2 | 3" | Elmegreen / R.Gonzalez | 31 08 78 | NGC 7424 | |||
2889 | 00 54 01 | -37 47 00 | 120m | 127 - 04 | RG 1 | 3" | Elmegreen / R.Gonzalez | 31 08 78 | NGC 300 |
Last Updated on 8/27/99
By Jorge Marin
September 1978 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2890 | 22 56 12 | -41 09 40 | 119m | 127 - 04 | RG 1 | 1.5" - 2" | Elmegreen / R.Gonzalez | 01 09 78 | NGC 7424 | |||
2891 | 22 56 12 | -41 09 40 | 150m | 098 - 04 | RG 1 | 2" - 3" | Elmegreen / R.Gonzalez | 02 09 78 | NGC 7424 | |||
2892 | 22 56 12 | -41 09 40 | 150m | 103a - O | GG 385 | 2" - 3" | Elmegreen / R.Gonzalez | 02 09 78 | NGC 7424 | |||
2893 | 01 35 41 | +15 42 | 90m | 103a - O | GG 385 | 2" | Elmegreen / R.Gonzalez | 02 09 78 | NGC 628 | |||
2894 | 01 35 41 | +15 42 | 199m | 103a - O | UG 2 | 2" | Elmegreen / R.Gonzalez | 02 09 78 | NGC 628 | |||
2895 | 22 56 12 | -41 09 40 | 240m | 098 - 04 | RG 1 | 1.5" | Elmegreen / R.Gonzalez | 03 09 78 | NGC 7424 | |||
2896 | 01 35 48 | +15 43 36 | 240m | 098 - 04 | RG 1 | 1" | Elmegreen / R.Gonzalez | 03 09 78 | NGC 628 | |||
2897 | 01 35 48 | +15 43 36 | 60m | 103a - D | GG 495 | 2" | Elmegreen / R.Gonzalez | 03 09 78 | NGC 628 | |||
2898 | 23 55 18 | -32 51 | 150m | 098 - 04 | RG 1 | 2" - 3" | Elmegreen / Czuia | 11 09 78 | NGC 7793 | |||
2899 | 23 55 18 | -32 51 | 90m | lla - O | GG 385 | 3" | Elmegreen / Czuia | 11 09 78 | NGC 7793 |
Last Updated on 8/27/99
By Guerra & Marin
November 1978 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2900 | 00 49 30 | -73 24 48 | 30m | 098 - 04 | RG 610 | 3" | Blanco / Ugarte | 12 11 78 | SMC - B48 | Broken bad cndtn | CTIO | |
2901 | 00 49 30 | -73 24 48 | 25m | 098 - 04 | RG 610 | 3" | Blanco / Ugarte | 12 11 78 | SMC - B48 | DESTROYED | CTIO | |
2902 | 00 49 30 | -73 24 48 | 90m | lN | RG 695 | 3" | Blanco / Ugarte | 12 11 78 | SMC - B48 | DESTROYED | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
1979 Plate logs for 1.5-m telescope
July 1979 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2903 | 18 02 17 | -30 01 08 | 20m | 103a - O | GG 385 | 2" - 4" | Graham / Ugarte | 02 07 79 | NGC 6522 | DESTROYED | CTIO | |
2904 | 20 04 30 | -44 48 02 | 13m | lla - O | GG 495 | 2" - 4" | Graham / Ugarte | 02 07 79 | E 8 Field | |||
2905 | 18 02 17 | -30 01 08 | 20m | 103a - O | GG 385 | 2" | Graham / Ugarte | 02 07 79 | NGC 6522 | DESTROYED | CTIO | |
2906 | 16 54 06 | -41 06 | 60m | 103a - O | 3" | Graham / Ugarte | 02 07 79 | TR 24/ NGC 6231 | ||||
2907 | 00 53 54 | -37 45 53 | 85m | lla - D | GG 495 | 1" | Graham / Ugarte | 02 07 79 | NGC 300 | |||
2908 | 00 53 54 | -37 45 53 | 75m | lla - O | GG 385 | 1" | Graham / Ugarte | 02 07 79 | NGC 300 | |||
2909 | 18 02 00 | -30 01 | 20m | 103a - O | GG 385 | 3" | Graham / Ugarte | 03 07 79 | NGC 6522 | Broken 3/4 plate | CTIO | |
2910 | 14 57 09 | -31 35 21 | 20m | 103a - O | GG 385 | 1" | Graham / Ugarte | 03 07 79 | Cen X - 4 | |||
2911 | 13 38 30 | -31 31 | 20m | 103a - O | GG 385 | 1" | Graham / Ugarte | 03 07 79 | NGC 5253 | |||
2912 | 18 02 00 | -30 01 | 20m | 103a - O | GG 385 | 1" | Graham / Ugarte | 03 07 79 | NGC 6522 | Broken Ok" | CTIO | |
2913 | 18 02 00 | -30 01 | 20m | 103a - O | GG 385 | 1" | Graham / Ugarte | 03 07 79 | NGC 6522 | Ok" | CTIO | |
2914 | 23 56 30 | -32 43 | 60m | 103a - O | GG 385 | 1" | Graham / Ugarte | 03 07 79 | NGC 7793 | |||
2915 | 00 53 54 | -37 45 53 | 10m | 103a - O | GG 385 | 1" | Graham / Ugarte | 03 07 79 | NGC 300 | |||
2916 | 00 53 54 | -37 45 53 | 60m | 103a - O | GG 385 | 1" | Graham / Ugarte | 03 07 79 | NGC 300 | |||
2917 | 00 53 54 | -37 45 53 | 90m | 103a - O | UG 2 | 2" | Graham / Ugarte | 03 07 79 | NGC 300 | |||
2918 | 00 53 54 | -37 45 53 | 20m | 103a - O | GG 385 | 2" | Graham / Ugarte | 03 07 79 | NGC 300 |
Last Updated on 8/27/99
By Guerra & Marin
August 1979 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2919 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | CTIO | ||
2920 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | CTIO | ||
2921 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | Broken bad cndtn | CTIO | |
2922 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | CTIO | ||
2923 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | CTIO | ||
2924 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | CTIO | ||
2925 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | CTIO | ||
2926 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | CTIO | ||
2927 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | Broken Ok" | CTIO | |
2928 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | Broken Ok" | CTIO | |
2929 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 2" | Blanco / Czuia | 02 08 79 | Baade´s Window | CTIO | ||
2930 | 18 02 24 | -30 01 | 14m | 103a - D | GG 495 | 2" | Blanco / Czuia | 02 08 79 | ||||
2931 | 00 55 24 | -72 37 | 40m | 098 - 04 | RG 610 | 2" | Blanco / Czuia | 03 08 79 | NGC 330 | CTIO | ||
2932 | 00 55 24 | -72 37 | 40m | 098 - 04 | RG 610 | 2" - 3" | Blanco / Ugarte | 04 08 79 | NGC 330 | CTIO | ||
2933 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2934 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 3" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2935 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 3" - 4" | Blanco / Ugarte | 05 08 79 | Baade´s Window | Broken Ok" | CTIO | |
2936 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 3" - 4" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2937 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 3" - 4" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2938 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 1" - 2" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2939 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2940 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 1" - 2" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2941 | 18 02 24 | -30 01 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2942 | 18 02 24 | -30 01 | 30m | 103a - D | GG 495 | 2" - 3" | Blanco / Ugarte | 05 08 79 | Baade´s Window | CTIO | ||
2943 | 00 55 24 | -72 37 | 120m | lN | RG 695 | 2" - 3" | Blanco / Ugarte | 05 08 79 | NGC 330 | CTIO | ||
2944 | 01 02 36 | -72 25 | 40m | 098 - 04 | RG 610 | 2" - 3" | Blanco / Ugarte | 05 08 79 | NGC 371 | CTIO | ||
2945 | 18 01 48 | -29 53 18 | 20m | 103a - O | GG 385 | 3" | Blanco / Martin | 17 08 79 | Baade´s Window | CTIO | ||
2946 | 18 01 48 | -29 53 18 | 30m | 103a - D | GG 495 | 3" | Blanco / Martin | 17 08 79 | Baade´s Window | CTIO | ||
2947 | 18 01 48 | -29 53 18 | 20m | 103a - O | GG 385 | 3" | Blanco / Martin | 17 08 79 | Baade´s Window | CTIO | ||
2948 | 18 01 48 | -29 53 18 | 30m | 103a - D | GG 495 | 2" - 3" | Blanco / Martin | 18 08 79 | ||||
2949 | 18 01 48 | -29 53 18 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Martin | 17 08 79 | Baade´s Window | CTIO | ||
2950 | 18 01 48 | -29 53 18 | 30m | 103a - D | GG 495 | 2" - 3" | Blanco / Martin | 18 08 79 | Baade´s Window | CTIO | ||
2951 | 01 15 06 | -73 27 | 60m | 098 - 04 | RG 610 | 2" - 3" | Blanco / Martin | 18 08 79 | NGC 465 | CTIO | ||
2952 | 01 07 12 | -73 05 | 60m | 098 - 04 | RG 610 | 2" - 3" | Blanco / Martin | 18 08 79 | NGC 419 | CTIO |
Last Updated on 8/27/99
By Jorge Marin
October 1979 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2953 | 01 17 52 | -28 44 45.6 | 15m | lla - O baked | RG 610 | 1.5" - 2" | Dufour et al / Cosgrove | 16 10 79 | Nov 19 event | |||
2954 | 01 17 52 | -28 44 45.6 | 30m | lla - O baked | UG 2 | 1.5" - 2" | Dufour et al / Cosgrove | 16 10 79 | Nov 19 event | |||
2955 | 01 17 52 | -28 44 45.6 | 30m | lla - O baked | GG 495 | 1.5" - 2" | Dufour et al / Cosgrove | 16 10 79 | Nov 19 event | |||
2956 | 01 17 52 | -28 44 45.6 | 10m | lla - O baked | GG 495 | 1.5" - 2" | Dufour et al / Cosgrove | 16 10 79 | Nov 19 event | |||
2957 | 01 17 52 | -28 44 45.6 | 60m | lla - O baked | 7 - 83 | 1.5" - 2" | Dufour et al / Cosgrove | 16 10 79 | Nov 19 event | |||
2958 | 01 17 52 | -28 44 45.6 | 10m | lla - O baked | 7 - 83 | 1.5" - 2" | Dufour et al / Cosgrove | 16 10 79 | Nov 19 event | |||
2959 | 05 26 08 | -66 06 03 | 2m | lla - O baked | RG 610 | 1.5" | Dufour et al / Cosgrove | 16 10 79 | N 49 | |||
2960 | 05 26 08 | -66 06 03 | 20m | lla - O baked | RG 610 | 1.5" | Dufour et al / Cosgrove | 16 10 79 | N 49 | |||
2961 | 05 26 08 | -66 06 03 | 1m | lla - O baked | GG 495 | 1.5" | Dufour et al / Cosgrove | 16 10 79 | N 49 | |||
2962 | 05 26 08 | -66 06 03 | 15m | lla - O baked | GG 495 | 1.5" | Dufour et al / Cosgrove | 16 10 79 | N 49 | |||
2963 | 05 26 08 | -66 06 03 | 45m | lla - O baked | 7 - 83 | 1.5" | Dufour et al / Cosgrove | 16 10 79 | N 49 | |||
2964 | 05 26 08 | -66 06 03 | 5m | lla - O baked | 7 - 83 | 1.5" | Dufour et al / Cosgrove | 16 10 79 | N 49 | |||
2965 | 01 17 52 | -28 44 45.6 | 25m | lla - O baked | 7 - 83 | 1.5" | Dufour et al / Cosgrove | 16 10 79 | Nov 19 event | |||
2966 | 01 17 52 | -28 44 45.6 | 5m | lla - O baked | GG 495 | 1.5" | Dufour et al / Cosgrove | 16 10 79 | Nov 19 event |
Last Updated on 8/27/99
By Guerra & Marin
December 1979 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2967 | 05 09 00 | -69 00 | 40m | 103a - O | GG 385 | 2" | Graham / Czuia | 20 12 79 | Bok - Tifft | |||
2968 | 04 59 02 | -66 01 17 | 40m | 103a - O | GG 385 | 2" | Graham / Czuia | 20 12 79 | NGC 1783 | |||
2969 | 04 03 04 | -44 46 54 | 3m | lla - O | GG 385 | 2" | Graham / Czuia | 20 12 79 | E 2 | |||
2970 | 06 41 53 | -45 07 31 | 3m | lla - O | GG 385 | 2" | Graham / Czuia | 20 12 79 | E 3 | |||
2971 | 05 08 58 | -69 00 19 | 40m | 103a - O | GG 385 | 2" - 3" | Graham / Czuia | 20 12 79 | Bok - Tifft | |||
2972 | 04 59 02 | -66 01 17 | 40m | 103a - O | GG 385 | 2" - 3" | Graham / Czuia | 20 12 79 | NGC 1783 | |||
2973 | 05 08 58 | -69 00 19 | 40m | 103a - O | GG 385 | 2" | Graham / Czuia | 20 12 79 | Bok - Tifft | |||
2974 | 04 59 02 | -66 01 17 | 40m | 103a - O | GG 385 | 2" | Graham / Czuia | 20 12 79 | NGC 1783 | |||
2975 | 05 08 58 | -69 00 19 | 60m | 103a - O | GG 385 | 2" | Graham / Czuia | 20 12 79 | Bok - Tifft | |||
2976 | 04 59 02 | -66 01 17 | 40m | 103a - O | GG 385 | 1" - 1.5" | Graham / Czuia | 21 12 79 | NGC 1783 | |||
2977 | 05 08 58 | -69 00 19 | 40m | 103a - O | GG 385 | 1" - 1.5" | Graham / Czuia | 21 12 79 | Bok - Tifft | |||
2978 | 04 03 04 | -44 46 54 | 6m | lla - D | GG 495 | 1" - 1.5" | Graham / Czuia | 21 12 79 | E 2 | |||
2979 | 05 08 58 | -69 00 19 | 40m | lla - D | GG 495 | 1" | Graham / Czuia | 21 12 79 | Bok - Tifft | |||
2980 | 05 08 58 | -69 00 19 | 40m | 103a - O | GG 385 | 1" | Graham / Czuia | 21 12 79 | Bok - Tifft | |||
2981 | 04 59 02 | -66 01 17 | 40m | 103a - O | GG 385 | 1" | Graham / Czuia | 21 12 79 | NGC 1783 | |||
2982 | 05 08 58 | -69 00 19 | 40m | 103a - O | GG 385 | 1.5" | Graham / Czuia | 21 12 79 | Bok - Tifft | |||
2983 | 04 59 02 | -66 01 17 | 40m | 103a - O | GG 385 | 1.5" | Graham / Czuia | 21 12 79 | NGC 1783 | |||
2984 | 05 08 58 | -69 00 19 | 40m | 103a - O | GG 385 | 1.5" | Graham / Czuia | 21 12 79 | Bok - Tifft |
Last Updated on 8/27/99
By Jorge Marin
1980 Plate logs for 1.5-m telescope
April 1980 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
2985 | 10 44 24 | -59 36 | 20m | 103a - O | GG 385 | 3" | Blanco / Martin | 15 04 80 | Trio Eta Carina | CTIO | ||
2986 | 08 39 42 | -52 59 | 5m | 103a - O | GG 385 | 3" | Blanco / Martin | 15 04 80 | IC 2391 | CTIO | ||
2987 | 12 38 48 | -11 31 | 30m | lla - O | 4" | Blanco / Martin | 15 04 80 | M 104 | ||||
2988 | 13 25 36 | -47 12 | 30m | lla - O | 3" - 4" | Blanco / Martin | 15 04 80 | Omega Cen. | ||||
2989 | 13 25 36 | -47 12 | 5m | lla - O | 3" | Blanco / Martin | 15 04 80 | Omega Cen. | ||||
2990 | 13 25 36 | -47 12 | 1m | lla - O | GG 385 | 3" | Blanco / Martin | 15 04 80 | Omega Cen. | CTIO | ||
2991 | 13 25 36 | -47 12 | 12s | lla - O | GG 385 | 3" | Blanco / Martin | 15 04 80 | Omega Cen. | CTIO | ||
2992 | 13 25 36 | -47 12 | 2s | lla - O | GG 385 | 3" | Blanco / Martin | 15 04 80 | Omega Cen. | CTIO | ||
2993a | 18 01 48 | -29 55 12 | 20m | 103a - O | GG 385 | 3" - 4" | Blanco / Martin | 15 04 80 | Baade´s Window | CTIO | ||
2993b | 13 19 30 | -46 56 54 | 8m - 4 - 2 - 1 | 103a - D | GG 385 | 2" | Blanco / Maturana | 16 06 80 | Flyspanker | |||
2994 | 13 19 30 | -46 56 54 | 8m - 4 - 2 - 1 | 103a - O | GG 385 | 2" | Blanco / Maturana | 15 04 80 | Flyspanker | CTIO | ||
2995 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
2996 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
2997 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
2998 | 18 01 54.6 | -29 55 13 | 25m | 103a - D | GG 495 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
2999 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | Broken Ok" | CTIO | |
3000 | 18 01 54.6 | -29 55 13 | 25m | 103a - D | GG 495 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
3001 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
3002 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
3003 | 18 01 54.6 | -29 55 13 | 25m | 103a - D | GG 495 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
3004 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
3005 | 18 01 54.6 | -29 55 13 | 25m | 103a - D | GG 495 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
3006 | 18 01 54.6 | -29 55 13 | 25m | 103a - O | GG 385 | 2" | Blanco / Maturana | 16 04 80 | Baade´s Window | CTIO | ||
3007 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" - 3" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3008 | 18 01 54.6 | -29 55 13 | 25m | 103a - D | GG 495 | 2" - 3" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3009 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 2" - 3" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3010 | 16 22 56 | -25 14 57 | lla - O | GG 385 | 1" - 1.5" | Blanco / Alday | 17 04 80 | Hyperher | Bad plate broken | CTIO | ||
3011 | 18 01 54.6 | -29 55 13 | 15m | 103a - D | GG 495 | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | |||
3012 | 18 01 54.6 | -29 55 13 | 20m | 103a - O | GG 385 | 1" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3013 | 18 01 54.6 | -29 55 13 | 15m | 103a - D | GG 495 | 1" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3014 | 18 01 54.6 | -29 55 13 | 20m | 103a - O | GG 385 | 1" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3015 | 18 01 54.6 | -29 55 13 | 25m | 103a - D | 1" | Blanco / Alday | 17 06 80 | Baade´s Window | ||||
3016 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 1" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3017 | 18 01 54.6 | -29 55 13 | 25m | 103a - D | GG 495 | 1" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3018 | 18 01 54.6 | -29 55 13 | 30m | 103a - O | GG 385 | 1" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO | ||
3019 | 18 01 54.6 | -29 55 13 | 30m | 103a - D | GG 495 | 1" | Blanco / Alday | 17 04 80 | Baade´s Window | CTIO |
Last Updated on 8/27/99
By Jorge Marin
September 1980 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3020 | 19 43 48 | -14 49 | 60m | 103a - O | GG 385 | 2" | Graham / Cosgrove | 10 09 80 | NGC 6822 | |||
3021 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | Graham / Cosgrove | 10 09 80 | NGC 121 | ||||
3022 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 2" | Graham / Cosgrove | 10 09 80 | NGC 121 | |||
3023 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 2" - 3" | Graham / Cosgrove | 10 09 80 | NGC 121 | |||
3024 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 2" - 4" | Graham / Cosgrove | 10 09 80 | NGC 121 | |||
3025 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 2" - 4" | Graham / Cosgrove | 10 09 80 | NGC 121 | |||
3026 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 2" - 3" | Graham / Cosgrove | 10 09 80 | NGC 121 | |||
3027 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 2" - 4" | Graham / Cosgrove | 10 09 80 | NGC 121 | |||
3028 | 17 38 48 | -53 40 | 60m | 103a - O | GG 385 | 1" - 2" | Graham / Cosgrove | 11 09 80 | NGC 6397 | |||
3029 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 1" - 2" | Graham / Cosgrove | 11 09 80 | NGC 121 | |||
3030 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 1.5" | Graham / Cosgrove | 11 09 80 | NGC 121 | |||
3031 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 1" | Graham / Cosgrove | 11 09 80 | NGC 121 | |||
3032 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 1" | Graham / Cosgrove | 11 09 80 | NGC 121 | |||
3033 | 00 25 42 | -71 41 | 40m | 103a - O | GG 385 | 1" | Graham / Cosgrove | 11 09 80 | NGC 121 | |||
3034 | 00 25 42 | -71 41 | 60m | 103a - O | GG 385 | 1.5" | Graham / Cosgrove | 11 09 80 | NGC 121 | |||
3035 | 00 25 42 | -71 41 | 50m | 103a - O | GG 385 | 2" | Graham / Cosgrove | 11 09 80 | NGC 121 | |||
3036 | 00 25 42 | -71 41 | 50m | 103a - O | GG 385 | 1" | Graham / Cosgrove | 11 09 80 | NGC 121 |
Last Updated on 8/27/99
By Guerra & Marin
October 1980 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3037 | 00 25 59 | -71 41 09 | 60m | 103a - O | GG 385 | 5" - 10" | Graham / Alday | 11 10 80 | NGC 121 | |||
3038 | 00 25 59 | -71 41 09 | 60m | 103a - O | GG 385 | 5" | Graham / Alday | 11 10 80 | NGC 121 | |||
3039 | 00 26 00 | -71 41 06 | 60m | 103a - O | GG 385 | 5" | Graham / Alday | 11 10 80 | NGC 121 | |||
3040 | 00 26 00 | -71 41 06 | 60m | 103a - O | GG 385 | 5" | Graham / Alday | 11 10 80 | NGC 121 | |||
3041 | 00 26 00 | -71 41 06 | 60m | 103a - O | GG 385 | 3" - 5" | Graham / Alday | 11 10 80 | NGC 121 | |||
3042 | 00 26 00 | -71 41 06 | 60m | 103a - O | GG 385 | 3" - 5" | Graham / Alday | 11 10 80 | NGC 121 | |||
3043 | 00 26 00 | -71 41 06 | 60m | 103a - O | GG 385 | 5" | Graham / Alday | 11 10 80 | NGC 121 |
Last Updated on 8/27/99
By Guerra & Marin
1981 Plate logs for 1.5-m telescope
March 1981 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3044 | 06 11 36 | -69 07 | 40m | 103a - O | GG 385 | 3" | Graham / Martin | 01 03 81 | NGC 2210 | |||
3045 | 06 11 29.6 | -69 07 22 | 60m | 103a - D | GG 495 | 3" | Graham / Martin | 01 03 81 | NGC 2210 | |||
3046 | 06 11 29.6 | -69 07 22 | 60m | 103a - O | GG 385 | 3" | Graham / Martin | 01 03 81 | NGC 2210 | |||
3047 | 06 11 29.6 | -69 07 22 | 60m | 103a - O | GG 385 | 3" | Graham / Martin | 01 03 81 | NGC 2210 | |||
3048 | 13 24 52 | -42 49 47 | 30m | 103a - D | GG 495 | 3" | Graham / Martin | 01 03 81 | NGC 5128 | |||
3049 | 13 24 50 | -42 49 39 | 30m | 103a - D | GG 495 | 3" | Graham / Martin | 01 03 81 | NGC 5128 | |||
3050 | 06 11 33.6 | -69 06 22 | 60m | 103a - O | GG 385 | 1" - 3" | Graham / Martin | 02 03 81 | NGC 2210 | |||
3051 | 06 11 33.6 | -69 06 22 | 60m | 103a - O | GG 385 | 1" - 3" | Graham / Martin | 02 03 81 | NGC 2210 | |||
3052 | 06 11 33.6 | -69 06 22 | 60m | 103a - O | GG 385 | 1" - 3" | Graham / Martin | 02 03 81 | NGC 2210 | |||
3053 | 06 11 33.6 | -69 06 22 | 60m | 103a - O | GG 385 | 1" - 3" | Graham / Martin | 02 03 81 | NGC 2210 | |||
3054 | 06 11 33.6 | -69 06 22 | 40m | 103a - O | GG 385 | 1" - 3" | Graham / Martin | 02 03 81 | NGC 2210 | |||
3055 | 13 24 30 | -42 49 30 | 80m | llla - J | 1" | Graham / Martin | 02 03 81 | NGC 5128 | ||||
3056 | 13 04 06 | -49 22 | 60m | 103a - D | GG 495 | 2" - 3" | Graham / Martin | 02 03 81 | NGC 4945 | |||
3057 | focus plate | 103a - O | GG 385 | 2" - 3" | Blanco / Martin | 03 03 81 | focus plate | |||||
3058 | focus plate | 103a - O | GG 385 | 2" | Blanco / Martin | 03 03 81 | focus plate | |||||
3059 | focus plate | 103a - O | GG 385 | 2" | Blanco / Martin | 03 03 81 | focus plate | |||||
3060 | focus plate | 103a - O | GG 385 | 2" | Blanco / Martin | 03 03 81 | focus plate | |||||
3061 | focus plate | 103a - O | GG 385 | 2" | Blanco / Martin | 03 03 81 | focus plate | |||||
3062 | focus plate | 103a - O | GG 385 | 2" | Blanco / Martin | 03 03 81 | focus plate | |||||
3063 | 18 00 23 | -30 04 46 | 15m | 103a - O | GG 385 | 2" | Blanco / Martin | 03 03 81 | NGC 6522 | CTIO | ||
3064 | 18 00 23 | -30 04 46 | 15m | 103a - O | GG 385 | 3" | Blanco / Martin | 03 03 81 | NGC 6522 | CTIO | ||
3065 | 13 25 12.5 | -42 42 06 | 5m | lla - O | GG 385 | 2" | Graham / Maturana | 25 03 81 | N 5128 | |||
3066 | 13 25 12.5 | -42 42 06 | 30m | lla - O | GG 385 | 2" - 3" | Graham / Maturana | 25 03 81 | N 5128 | |||
3067 | 13 25 12.5 | -42 42 06 | 10m | lla - D | GG 495 | 2" - 3" | Graham / Maturana | 25 03 81 | N 5128 | |||
3068 | 13 25 12.5 | -42 42 06 | 45m | lla - D | GG 495 | 2" | Graham / Maturana | 25 03 81 | N 5128 | |||
3069 | 13 25 12.5 | -42 42 06 | 60m | lla - O | UG 2 | 3" | Graham / Maturana | 25 03 81 | N 5128 | |||
3070 | 13 25 12.5 | -42 42 06 | GG 385 | Graham / Maturana | 25 03 81 | N 5128 |
Last Updated on 8/27/99
By Guerra & Marin
August 1981 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3071 | 15 35 48 | -28 04 | 10s each | 103a - D | 2" | Blanco / Martin | 03 08 81 | focus plate | ||||
3072 | 18 01 54 | -29 57 | 40m | 103a - O | GG 385 | 2" | Blanco / Martin | 03 08 81 | Baade's Window | CTIO |
Last Updated on 8/27/99
By Jorge Marin
October 1981 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3073 | 21 31 30 | -67 47 42 | 15s each | 103a - O | GG 385 | 1.5" | Klemola / Martin | 27 10 81 | focus plate | |||
3074 | 01 22 23 | -42 24 18 | 10m | 103a - J | GG 385 | 3" | Klemola / Martin | 27 10 81 | U Y Phe | |||
3075 | 00 26 03 | -71 38 15 | 60m | 103a - O | GG 385 | 1.5" | Klemola / Martin | 28 10 81 | NGC 121 | |||
3076 | 00 26 03 | -71 38 15 | 60m | 103a - O | GG 385 | 1.5" | Klemola / Martin | 28 10 81 | NGC 121 | |||
3077 | 00 26 03 | -71 38 15 | 60m | 103a - O | GG 385 | 1" | Klemola / Martin | 28 10 81 | NGC 121 | |||
3078 | 00 26 03 | -71 38 15 | 60m | 103a - O | GG 385 | 1.5" | Klemola / Martin | 28 10 81 | NGC 121 | |||
3079 | 00 26 03 | -71 38 15 | 60m | 103a - O | GG 385 | 1" | Klemola / Martin | 28 10 81 | NGC 121 | |||
3080 | 04 19 58 | -69 00 52 | 50m | llla - J | GG 385 | 1" | Klemola / Martin | 28 10 81 | LMC 0421 - 69 | |||
3081 | 04 19 58 | -69 00 52 | 50m | llla - J | GG 385 | 1" | Klemola / Martin | 28 10 81 | LMC 0421 - 69 | |||
3082 | 00 25 36 | -71 39 54 | 60m | 103a - O | GG 385 | 1.5 - 3" | Klemola / Ugarte | 29 10 81 | NGC 121 | |||
3083 | 00 25 36 | -71 39 54 | 60m | 103a - O | GG 385 | 1.5 3" | Klemola / Ugarte | 29 10 81 | NGC 121 | |||
3084 | 00 25 36 | -71 39 54 | 60m | 103a - O | GG 385 | 2" - 3" | Klemola / Ugarte | 29 10 81 | NGC 121 | |||
3085 | 00 25 36 | -71 39 54 | 60m | 103a - O | GG 385 | 2" - 3" | Klemola / Ugarte | 29 10 81 | NGC 121 | |||
3086 | 00 25 36 | -71 39 54 | 60m | 103a - O | GG 385 | 1.5" - 2" | Klemola / Ugarte | 29 10 81 | NGC 121 | |||
3087 | 04 19 56 | -69 00 58 | 60m | llla - J | GG 385 | 1.5" - 2" | Klemola / Ugarte | 29 10 81 | LMC 0421 - 69 | |||
3088 | 04 19 56 | -69 00 58 | 60m | llla - J | GG 385 | 1.5" - 2" | Klemola / Ugarte | 29 10 81 | LMC 0421 - 69 | |||
3089 | 05 18 06 | -68 22 31 | 5m | llla - J | GG 385 | 1.5" - 2" | Klemola / Ugarte | 29 10 81 | Stellar group | |||
3090 | 00 25 48 | -71 39 12 | 60m | 103a - O | GG 385 | 1" - 1.5" | Klemola / Ugarte | 30 10 81 | NGC 121 | |||
3091 | 00 25 48 | -71 39 12 | 60m | 103a - O | GG 385 | 1" - 3" | Klemola / Ugarte | 30 10 81 | NGC 121 | |||
3092 | 00 25 48 | -71 39 12 | 60m | 103a - O | GG 385 | 1" -1.5" | Klemola / Ugarte | 30 10 81 | NGC 121 | |||
3093 | 00 25 48 | -71 39 12 | 60m | 103a - O | GG 385 | 1" -1.5" | Klemola / Ugarte | 30 10 81 | NGC 121 | |||
3094 | 00 25 48 | -71 39 12 | 60m | 103a - O | GG 385 | 1" -1.5" | Klemola / Ugarte | 30 10 81 | NGC 121 | |||
3095 | 04 19 57 | -69 00 45 | 60m | llla - J | GG 385 | 1" -1.5" | Klemola / Ugarte | 30 10 81 | LMC 0421 - 69 | |||
3096 | 04 19 57 | -69 00 45 | 60m | llla - J | GG 385 | 1" -1.5" | Klemola / Ugarte | 30 10 81 | LMC 0421 - 69 | |||
3097 | 05 18 04 | -68 22 28 | 5m | llla - J | GG 385 | 1" -1.5" | Klemola / Ugarte | 30 10 81 | Stellar group | |||
3098 | 05 18 04 | -68 22 28 | 5m | llla - J | GG 385 | 1" -1.5" | Klemola / Ugarte | 30 10 81 | Stellar group | |||
3099 | 00 25 50 | -71 38 11 | 60m | 103a - O | GG 385 | 1" -1.5" | Klemola / Ugarte | 31 10 81 | NGC 121 | |||
3100 | 00 25 50 | -71 38 11 | 60m | 103a - O | GG 385 | 0.5" - 1" | Klemola / Ugarte | 31 10 81 | NGC 121 | |||
3101 | 00 25 50 | -71 38 11 | 60m | 103a - O | GG 385 | 1" - 1.5" | Klemola / Ugarte | 31 10 81 | NGC 121 | |||
3102 | 00 25 50 | -71 38 11 | 60m | 103a - O | GG 385 | 1" - 1.5" | Klemola / Ugarte | 31 10 81 | NGC 121 | |||
3103 | 00 25 50 | -71 38 11 | 60m | 103a - O | GG 385 | 1" - 1.5" | Klemola / Ugarte | 31 10 81 | NGC 121 | |||
3104 | 04 19 53 | -69 00 56 | 60m | llla - J | GG 385 | 1" - 1.5" | Klemola / Ugarte | 31 10 81 | LMC 0421 - 69 | |||
3105 | 04 19 53 | -69 00 56 | 60m | 103a - D | GG 495 | 1" - 1.5" | Klemola / Ugarte | 31 10 81 | LMC 0421 - 69 | |||
3106 | 05 18 02 | -68 22 10 | 5m | 103a - D | GG 495 | 1" - 1.5" | Klemola / Ugarte | 31 10 81 | Stellar group |
Last Updated on 8/27/99
By Guerra & Marin
November 1981 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3107 | 00 25 41 | -71 38 33 | 50m | 103a - O | GG 385 | 1" - 1.5" | Klemola / Ugarte | 01 11 81 | NGC 121 | |||
3108 | 00 25 41 | -71 38 33 | 50m | 103a - O | GG 385 | 1.5" | Klemola / Ugarte | 01 11 81 | NGC 121 | |||
3109 | 00 25 41 | -71 38 33 | 60m | 103a - O | GG 385 | 1.5" | Klemola / Ugarte | 01 11 81 | NGC 121 | |||
3110 | 00 25 41 | -71 38 33 | 60m | 103a - O | GG 385 | 1.5" | Klemola / Ugarte | 01 11 81 | NGC 121 | |||
3111 | 00 25 41 | -71 38 33 | 60m | 103a - O | GG 385 | 1.5" | Klemola / Ugarte | 01 11 81 | NGC 121 | |||
3112 | 04 19 47 | -69 00 57 | 55m | llla - J | GG 385 | 1.5" | Klemola / Ugarte | 01 11 81 | LMC 0421 - 69 | |||
3113 | 04 19 47 | -69 00 57 | 60m | llla - J | GG 385 | 1.5" | Klemola / Ugarte | 01 11 81 | LMC 0421 - 69 | |||
3114 | 04 19 47 | -69 00 57 | 60m | 103a - D | GG 495 | 1.5" | Klemola / Ugarte | 01 11 81 | LMC 0421 - 69 | |||
3115 | 04 54 24 | -69 51 | 25m | 098 - 04 | RG 610 | 2.5" | Blanco / Ugarte | 02 11 81 | NGC 1751 | CTIO | ||
3116 | 04 58 24 | -66 02 | 25m | 098 - 04 | RG 610 | 2.5" | Blanco / Ugarte | 02 11 81 | NGC 1783 | CTIO | ||
3117 | 05 07 36 | -67 30 | 25m | 098 - 04 | RG 610 | 2.5" | Blanco / Ugarte | 02 11 81 | NGC 1846 | CTIO | ||
3118 | 05 13 24 | -65 29 | 25m | 098 - 04 | RG 610 | 2.5" | Blanco / Ugarte | 02 11 81 | NGC 1866 | CTIO | ||
3119 | 05 57 30 | -67 15 | 25m | 098 - 04 | RG 610 | 2.5" | Blanco / Ugarte | 02 11 81 | NGC 2154 | CTIO | ||
3120 | 06 11 06 | -71 33 | 25m | 098 - 04 | RG 610 | 2.5" | Blanco / Ugarte | 02 11 81 | NGC 2213 | CTIO | ||
3121 | 06 29 48 | -64 09 | 25m | 098 - 04 | RG 610 | 2.5" | Blanco / Ugarte | 02 11 81 | NGC 2257 | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
December 1981 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3122 | 06 05 33.8 | -75 25 29 | 40m | lla - O | GG 385 | 2" - 3" | Graham / Martin | 24 12 81 | NGC 2203 | |||
3123 | 06 05 31 | -75 25 48 | 60m | 103a - D | GG 495 | 2" - 3" | Graham / Martin | 24 12 81 | NGC 2203 | |||
3124 | 06 05 31 | -75 25 48 | 40m | lla - O | GG 385 | 2" - 3" | Graham / Martin | 24 12 81 | NGC 2203 | |||
3125 | 06 05 31 | -75 25 48 | 45m | lla - O | GG 385 | 2" - 3" | Graham / Martin | 24 12 81 | NGC 2203 | |||
3126 | 06 05 31 | -75 25 48 | 60m | 103a - D | GG 495 | 2" | Graham / Martin | 24 12 81 | NGC 2203 | |||
3127 | 06 05 31 | -75 25 48 | 20m | lla - O | GG 385 | 2" | Graham / Martin | 24 12 81 | NGC 2203 | |||
3128 | 06 05 31 | -75 25 48 | 40m | lla - O | GG 385 | 2" | Graham / Martin | 24 12 81 | NGC 2203 | |||
3129 | 06 05 25 | -75 24 18 | 45m | lla - O | GG 385 | 2" | Graham / Ugarte | 27 12 81 | NGC 2203 | |||
3130 | 06 11 34.3 | -69 05 15 | 60m | 103a - O | GG 385 | 2" | Graham / Ugarte | 27 12 81 | NGC 2210 | |||
3131 | 06 05 18.7 | -75 25 07 | 40m | lla - O | GG 385 | 2" | Graham / Ugarte | 27 12 81 | NGC 2203 | |||
3132 | 06 05 18.7 | -75 25 07 | 40m | lla - O | GG 385 | 2" | Graham / Ugarte | 27 12 81 | NGC 2203 | |||
3133 | 06 05 18.7 | -75 25 07 | 40m | lla - O | GG 385 | 1" | Graham / Ugarte | 27 12 81 | NGC 2203 | |||
3134 | 06 11 26 | -69 05 33 | 60m | 103a - O | GG 385 | 1.5" | Graham / Ugarte | 27 12 81 | NGC 2210 | |||
3135 | 06 05 09 | -75 25 04 | 45m | lla - O | GG 385 | 1.5" | Graham / Ugarte | 27 12 81 | NGC 2203 |
Last Updated on 8/27/99
1982 Plate logs for 1.5-m telescope
February 1982 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3136 | 05 01 00 | -69 40 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | LMC 50-69.7 | CTIO | ||
3137 | 05 09 09.8 | -68 52 29 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | NGC 1854 | CTIO | ||
3138 | 05 43 27.4 | -70 39 01 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | NGC 2107 | CTIO | ||
3139 | 05 44 00 | -69 13 52 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | NGC 2108 | CTIO | ||
3140 | 05 53 00 | -69 30 00 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | NGC 2136 | CTIO | ||
3141 | 06 11 04.4 | -71 33 14 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | NGC 2213 | CTIO | ||
3142 | 06 20 30 | -67 31 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | NGC 2231 | CTIO | ||
3143 | 06 12 54 | -68 16 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | NGC 2214 | CTIO | ||
3144 | 05 09 09.8 | -60 52 29 | 15m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | NGC 1854 | CTIO | ||
3145 | 06 40 30 | -50 57 06 | 30m | 098 - 04 | RG 610 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | Dwarf Car. Galaxy | CTIO | ||
3146 | 08 54 16 | -47 30 04 | lla - O | GG 385 | 1.5" | Blanco / Cosgrove / Hernandez | 04 02 82 | ?? | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
April 1982 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3147 | 08 18 00 | -30 00 | 10s | llla - J | 2" | Ugarte / R.Gonzalez | 15 04 82 | Focus plate | ||||
3148 | 08 49 00 | -30 00 | 10s | llla - J | Ugarte / R.Gonzalez | 15 04 82 | Focus plate | |||||
3149 | 09 10 00 | +30 00 | 10s | llla - J | Ugarte / R.Gonzalez | 15 04 82 | focus north | |||||
3150 | 09 20 00 | -90 00 | 10s | llla - J | Ugarte / R.Gonzalez | 15 04 82 | focus south | |||||
3151 | 13 28 00 | -30 00 | 10s | llla - J | Ugarte / R.Gonzalez | 15 04 82 | focus east | |||||
3152 | 05 45 00 | -30 00 | 10s | llla - J | Ugarte / R.Gonzalez | 15 04 82 | focus west | |||||
3153 | 07 55 00 | -30 00 | 10s | 103a - O | 1" - 2" | Graham / Ugarte | 16 04 82 | focus zenith | ||||
3154 | +30 00 | 10s | 103a - O | Graham / Ugarte | 16 04 82 | focus north | ||||||
3155 | 09 25 00 | -90 00 | 10s | 103a - O | 1" - 2" | Graham / Ugarte | 16 04 82 | focus south | ||||
3156 | 13 37 00 | -30 00 | 10s | 103a - O | 1" - 2" | Graham / Ugarte | 16 04 82 | focus east | ||||
3157 | 06 12 00 | -30 00 | 10s | 103a - O | 1" - 2" | Graham / Ugarte | 16 04 82 | focus west |
Last Updated on 8/27/99
By Jorge Marin
August 1982 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3158 | zenith | 10s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | focus | |||||
3159 | 16 47 00 | -56 46 | 2m / 10m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Nor 2645 | ||||
3160 | 16 51 00 | -57 12 | 10m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Nor 305 - 6 | ||||
3161 | 17 21 00 | -67 57 | 2m20s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Nor 600 - 1 | ||||
3162 | 18 13 00 | -66 55 | 2m20s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Nor 857 - 60 | ||||
3163 | 17 56 00 | -32 55 | 10m2s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 79 - 81 | ||||
3164 | 17 56 00 | -34 27 | 10m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 83 | ||||
3165 | 17 58 00 | -30 17 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 149 | ||||
3166 | 18 02 00 | -29 59 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 265 | ||||
3167 | 18 02 00 | -28 08 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 268 | ||||
3168 | 18 03 00 | -34 23 | 5m+1m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 330 | ||||
3169 | 18 04 00 | -27 52 | 5m+1m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 361 - 2 | ||||
3170 | 18 04 00 | -27 55 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 386 - 7 | ||||
3171 | 18 05 00 | -26 42 | 3m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 455 | ||||
3172 | 18 06 00 | -31 51 | 7m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 487 | ||||
3173 | 18 07 00 | -26 30 30 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 552 | ||||
3174 | 18 09 00 | -28 06 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 605 | ||||
3175 | 18 12 00 | -29 45 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 805 | ||||
3176 | 18 17 00 | -34 27 | 3m20s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 1138 | ||||
3177 | 18 21 00 | -39 40 | 2m20s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 1326 | ||||
3178 | 18 23 00 | -27 02 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 1403 | ||||
3179 | 18 15 00 | -23 29 | 3m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr W 990 | ||||
3180 | 18 28 00 | -31 29 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Sgr E 179 | ||||
3181 | 20 56 00 | -14 28 30 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Cap 21 - 22 | ||||
3182 | 21 35 30 | -19 27 | 5m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Cap 123 - 4 | ||||
3183 | 22 34 00 | -45 04 | 7m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Par 84 - 85 | ||||
3184 | 20 57 00 | -49 21 | 10m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | 2054 - 492 | ||||
3185 | 23 19 00 | -05 15 | 2.5m+30s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Feije 110 | ||||
3186 | 23 19 00 | -05 15 | 2.5m+30s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Feije 110 | ||||
3187 | 02 34 00 | -16 12 | 5m+20s | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Cet 15 - 17 | ||||
3188 | 02 35 00 | -08 57 | 5m+1m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Cet 22 - 23 | ||||
3189 | 02 52 00 | -20 18 | 5m+1m | lla - O | 1" - 2" | Bozyan / Opal / R.Gonzalez | 08 08 82 | Cet 37 - 41 | ||||
3190 | 17 14 59 | -62 47 21 | 20m | lla - O | GG 385 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | NG 300 | |||
3191 | 17 14 59 | -62 47 21 | 90m | lla - O | UG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | NG 300 | |||
3192 | 20 36 23 | -23 37 36 | 20m | lla - O | GG 385 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | 2034 - 274 | |||
3193 | 19 16 51 | -60 34 18 | 90m | llla - F | H alpha | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | NG 769 / 70 | |||
3194 | 19 14 01 | -54 40 15 | 90m | llla - F | GG 50 H alpha | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | 1911 - 544 | |||
3195 | 21 28 00 | -22 17 | 10s | llla - F | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | Vesta | ||||
3196 | 00 45 40 | -52 08 | 60m | llla - F | RG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | 0045 - 522 | |||
3197 | 01 12 24 | -00 36 42 | 3s 30s | lla - O | GG 385 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | 9 Metis | |||
3198 | 01 19 07 | -41 15 29 | 20m | lla - O | GG 385 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | VV 578 | |||
3199 | 00 53 42 | -32 06 45 | 72m | llla - F | RG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 09 08 82 | 00 52 - 3210 | |||
3200 | 17 14 59 | -62 46 26 | 60m | lla - D | GG 495 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | NG 300 | |||
3201 | 17 27 16 | -62 26 29 | 30m | lla - O | GG 385 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | 1724 - 621 | |||
3202 | 17 27 16 | -62 26 29 | 90m | lla - O | UG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | 1724 - 621 | |||
3203 | 18 50 26 | 10 17 39 | 3m 1m 30s | 103a - D | GG 495 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | N 6709 | |||
3204 | 18 50 26 | 10 17 39 | 3m 1m 30s | lla - O | GG 385 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | N 6709 | |||
3205 | 18 50 26 | 10 17 39 | 6m 3m 1m | lla - O | UG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | N 6709 | |||
3206 | 19 16 51 | -60 34 18 | 180m | llla - F | H alpha | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | NG 769 / 70 | |||
3207 | 22 45 59 | -65 08 12 | 60m | llla - F | RG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | 2244 - 651 | |||
3208 | 01 18 58 | -41 22 17 | 60m | llla - F | RG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 10 08 82 | VV 578 | |||
3209 | 16 22 30 | -26 28.4 | 60m | 103a - D | GG 495 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 11 08 82 | M 4 | |||
3210 | 19 16 51 | -60 32 34 | 60m | 103a - D | GG 495 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 11 08 82 | N 6769 - 70 | |||
3211 | 19 13 59 | -54 40 17 | 60m | 103a - D | GG 495 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 11 08 82 | 1911 - 544 | |||
3212 | 22 45 56 | -65 08 18 | 30m | lla - O | GG 385 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 11 08 82 | 2244 - 651 | |||
3213 | 22 27 37 | -24 56 40 | 30m | lla - O | GG 385 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 2225 - 250 | ||||
3214 | 18 35 17 | -23 56 19 | 15m | 103a - D | GG 495 | 1" - 2" | Bozyan / Opal / R.Gonzalez | M 22 | ||||
3215 | 19 16 51 | -60 34 16 | 60m | llla - F | RG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | M 6769 - 70 | ||||
3216 | 22 27 37 | -24 56 43 | 60m | llla - F | RG 1 | 1" - 2" | Bozyan / Opal / R.Gonzalez | 2225 - 25º | ||||
3217 | 00 14 00 | -39 19 27 | 130m | llla - F | H alpha | 1" - 2" | Bozyan / Opal / R.Gonzalez | N 55 |
Last Updated on 8/27/99
By Jorge Marin
1983 Plate logs for 1.5-m telescope
November 1983 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3218 | 00 20 18 | -74 30 | 5m | 098 - 04 | RG 610 | 1.5" | Bravo | 21 11 83 | SMC. C -area A | CTIO | ||
3219 | 00 30 24 | -75 01 | 5m | 098 - 04 | RG 610 | 1" | Bravo | 22 11 83 | SMC. C -area B | CTIO | ||
3220 | 00 35 18 | -74 15 | 5m | 098 - 04 | RG 610 | 1" | Bravo | 22 11 83 | SMC. C -area C | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
1984 Plate logs for 1.5-m telescope
January 1984 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3221 | 05 20 49.6 | -68 37 37 | 40m | lla - O bkd | GG 385 | <1" | Blanco / Cosgrove | 04 01 84 | LMC. RR - A | CTIO | ||
3222 | 05 20 49.6 | -68 37 37 | 40m | lla - O | GG 385 | <1" | Blanco / Cosgrove | 04 01 84 | LMC. RR - A | CTIO | ||
3223 | 05 20 49.6 | -68 37 37 | 30m | lla - O bkd | GG 385 | 1" | Blanco / Cosgrove | 04 01 84 | LMC. RR - A | CTIO | ||
3224 | 05 20 49.8 | -68 37 35 | 31m10s | lla - O bkd | GG 385 | <1" | Blanco / Hernandez | 05 01 84 | LMC. RR - A | CTIO | ||
3225 | 05 20 48.8 | -68 37 37 | 45m | lla - O bkd | GG 385 | 1" | Blanco / Cosgrove | 30 01 84 | LMC. RR - A | CTIO | ||
3226 | 05 20 48.8 | -68 37 37 | 45m | lla - O bkd | GG 385 | <1" | Blanco / Cosgrove | 30 01 84 | LMC. RR - A | CTIO | ||
3227 | 05 20 48.8 | -68 37 37 | 45m | lla - O bkd | GG 385 | 1.5" | Blanco / Cosgrove | 30 01 84 | LMC. RR - A | CTIO | ||
3228 | 05 20 48.8 | -68 37 37 | 45m | lla - O bkd | GG 385 | 2.5" | Blanco / Cosgrove | 30 01 84 | LMC. RR - A | CTIO | ||
3229 | 05 20 48.8 | -68 37 37 | 45m | lla - O bkd | GG 385 | Blanco / Cosgrove | 30 01 84 | LMC. RR - A | CTIO | |||
3230 | 05 20 48.8 | -68 37 37 | 45m | 103a-O bkd | GG 385 | 1.5" | Blanco / Cosgrove | 01 02 84 | LMC. RR - A | CTIO | ||
3231 | 05 20 48.8 | -68 37 37 | 45m | 103a-O bkd | GG 385 | 1.5" | Blanco / Cosgrove | 01 02 84 | LMC. RR - A | CTIO | ||
3232 | 05 20 48.8 | -68 37 37 | 45m | 103a-O bkd | GG 385 | 1" | Blanco / Cosgrove | 01 02 84 | LMC. RR - A | DESTROYED | CTIO | |
3233 | 05 20 48.8 | -68 37 37 | 45m | 103a-O bkd | GG 385 | 1" | Blanco / Cosgrove | 01 02 84 | LMC. RR - A | CTIO | ||
3234 | 05 20 48.8 | -68 37 37 | 45m | 103a-O bkd | GG 385 | 1" | Blanco / Cosgrove | 01 02 84 | LMC. RR - A | CTIO | ||
3235 | 05 20 48.8 | -68 37 37 | 45m | 103a-O bkd | GG 385 | 1.5" | Blanco / Cosgrove | 01 02 84 | LMC. RR - A | CTIO | ||
3236 | -61 47 | 10s each | lla - O bkd | GG 385 | 2" | Martin / Cosgrove | 20 01 84 | Focus Plate | CTIO | |||
3237 | -33 00 | 10s | lla - O bkd | GG 385 | 2" | Martin / Cosgrove | 20 01 84 | Focus Plate Zenit | CTIO | |||
3238 | -24 00 | 10s | lla - O bkd | GG 385 | 2" | Martin / Cosgrove | 20 01 84 | Focus Plate East | CTIO | |||
3239 | -36 00 | 10s | lla - O bkd | GG 385 | 2" | Martin / Cosgrove | 20 01 84 | Focus Plate West | CTIO | |||
3240 | +14 00 | 10s | lla - O bkd | GG 385 | 2" | Martin / Cosgrove | 20 01 84 | Focus Plate North | CTIO | |||
3241 | -65 00 | 10s | lla - O bkd | GG 385 | 2" | Martin / Cosgrove | 20 01 84 | Focus Plate South | CTIO | |||
3242 | 14 44 40.8 | -65 27 13 | 25m | lla - O bkd | GG 385 | 2" | Martin / Cosgrove | 20 01 84 | Test Plate | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
July 1984 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3243 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 19 07 84 | 0.6 - 5.5 | Broken Ok" | CTIO | |
3244 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 1.5" - 5" | Blanco / Ugarte | 19 07 84 | 0.0 - 5.8 | |||
3245 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 2" - 4" | Blanco / Ugarte | 19 07 84 | 0.6 - 5.5 | CTIO | ||
3246 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 2" - 4" | Blanco / Ugarte | 19 07 84 | 0.0 - 5.8 | |||
3247 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 20 07 84 | 0.6 - 5.5 | CTIO | ||
3248 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 20 07 84 | 0.0 - 5.8 | |||
3249 | 18 05 45 | -31 10 18 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 20 07 84 | 0.6 - 5.5 | CTIO | ||
3250 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 20 07 84 | 0.0 - 5.8 | |||
3251 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 20 07 84 | 0.6 - 5.5 | CTIO | ||
3252 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 20 07 84 | 0.0 - 5.8 | |||
3253 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 20 07 84 | 0.6 - 5.5 | CTIO | ||
3254 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 20 07 84 | 0.0 - 5.8 | |||
3255 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 20 07 84 | 0.6 - 5.5 | CTIO | ||
3256 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 20 07 84 | 0.0 - 5.8 | |||
3257 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 1.5" | Blanco / Ugarte | 20 07 84 | 0.6 - 5.5 | CTIO | ||
3258 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 1.5" | Blanco / Ugarte | 20 07 84 | 0.0 - 5.8 | |||
3259 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 1.5" | Blanco / Ugarte | 20 07 84 | 0.6 - 5.5 | CTIO | ||
3260 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 1.5" | Blanco / Ugarte | 20 07 84 | 0.0 - 5.8 | |||
3261 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 1.5" | Blanco / Ugarte | 20 07 84 | 0.6 - 5.5 | CTIO | ||
3262 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 1.5" | Blanco / Ugarte | 20 07 84 | 0.0 - 5.8 |
Last Updated on 8/27/99
By Guerra & Marin
August 1984 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3263 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 01 08 84 | 0.6 - 5.5 | CTIO | ||
3264 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 01 08 84 | 0.0 - 5.8 | |||
3265 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 01 08 84 | 0.6 - 5.5 | CTIO | ||
3266 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 01 08 84 | 0.0 - 5.8 | |||
3267 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 01 08 84 | 0.6 - 5.5 | CTIO | ||
3268 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 01 08 84 | 0.0 - 5.8 | |||
3269 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 01 08 84 | 0.6 - 5.5 | CTIO | ||
3270 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 01 08 84 | #REF! | |||
3271 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 01 08 84 | 0.6 - 5.5 | CTIO | ||
3272 | 18 06 47 | -32 09 14 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 01 08 84 | 0.0 - 5.8 | |||
3273 | 18 05 45 | -31 10 08 | 20m | 103a - O | GG 385 | 3" - 4" | Blanco / Ugarte | 01 08 84 | 0.6 - 5.5 | CTIO | ||
3274 | 18 05 45 | -31 10 08 | 30m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 02 08 84 | 0.6 - 5.5 | CTIO | ||
3275 | 18 06 47 | -32 09 14 | 30m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 02 08 84 | 0.0 - 5.8 | |||
3276 | 17 59 04.6 | -46 50 04 | 20m | 103a - O | GG 385 | 2" - 3" | Blanco / Ugarte | 02 08 84 | comet Neujmin | |||
3277 | 18 05 45 | -31 10 08 | 30m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 02 08 84 | 0.6 - 5.5 | CTIO | ||
3278 | 18 06 47 | -32 09 14 | 30m | 103a - O | GG 385 | 1" - 5" | Blanco / Ugarte | 02 08 84 | 0.0 - 5.8 | |||
3279 | 18 05 45 | -31 10 08 | 30m | 103a - O | GG 385 | 2" - 5" | Blanco / Ugarte | 02 08 84 | 0.6 - 5.5 | CTIO | ||
3280 | 17 59 04.6 | -46 50 04 | 15m | 103a - O | GG 385 | 1" - 2" | Blanco / Ugarte | 02 08 84 | comet Neujmin | |||
3281 | 18 05 45 | -31 10 08 | 30m | 103a - O | GG 385 | 2" | Blanco / Ugarte | 02 08 84 | 0.6 - 5.5 | CTIO | ||
3282 | 18 06 47 | -32 08 14 | 10m | 103a - O | GG 385 | Blanco / Ugarte | 02 08 84 | 0.0 - 5.5 |
Last Updated on 8/27/99
By Jorge Marin
September 1984 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3283 | 16 31 27 | -44 52 44 | 30m | 103a - O | GG 495 | Graham / Klemola / Bravo | 21 09 84 | HH - 57 | ||||
3284 | 17 09 25.6 | -23 18 35 | 30m | 103a - O | GG 495 | Graham / Klemola / Bravo | 21 09 84 | Ophiuchus | ||||
3285 | 19 00 41 | -36 59 06 | 30m | 103a - O | GG 385 | Graham / Klemola / Bravo | 21 09 84 | R Cr A | ||||
3286 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | Graham / Klemola / Bravo | 21 09 84 | NGC 121 | ||||
3287 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | Graham / Klemola / Bravo | 21 09 84 | NGC 121 | ||||
3288 | 00 24 27 | -71 48 24 | 60m | 103a - O | GG 385 | Graham / Klemola / Bravo | 21 09 84 | NGC 121 | ||||
3289 | 00 24 27 | -71 48 24 | 3m | 103a - O | GG 385 | Graham / Klemola / Bravo | 21 09 84 | NGC 121 | ||||
3290 | 17 09 25.6 | -23 18 35 | 30m | 103a - O | GG 385 | 1" | Graham / Klemola / Rivera | 22 09 84 | Ophiuchus | |||
3291 | 19 00 41 | -36 59 06 | 30m | 103a - O | GG 385 | 1" | Graham / Klemola / Rivera | 22 09 84 | R Cr A | |||
3292 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | 2" | Graham / Klemola / Rivera | 22 09 84 | NGC 121 | |||
3293 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | 1" - 2" | Graham / Klemola / Rivera | 22 09 84 | NGC 121 | |||
3294 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | 1" | Graham / Klemola / Rivera | 22 09 84 | NGC 121 | |||
3295 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | 1" | Graham / Klemola / Rivera | 22 09 84 | NGC 121 | |||
3296 | 17 09 25.3 | -23 18 49 | 30m | 103a - D | GG 495 | 2" | Graham / Klemola / Rivera | 23 09 84 | Ophiuchus | |||
3297 | 19 00 41 | -36 59 06 | 40m | 103a - O | GG 385 | 1.5" | Graham / Klemola / Rivera | 23 09 84 | R Cr A | |||
3298 | 17 09 25.6 | -23 18 35 | 45m | 103a - O | UG 1 | 1" - 2" | Graham / Klemola / Rivera | 24 09 84 | Ophiuchus | |||
3299 | 19 00 41 | -36 59 06 | 30m | 103a - O | GG 385 | 1.5" | Graham / Klemola / Rivera | 24 09 84 | R Cr A | |||
3300 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | 1" - 2" | Graham / Klemola / Rivera | 24 09 84 | NGC 121 | |||
3301 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | 1" - 4" | Graham / Klemola / Rivera | 24 09 84 | NGC 121 | |||
3302 | 00 24 27 | -71 48 24 | 90m | 103a - O | GG 385 | 2" - 3" | Graham / Klemola / Rivera | 24 09 84 | NGC 121 | |||
3303 | 00 24 27 | -71 48 24 | 72m | 103a - O | GG 385 | 2" - 3" | Graham / Klemola / Rivera | 24 09 84 | NGC 121 |
Last Updated on 8/27/99
By Guerra & Marin
December 1984 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3304 | llla - F | GG 385 | 1.5" | Bass / Hernandez | 19 12 84 | focus | ||||||
3305 | 04 19 35.2 | -54 58 09 | 155m | llla - J | GG 385 | 1.5" - 2" | Bass / Hernandez | 19 12 84 | NGC 1566 |
Last Updated on 8/27/99
By Jorge Marin
1985 Plate logs for 1.5-m telescope
May 1985 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3306 | 17 29 51 | -37 21 47 | 10s each | lla - O bkd | GG 385 | Blanco / Elicer / R.Gonzalez | 24 05 85 | focus | ||||
3307 | 18 08 06 | -31 10 20 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.5 | CTIO | ||
3308 | 18 08 57 | -32 07 37 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.8 | |||
3309 | 18 08 07.7 | -31 10 18 | 25m | lla - O bkd | GG 495 | 2" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.5 | CTIO | ||
3310 | 18 08 58.1 | -32 07 34 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.8 | |||
3311 | 18 08 08 | -31 10 13 | 25m | lla - O bkd | GG 385 | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.5 | CTIO | |||
3312 | 18 08 58 | -32 07 34 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.8 | |||
3313 | 18 08 09 | -31 10 14 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.5 | CTIO | ||
3313 | 18 08 09 | -31 10 14 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.5 | |||
3314 | 18 08 51.7 | -32 07 32 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.8 | |||
3315 | 18 08 09 | -31 10 14 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.5 | CTIO | ||
3316 | 18 08 59 | -32 07 32 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.8 | |||
3317 | 18 08 10 | -31 10 15 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.5 | CTIO | ||
3318 | 18 08 59 | -32 07 32 | 25m | lla - O bkd | GG 385 | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.8 | ||||
3319 | 18 08 10 | -31 10 15 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer / R.Gonzalez | 24 05 85 | 0.6 - 5.5 | CTIO | ||
3320 | 18 08 59 | -32 07 32 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.8 | |||
3321 | 18 08 10 | -31 10 15 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.5 | CTIO | ||
3322 | 18 08 57.5 | -32 06 49 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.8 | |||
3323 | 18 08 10 | -31 10 15 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.5 | CTIO | ||
3324 | 18 08 58.2 | -32 06 46 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.8 | |||
3325 | 18 08 10 | -31 10 15 | 25m | lla - O bkd | GG 385 | seeing variable | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.5 | CTIO | ||
3326 | 18 08 58.2 | -32 06 46 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.8 | |||
3327 | 18 08 10 | -31 10 15 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.5 | CTIO | ||
3328 | 18 08 58 | -32 06 40 | 25m | lla - O bkd | GG 385 | 1" | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.8 | |||
3329 | 18 08 10 | -31 10 15 | 25m | lla - O bkd | GG 385 | 1" - 2" | Blanco / Elicer / R.Gonzalez | 26 05 85 | 0.6 - 5.5 | CTIO | ||
3330 | 18 09 00 | -32 06 40 | 25m | lla - O bkd | GG 385 | seeing variable | Blanco / Elicer / R.Gonzalez | 25 05 85 | 0.6 - 5.8 | |||
3331 | 18 08 10.7 | -31 10 13 | 25m | lla - O bkd | GG 385 | 2" - 4" | Blanco / Elicer | 26 05 85 | 0.6 - 5.5 | |||
3332 | 18 08 58.8 | -32 07 35 | 25m | lla - O bkd | GG 385 | 2" - 4" | Blanco / Elicer | 26 05 85 | 0.6 - 5.8 | |||
3333 | 18 08 10.7 | -31 10 13 | 25m | lla - O bkd | GG 385 | 2" - 4" | Blanco / Elicer | 26 05 85 | 0.6 - 5.5 | CTIO | ||
3334 | 18 08 58.5 | -32 07 35 | 25m | lla - O bkd | GG 385 | 2" - 3" | Blanco / Elicer | 26 05 85 | 0.6 - 5.8 | |||
3335 | 18 08 11 | -31 10 10 | 25m | lla - O bkd | GG 385 | 2" - 3" | Blanco / Elicer | 26 05 85 | 0.6 - 5.5 | CTIO | ||
3336 | 18 08 59 | -32 07 29 | 25m | lla - O bkd | GG 385 | 2" - 3" | Blanco / Elicer | 26 05 85 | 0.6 - 5.8 | |||
3337 | 18 08 11 | -31 10 09 | 25m | lla - O bkd | GG 385 | 2" - 3" | Blanco / Elicer | 26 05 85 | 0.6 - 5.5 | CTIO | ||
3338 | 18 09 00 | -32 07 30 | 25m | lla - O bkd | GG 385 | 1" - 1.5" | Blanco / Elicer | 26 05 85 | 0.6 - 5.8 | |||
3339 | 18 08 12 | -31 10 07 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer | 26 05 85 | 0.6 - 5.5 | CTIO | ||
3340 | 18 08 59 | -32 07 31 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer | 26 05 85 | 0.6 - 5.8 | |||
3341 | 18 08 10 | -31 10 07 | 25m | lla - O bkd | GG 385 | 2.5" | Blanco / Elicer | 26 05 85 | 0.6 - 5.5 | CTIO | ||
3342 | 18 08 58 | -32 07 48 | 25m | lla - O bkd | GG 385 | 2" - 4" | Blanco / Elicer | 26 05 85 | 0.6 - 5.8 | |||
3343 | 18 08 10 | -31 10 07 | 25m | lla - O bkd | GG 385 | 2" - 4" | Blanco / Elicer | 27 05 85 | 0.6 - 5.5 | CTIO | ||
3344 | 18 08 58 | -32 07 48 | 25m | lla - O bkd | GG 385 | 1" - 2" | Blanco / Elicer | 27 05 85 | 0.6 - 5.8 | |||
3345 | 18 08 10 | -31 10 07 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer | 27 05 85 | 0.6 - 5.5 | |||
3346 | 18 08 58 | -32 07 48 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer | 27 05 85 | 0.6 - 5.8 | |||
3347 | 18 08 10 | -31 10 07 | 25m | lla - O bkd | GG 385 | 2" | Blanco / Elicer | 27 05 85 | 0.6 - 5.5 | CTIO | ||
3348 | 18 08 58 | -32 07 48 | 25m | lla - O bkd | GG 385 | 1" | Blanco / Elicer | 27 05 85 | 0.6 - 5.8 | |||
3349 | 18 08 10 | -31 10 07 | 25m | lla - O bkd | GG 385 | 1" | Blanco / Elicer | 27 05 85 | 0.6 - 5.5 | CTIO | ||
3350 | 18 08 58 | -32 07 48 | 25m | lla - O bkd | GG 385 | 1" | Blanco / Elicer | 27 05 85 | 0.6 - 5.8 | |||
3351 | 18 08 10 | -31 10 07 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer | 27 05 85 | 0.6 - 5.5 | CTIO | ||
3352 | 18 08 58 | -32 07 48 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer | 27 05 85 | 0.6 - 5.8 | |||
3353 | 18 08 10 | -31 10 07 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer | 27 05 85 | 0.6 - 5.5 | CTIO | ||
3354 | 18 08 58 | -32 07 48 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer | 27 05 85 | 0.6 - 5.8 | |||
3355 | 18 08 10 | -31 10 07 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer | 27 05 85 | 0.6 - 5.5 | CTIO | ||
3356 | 18 08 58 | -32 07 48 | 25m | lla - O bkd | GG 385 | 1.5" | Blanco / Elicer | 27 05 85 | 0.6 - 5.8 |
Last Updated on 8/27/99
By Guerra & Marin
August 1985 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3357 | 12 24 57.8 | -39 03 43 | 120m | lla - O bkd | GG 385 | Jarvis / Cosgrove | 10 08 85 | IC 3370 | ||||
3358 | 18 58 48 | -64 58 06 | 120m | lla - O bkd | GG 385 | 3" - 4" | Jarvis / Cosgrove | 10 08 85 | NGC 6722 | |||
3359 | 19 14 14 | -60 38 12 | 120m | lla - O bkd | GG 495 | 4" - 5" | Jarvis / Cosgrove | 10 08 85 | NGC 6771 | |||
3360 | 21 59 50.3 | -32 14 04 | 150m | lla - D | GG 495 | Jarvis / Cosgrove | 10 08 85 | 466 - 946 | ||||
3361 | 18 05 45.2 | -31 10 05 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field l | CTIO | |||
3362 | 18 06 47 | -32 09 14 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field ll | ||||
3363 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field lll | CTIO | |||
3364 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field ll | CTIO | |||
3365 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field ll | ||||
3366 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field lll | CTIO | |||
3367 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field l | CTIO | |||
3368 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field ll | ||||
3369 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 11 08 85 | Field lll | CTIO | |||
3370 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 4" | Blanco / Cosgrove | 11 08 85 | Field l | CTIO | |||
3371 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 4" | Blanco / Cosgrove | 11 08 85 | Field ll | ||||
3372 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" | Blanco / Cosgrove | 12 08 85 | Field l | CTIO | |||
3373 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" | Blanco / Cosgrove | 12 08 85 | Field ll | ||||
3374 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" | Blanco / Cosgrove | 12 08 85 | Field lll | CTIO | |||
3375 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" | Blanco / Cosgrove | 12 08 85 | Field l | CTIO | |||
3376 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 12 08 85 | Field ll | ||||
3377 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 12 08 85 | Field lll | CTIO | |||
3378 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 12 08 85 | Field l | CTIO | |||
3379 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 12 08 85 | Field ll | ||||
3380 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 12 08 85 | Field lll | CTIO | |||
3381 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 12 08 85 | Field l | CTIO | |||
3382 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 1" - 3" | Blanco / Cosgrove | 12 08 85 | Field ll | ||||
3383 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 2" - 3" | Blanco / Cosgrove | 12 08 85 | Field ll | ||||
3384 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 2" - 4" | Blanco / Cosgrove | 12 08 85 | Field l | CTIO | |||
3385 | 18 10 24 | -29 33 | lla - O bkd | GG 385 | 2" - 4" | Blanco / Cosgrove | 12 08 85 | Field ll | ||||
3386 | 18 05 45.2 | -31 10 05 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 13 08 85 | Field l | CTIO | |||
3387 | 18 06 47 | -32 09 14 | 20m | lla - O bkd | Blanco / Cosgrove | 13 08 85 | Field ll | |||||
3388 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 13 08 85 | Field lll | CTIO | |||
3389 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 13 08 85 | Field l | CTIO | |||
3390 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | Blanco / Cosgrove | 13 08 85 | Field ll | |||||
3391 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 13 08 85 | Field lll | CTIO | |||
3392 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 13 08 85 | Field l | CTIO | |||
3393 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | Blanco / Cosgrove | 13 08 85 | Field ll | |||||
3394 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 13 08 85 | Field l | CTIO | |||
3395 | 18 10 24 | -29 33 01 | 20m30s | lla - O bkd | Blanco / Cosgrove | 13 08 85 | Field ll | |||||
3396 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 13 08 85 | Field l | CTIO | |||
3397 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | Blanco / Cosgrove | 13 08 85 | Field ll | |||||
3398 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 14 08 85 | Field l | CTIO | |||
3399 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 14 08 85 | Field lll | CTIO | |||
3400 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 15 08 85 | Field l | CTIO | |||
3401 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | Blanco / Cosgrove | 15 08 85 | Field ll | |||||
3402 | 18 10 24 | -29 33 01 | 20m04s | lla - O bkd | GG 385 | Blanco / Cosgrove | 15 08 85 | Field lll | CTIO | |||
3403 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 15 08 85 | Field l | CTIO | |||
3404 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | Blanco / Cosgrove | 15 08 85 | Field ll | |||||
3405 | 18 10 24 | -29 33 01 | 3m | lla - O bkd | GG 385 | Blanco / Cosgrove | 15 08 85 | Field lll | CTIO | |||
3406 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 15 08 85 | Field lll | CTIO | |||
3407 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 15 08 85 | Field l | CTIO | |||
3408 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | Blanco / Cosgrove | 15 08 85 | Field ll | |||||
3409 | 18 10 24 | -29 33 01 | 20m | lla - D bkd | GG 395 | Blanco / Cosgrove | 15 08 85 | Field l | CTIO | |||
3410 | 18 10 24 | -29 33 01 | 20m | lla - D bkd | GG 395 | Blanco / Cosgrove | 15 08 85 | Field ll | CTIO | |||
3411 | 18 10 24 | -29 33 01 | 20m | lla - D bkd | GG 395 | Blanco / Cosgrove | 15 08 85 | Field lll | CTIO | |||
3412 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 15 08 85 | Field l | CTIO | |||
3413 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | Blanco / Cosgrove | 15 08 85 | Field ll | ||||
3414 | 18 10 24 | -29 33 01 | 20m | lla - O bkd | GG 385 | 1.5" | Blanco / Cosgrove | 15 08 85 | Field lll | CTIO | ||
3415 | 18 05 45.5 | -31 10 07 | 20m | lla -- O | GG 385 | 2" - 3" | Blanco / Ugarte | 16 08 85 | Field l | CTIO | ||
3416 | 18 06 47 | -32 09 14 | 20m | lla -- O | GG 385 | 2" - 3" | Blanco / Ugarte | 16 08 85 | Field ll | |||
3417 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 2" - 3" | Blanco / Ugarte | 16 08 85 | Field lll | CTIO | ||
3418 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 2" - 3" | Blanco / Ugarte | 16 08 85 | Field l | CTIO | ||
3419 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 2" - 3" | Blanco / Ugarte | 16 08 85 | Field ll | |||
3420 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" | Blanco / Ugarte | 16 08 85 | Field lll | CTIO | ||
3421 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" | Blanco / Ugarte | 16 08 85 | Field l | CTIO | ||
3422 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" - 2" | Blanco / Ugarte | 16 08 85 | Field ll | |||
3423 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" - 2" | Blanco / Ugarte | 16 08 85 | Field lll | CTIO | ||
3424 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 2" - 4" | Blanco / Ugarte | 16 08 85 | Field l | CTIO | ||
3425 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" - 2" | Blanco / Ugarte | 16 08 85 | Field lll | CTIO | ||
3426 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" - 2" | Blanco / Ugarte | 16 08 85 | Field lll | |||
3427 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" - 2" | Blanco / Ugarte | 16 08 85 | Field l | CTIO | ||
3428 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" - 2" | Blanco / Ugarte | 16 08 85 | Field ll | |||
3429 | 18 10 24 | -29 33 01 | 20m | lla -- O | GG 385 | 1" - 2" | Blanco / Ugarte | 16 08 85 | Field ll | CTIO | ||
3430 | 18 10 24 | -29 33 01 | 15m | lla - D | GG 395 | 1" - 2" | Blanco / Ugarte | 16 08 85 | Field lll | CTIO | ||
3431 | 18 10 24 | -29 33 01 | 15m | lla - D | GG 395 | 3" | Blanco / Ugarte | 16 08 85 | Field l | CTIO | ||
3432 | 18 10 24 | -29 33 01 | 15m | lla - D | GG 395 | 3" | Blanco / Ugarte | 16 08 85 | Field ll | CTIO |
Last Updated on 8/27/99
By Jorge Marin
1986 Plate logs for 1.5-m telescope
May 1986 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3433 | 18 10 24 | -29 33 02 | 25m | lla - O bkd | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field lll | CTIO | ||
3434 | 18 06 47 | -32 09 14 | 25m | lla - O | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field ll | |||
3435 | 18 10 24 | -29 33 01 | 25m | lla - O bkd | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field lll | CTIO | ||
3436 | 18 05 36.8 | -31 10 49 | 25m | lla - O bkd | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field l | CTIO | ||
3437 | 18 05 36.8 | -31 10 49 | 25m | lla - O bkd | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field lll | CTIO | ||
3438 | 18 05 36.8 | -31 10 49 | 25m | lla - O | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field ll | |||
3439 | 18 05 36.8 | -31 10 49 | 25m | lla - O bkd | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field lll | CTIO | ||
3440 | 18 05 36.8 | -31 10 49 | 25m | lla - O bkd | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field l | CTIO | ||
3441 | 18 05 36.8 | -31 10 49 | 25m | lla - O bkd | GG 385 | 1.4" | Blanco / Hernandez | 31 05 86 | Field lll | CTIO | ||
3442 | 18 05 36.8 | -31 10 49 | 25m | lla - D bkd | GG 395 | 1.4" | Blanco / Hernandez | 31 05 86 | Field lll | CTIO | ||
3443 | 18 06 45 | -32 09 14 | 25m | lla - D bkd | GG 395 | 1" - 3" | Blanco / Hernandez | 31 05 86 | Field ll | CTIO | ||
3444 | 18 06 45 | -32 09 14 | 25m | lla - O bkd | GG 385 | 1" - 3" | Blanco / Hernandez | 31 05 86 | Field lll | CTIO | ||
3445 | 18 06 45 | -32 09 14 | 25m | lla - D bkd | GG 395 | 1" - 3" | Blanco / Hernandez | 31 05 86 | Field l | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
June 1986 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3446 | 18:10:31.2 | -29 33 57 | 25m | lla - O bkd | GG 385 | 2" - 3" | Blanco / Hernandez | 01 06 86 | Field lll | CTIO | ||
3447 | 18 06 53 | -32 10 15 | 25m | lla - O | GG 385 | 2" - 3" | Blanco / Hernandez | 01 06 86 | Field ll | |||
3448 | 18 05 47.2 | -31 11 56 | 25m | lla - O bkd | GG 385 | 2" - 3" | Blanco / Hernandez | 01 06 86 | Field l | CTIO | ||
3449 | 18 10 32 | -29 33 53 | 25m | lla - O bkd | GG 385 | 2" - 3" | Blanco / Hernandez | 01 06 86 | Field lll | CTIO | ||
3450 | 18 10 32 | -29 33 53 | 25m | lla - O | GG 385 | 2" - 3" | Blanco / Hernandez | 01 06 86 | Field ll | |||
3451 | 18 10 32 | -29 33 53 | 25m | lla - O | GG 385 | 2" - 3" | Blanco / Hernandez | 01 06 86 | Field lll | CTIO | ||
3452 | 18 10 32 | -29 33 53 | 25m | lla - O | GG 385 | 2" - 3" | Blanco / Hernandez | 01 06 86 | Field l | CTIO | ||
3453 | 18 10 32 | -29 33 53 | 25m | lla - O | GG 385 | 2" - 3" | Blanco / Hernandez | 01 06 86 | Field lll | CTIO | ||
3454 | 18 10 32 | -29 33 53 | 25m | lla - D | GG 495 | 1" - 2" | Blanco / Hernandez | 01 06 86 | Field ll | |||
3455 | 18 10 32 | -29 33 53 | 25m | lla - D | GG 395 | 1" - 2" | Blanco / Hernandez | 01 06 86 | Field lll | CTIO | ||
3456 | 18 10 32 | -29 33 53 | 25m | lla - D | GG 395 | 1" - 2" | Blanco / Hernandez | 01 06 86 | Field l | CTIO | ||
3457 | 18 10 32 | -29 33 53 | 25m | lla - O | GG 385 | 1" - 2" | Blanco / Hernandez | 01 06 86 | Field lll | CTIO | ||
3458 | 18 10 32 | -29 33 53 | 25m | lla - O | GG 385 | 1" - 2" | Blanco / Hernandez | 01 06 86 | Field l | |||
3459 | 18 05 47.6 | -31 12 01 | 25m | lla - O bkd | GG 385 | 1.5" - 2" | Blanco / Hernandez | 02 06 86 | Field l | CTIO | ||
3460 | 18 05 47.6 | -31 12 01 | 25m | lla - O bkd | GG 385 | 1.5" - 2" | Blanco / Hernandez | 02 06 86 | Field lll | CTIO | ||
3461 | 18 05 47.6 | -31 12 01 | 25m | lla - O | GG 385 | 1.5" - 2" | Blanco / Hernandez | 02 06 86 | Field ll | |||
3462 | 18 05 47.6 | -31 12 01 | 25m | lla - O bkd | GG 385 | 1.5" - 2" | Blanco / Hernandez | 02 06 86 | Field lll | CTIO | ||
3463 | 18 24 11 | -33 54 58 | 30m | IV N | RG 2 | 1.5" | Blanco / Hernandez | 02 06 86 | M Dwarf | |||
3464 | 18 08 36 | -31 47 00 | 25m | lV N bkd | RG 610 | 1" - 1.5" | Blanco / Hernandez | 02 06 86 | NGC 6558 | CTIO | ||
3465 | 18 08 36 | -31 47 00 | 25m | lV N bkd | RG 610 | 1" - 1.5" | Blanco / Hernandez | 02 06 86 | Field ll | CTIO | ||
3466 | 18 08 36 | -31 47 00 | 25m | lla - O bkd | GG 385 | 1" - 1.5" | Blanco / Hernandez | 02 06 86 | Field lll | CTIO | ||
3467 | 18 08 36 | -31 47 00 | 25m | lla - O bkd | GG 385 | 1" - 1.5" | Blanco / Hernandez | 02 06 86 | Field l | CTIO | ||
3468 | 18 08 36 | -31 47 00 | 25m | lla - O bkd | GG 385 | 1" - 1.5" | Blanco / Hernandez | 02 06 86 | Field lll | CTIO | ||
3469 | 18 08 36 | -31 47 00 | 25m | lla - O | GG 385 | 1.5" - 2" | Blanco / Hernandez | 02 06 86 | Field ll | |||
3470 | 18 08 36 | -31 47 00 | 25m | lla - O bkd | GG 385 | 1.5" - 2" | Blanco / Hernandez | 02 06 86 | Field lll | CTIO | ||
3471 | 18 08 36 | -31 47 00 | 25m | lla - O bkd | GG 385 | 1.5" - 2" | Blanco / Hernandez | 02 06 86 | Field l | CTIO | ||
3472 | 18 08 36 | -31 47 00 | 25m | lla - O bkd | GG 385 | 2" - 3" | Blanco / Hernandez | 02 06 86 | Field ll | CTIO | ||
3473 | 18 08 36 | -31 47 00 | 25m | lla - O | GG 385 | 2" - 3" | Blanco / Hernandez | 02 06 86 | Field ll |
Last Updated on 8/27/99
By Guerra & Marin
December 1986 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3474 | 01 02 22.3 | -71 26 25 | 60m | 103a - O | 2" | Baird / Bravo | 06 12 86 | SMC Field 0102 - 71.5 | ||||
3475 | 01 02 22.3 | -71 26 25 | 60m | HD3L9 batch | 2" | Baird / Bravo | 06 12 86 | SMC Field 0102 - 71.5 | ||||
3476 | 06 30 15.5 | -64 18 29 | 10m | lla - O baked | GG 385 | 1" | Suntzeff - Bravo | 06 12 86 | NGC 2257 | |||
3477 | 06 30 14.9 | -64 19 03 | 47m | lla - O baked | GG 385 | 1" | Suntzeff - Bravo | 06 12 86 | NGC 2257 | |||
3478 | 01 02 19.1 | -71 26 37 | 70m | 103a - D | GG 495 | 1" | Baird / Bravo | 07 12 86 | SMC Field 0102 - 71.5 | |||
3479 | 01 02 19.1 | -71 26 37 | 70m | 103a - D HDIKI batch | GG 495 | 1" | Baird / Bravo | 07 12 86 | SMC Field 0102 - 71.5 | |||
3480 | 01 02 19.1 | -71 26 37 | 70m | 103a - D | GG 495 | 1" | Baird / Bravo | 07 12 86 | SMC Field 0102 - 71.5 | |||
3481 | 06 29 58.7 | -64 17 50 | 90m | lla - O baked | GG 385 | 2" | Suntzeff - Bravo | 07 12 86 | NGC 2257 | |||
3482 | 06 29 58.7 | -64 17 50 | 40m | lla - O bkd | GG 385 | 2" | Suntzeff - Bravo | 07 12 86 | NGC 2257 | CTIO | ||
3483 | 01 02 17 | -71 26 24 | 60m | 103a - D | GG 495 | 2" | Baird / Bravo | 08 12 86 | SMC Field 0102 - 71.5 | |||
3484 | 01 02 17 | -71 26 24 | 60m | 103a - D HDIKI batch | GG 495 | 2" | Baird / Bravo | 08 12 86 | SMC Field 0102 - 71.5 | |||
3485 | 06 29 56.6 | -64 17 54 | 90m | lla - O baked | GG 385 | 1" | Suntzeff - Bravo | 08 12 86 | NGC 2257 | |||
3486 | 06 29 56.6 | -64 17 54 | 90m | lla - O baked | GG 385 | 2" | Suntzeff - Bravo | 08 12 86 | NGC 2257 | |||
3487 | 01 02 19.3 | -71 26 27 | 90m | lla - D bkd | GG 495 | 1.5" | Baird / Bravo | 09 12 86 | SMC Field 0102 - 71.5 | |||
3488 | 01 02 19.3 | -71 26 27 | 75m | lla - D IH4 batch | GG 495 | 1" | Baird / Bravo | 09 12 86 | SMC Field 0102 - 71.5 | |||
3489 | 06 29 59.7 | -64 17 46 | 90m | lla - O baked | GG 385 | 1.5" | Suntzeff - Bravo | 09 12 86 | NGC 2257 | |||
3490 | 06 29 59.7 | -64 17 46 | 90m | lla - O baked | GG 385 | 1.5" | Suntzeff - Bravo | 09 12 86 | NGC 2257 | |||
3491 | 01 02 20.9 | 71 26 29 | 70m | lla - D bkd | GG 495 | 2" | Baird / Bravo | 10 12 86 | SMC Field 0102 - 71.5 | |||
3492 | 01 02 20.9 | 71 26 29 | 60m | lla - D bkd | GG 495 | Baird / Bravo | 10 12 86 | SMC Field 0102 - 71.5 | ||||
3493 | 01 02 20.9 | 71 26 29 | 45m | 103a - O | Baird / Bravo | 10 12 86 | SMC Field 0102 - 71.5 | |||||
3494 | 05 13 27.4 | -65 28 21 | 5m | lla - D bkd | GG 495 | Baird / Bravo | 10 12 86 | LMC NGC 1866 | ||||
3495 | 05 13 27.4 | -65 28 21 | 15m | lla - D bkd | GG 495 | 2" | Baird / Bravo | 10 12 86 | LMC NGC 1866 | |||
3496 | 05 13 27.4 | -65 28 21 | 45m | lla - D bkd | GG 495 | 2" | Baird / Bravo | 10 12 86 | LMC NGC 1866 | |||
3497 | 01 02 19.5 | -71 26 25 | 60m | 103a - O / HD3L9 | 2.5" | Baird / Bravo | 11 12 86 | SMC Field 0102 - 71.5 | ||||
3498 | 01 02 19.5 | -71 26 25 | 60m | 103a - O / HD3L9 | 3" | Baird / Bravo | 11 12 86 | SMC Field 0102 - 71.5 | ||||
3499 | 01 02 19.5 | -71 26 25 | 60m | lla - D bkd | GG 495 | 1.5" | Baird / Bravo | 11 12 86 | SMC Field 0102 - 71.5 | |||
3500 | 05 13 28 | -65 28 27 | 45m | 103a - O | 2" | Baird / Bravo | 11 12 86 | LMC NGC 1866 | ||||
3501 | 05 13 28 | -65 28 27 | 15m | 103a - O | 2" | Baird / Bravo | 11 12 86 | LMC NGC 1866 | ||||
3502 | 05 13 28 | -65 28 27 | 5m | 103a - O | 1" | Baird / Bravo | 11 12 86 | LMC NGC 1866 | ||||
3503 | 02 36 18 | -30 03 | 13*20s | 103a - D | Blanco / Gonzalez / Ugarte | 23 12 86 | focus | |||||
3504 | 05 22 00 | -34 57 | Blanco / Gonzalez / Ugarte | 23 12 86 | focus | |||||||
3505 | 02 08 33 | -30 50 20 | 15*20s | Weller / Ugarte | 24 12 86 | focus | ||||||
3506 | 03 00 45 | -30 50 20 | 0.5m | Weller / Ugarte | 24 12 86 | out of focus images | ||||||
3507 | 05 25 00 | -35 29 | 5m | Weller / Ugarte / Saá | 24 12 86 | Hartnann plate | ||||||
3508 | Weller / Ugarte / Saá | 24 12 86 | Hartnann plate | |||||||||
3509 | Weller / Ugarte / Saá | 24 12 86 | out of focus zenith | |||||||||
3510 | Weller / Ugarte / Saá | 24 12 86 | out of focus zenith | |||||||||
3511 | 20s | Weller / Ugarte / Saá | 24 12 86 | out of focus zenith | ||||||||
3512 | Weller / Ugarte / Saá | 24 12 86 | Hartnann zenith | |||||||||
3513 | Weller / Saá / Bravo | 24 12 86 | Focus plate | |||||||||
3514 | Weller / Saá / Bravo | 24 12 86 | Focus plate | |||||||||
3515 | Weller / Saá / Bravo | 24 12 86 | focus plate way out of focus |
Last Updated on 8/27/99
By Jorge Marin
1987 Plate logs for 1.5-m telescope
February 1987 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3516 | 10s | Weller / Saá / Tirado | 11 02 87 | focus plate | ||||||||
3517 | 10s | Weller / Saá / Tirado | 11 02 87 | focus plate | ||||||||
3518 | 15s | Weller / Saá / Tirado | 12 02 87 | focus plate | ||||||||
3519 | 15s | Weller / Saá / Tirado | 12 02 87 | focus plate | ||||||||
3520 | 15s | Weller / Saá / Tirado | 12 02 87 | focus plate | ||||||||
3521 | 15s | Weller / Saá / Tirado | 12 02 87 | focus plate | ||||||||
3522 | 10s | Weller / Saá / Tirado | 12 02 87 | focus plate | ||||||||
3523 | 10s | Weller / Saá / Tirado | 13 02 87 | focus plate | ||||||||
3524 | 10s | Weller / Saá / Tirado | 13 02 87 | focus plate | ||||||||
3525 | 10s | Weller / Saá / Tirado | 13 02 87 | focus plate | ||||||||
3526 | 10s | Weller / Saá / Tirado | 13 02 87 | focus plate | ||||||||
3527 | zenith | 10s | Weller / Saá / Tirado | 13 02 87 | focus plate | |||||||
3528 | zenith | 10s | Weller / Saá / Tirado | 13 02 87 | focus plate | |||||||
3529 | zenith | 10s | Weller / Saá / Tirado | 13 02 87 | focus plate | |||||||
3530 | zenith | 15s | Weller / Saá / Tirado | 13 02 87 | focus plate | |||||||
3531 | zenith | 10s | Weller / Saá / Tirado | 13 02 87 | focus plate | |||||||
3532 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3533 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3534 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3535 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3536 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3537 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3538 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3539 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3540 | zenith | 60s | Weller / Gonzalez / Tirado | 14 02 87 | test exposure | |||||||
3541 | zenith | 10s | Weller / Gonzalez / Tirado | 14 02 87 | focus plate | |||||||
3542 | zenith | 60s | Weller / Gonzalez / Tirado | 14 02 87 | test exposure | |||||||
3543 | zenith | 10s each | Weller / Gonzalez / Tirado | 14 02 87 | focus exposure | |||||||
3544 | zenith | 60s | Weller / Gonzalez / Tirado | 14 02 87 | test exposure | |||||||
3545 | zenith | 60s | Weller / Gonzalez / Tirado | 14 02 87 | test exposure |
Last Updated on 8/27/99
By Guerra & Marin
March 1987 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3546 | 05 35 50 | -69 18 00 | 60s | lV N | RG 610 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3547 | 05 35 50 | -69 18 00 | 60s | lV N | RG 610 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3548 | 05 35 50 | -69 18 00 | 60s | lV N | RG 610 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3549 | 05 35 50 | -69 18 00 | 60s | lV N | RG 610 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3550 | 05 35 50 | -69 18 00 | 2m | lV N | RG 610 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3551 | 05 35 50 | -69 18 00 | 2m | lV N | RG 610 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3552 | 05 35 50 | -69 18 00 | 30s | lV N | RG 610 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3553 | 05 35 50 | -69 18 00 | 30s | lV N | RG 610 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3554 | 05 35 50 | -69 18 00 | 20s | lla - O | GG 385 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3555 | 05 35 50 | -69 18 00 | 20s | lla - O | GG 385 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | CTIO | |||
3556 | 05 35 50 | -69 18 00 | 30m | lla - O | GG 495 | Blanco / Cosgrove | 08 03 87 | Super Nova 1987-1 | Broken Ok" | CTIO | ||
3557 | zenith | lla - O | Blanco / Cosgrove | 08 03 87 | focus plate | |||||||
3558 | zenith | lla - O | Blanco / Cosgrove | 08 03 87 | focus plate | |||||||
3559 | 06 16 38 | -32 24 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3560 | 06 16 38 | -32 24 | 7m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3561 | 08 14 50 | -33 02 | 7m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3562 | 08 14 50 | -33 02 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3563 | 09 22 20 | -35 58 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3564 | 09 22 20 | -35 58 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3565 | 10 20 04 | -31 06 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3566 | 10 57 20 | -30 52 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3567 | 10 57 20 | -30 52 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3568 | 12 43 07 | -33 55 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3569 | 12 43 07 | -33 55 | 20s each | 103a - D | Weller / Saá / Ugarte | 17 03 87 | focus plate | |||||
3570 | 13 28 30 | -33 00 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | Optic test | |||||
3571 | 15 06 24 | -31 00 | 5m | 103a - D | Weller / Saá / Ugarte | 17 03 87 | test | |||||
3572 | 06 39 40 | -26 19 30 | 3m | 103a - D | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3573 | 06 39 40 | -26 19 30 | 3m | 103a - D | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3574 | 06 39 40 | -26 19 30 | 3m | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3575 | 11 03 33 | -31 44 20 | 5m | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3576 | 11 02 09 | -59 23 | 3m | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3577 | 11 02 09 | -59 23 | 3m | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3578 | 11 02 09 | -59 23 | 3m | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3579 | 15 59 13 | -26 22 00 | 1m40s | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3580 | 12 23 15 | -60 13 00 | 3m | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3581 | 12 23 15 | -60 13 00 | 3m | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3582 | 12 23 15 | -60 13 00 | 3m | 103a - O | Weller / Saá / Ugarte | 18 03 87 | Optic test | |||||
3583 | 06 21 35 | -33 24 37 | 3m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3584 | 07 31 00.2 | -29 10 01 | 5m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3585 | 08 16 33 | -29 16 46 | 3m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3586 | 09 23 04 | -28 58 18 | 3m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3587 | 10 06 38.9 | -28 45 07 | 3m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3588 | 10 29 00 | -29 33 04 | 3m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3589 | 11 20 57 | -29 30 23 | 3m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3590 | 11 34 34 | -29 56 24 | 3m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3591 | 12 58 24.7 | -29 53 06 | 3m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3592 | 14 03 51 | -28 57 29 | 2m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3593 | 14 26 30 | -30 01 32 | 15s each | lla - O | Weller / Saá / Hernandez | 20 03 87 | focus plate | |||||
3594 | 14 03 52 | -28 57 11 | 2m | lla - O | Weller / Saá / Hernandez | 20 03 87 | Optic test | |||||
3595 | 16 40 18 | -48 44 00 | 2m | lla - O | Weller / Saá / Hernandez | 20 03 87 | N 6193 |
Last Updated on 8/27/99
By Guerra & Marin
April 1987 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3596 | 07 23 30 | -29 16 42 | 3m | lla - O | Blanco / Bravo / Saá | 02 04 87 | eta Canis major | |||||
3597 | 07 23 30 | -29 16 42 | 5*1m | lla - O | Blanco / Bravo / Saá | 02 04 87 | eta Canis major | |||||
3598 | 07 23 30 | -29 16 42 | 5*15s | lla - O | Blanco / Bravo / Saá | 02 04 87 | eta Canis major | |||||
3599 | 07 23 30 | -29 16 42 | 9*15s | lla - O | Blanco / Bravo / Saá | 02 04 87 | eta Canis major | |||||
3600 | 07 23 30 | -29 16 42 | 9*15s | lla - O | Blanco / Bravo / Saá | 02 04 87 | eta Canis major | |||||
3601 | 07 23 30 | -29 16 42 | 9*15s | lla - O | Blanco / Bravo / Saá | 02 04 87 | eta Canis major | |||||
3602 | 07 23 30 | -29 16 42 | 9*15s | lla - O | Blanco / Bravo / Saá | 02 04 87 | eta Canis major | |||||
3603 | 11 04 43 | -30 06 20 | lla - O | 1" -2" | Blanco / Bravo / Saá | 02 04 87 | focus | |||||
3604 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1.5" | Blanco / Bravo | 02 04 87 | Window l | CTIO | ||
3605 | 18 05 45 | -31 10 08 | 20m | lla - D | GG 495 | 1.5" | Blanco / Bravo | 02 04 87 | Window l | CTIO | ||
3606 | 18 10 24 | -29 33 01 | 20m | lla - D | GG 495 | 1.5" | Blanco / Bravo | 02 04 87 | Window lll | CTIO | ||
3607 | 18 10 24 | -29 33 01 | 20m | lla - O | GG 385 | 1.5" | Blanco / Bravo | 02 04 87 | Window lll | CTIO | ||
3608 | 18 06 47 | -32 09 14 | 20m | lla - O | 1.5" | Blanco / Bravo | 02 04 87 | Window ll | ||||
3609 | 18 06 47 | -32 09 14 | 20m | lla - D | 1" | Blanco / Bravo | 02 04 87 | Window ll | ||||
3610 | 05 38 44.3 | -69 05 59 | 20m | 103a - O | GG 385 | 1" | Blanco / Hernandez | 03 04 87 | 30 Dor. + S. N. 1987 | CTIO | ||
3611 | 05 38 44.3 | -69 05 59 | 20m | 103a - O | GG 385 | 1" | Blanco / Hernandez | 03 04 87 | 30 Dor. + S. N. 1987 | CTIO | ||
3612 | 08 48 10 | -30 10 15 | 103a - O | GG 385 | Blanco / Hernandez | 03 04 87 | Focus plate | CTIO | ||||
3613 | 08 48 10 | -30 10 15 | 103a - O | Blanco / Hernandez | 03 04 87 | focus |
Last Updated on 8/27/99
By Jorge Marin
May 1987 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3614 | 18 10 24 | -29 33 01 | 25m | lla - O | GG 385 | 3" | Blanco / M.Fernandez | 20 05 87 | Field lll | CTIO | ||
3615 | 18 06 47 | -32 09 14 | 25m | lla - O | GG 385 | Blanco / M.Fernandez | 20 05 87 | Field ll | ||||
3616 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1.5" | Blanco / M.Fernandez | 20 05 87 | Field l | CTIO | ||
3617 | 18 05 45 | -31 10 08 | 20m | lla - D | GG 495 | 1.5" | Blanco / M.Fernandez | 20 05 87 | Field lll | CTIO | ||
3618 | 18 05 45 | -31 10 08 | 20m | lla - D | GG 495 | 2" - 3" | Blanco / M.Fernandez | 20 05 87 | Field ll | |||
3619 | 18 05 45 | -31 10 08 | 20m | lla - D | GG 495 | 2" - 3" | Blanco / M.Fernandez | 20 05 87 | Field l | CTIO | ||
3620 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | Blanco / M.Fernandez | 20 05 87 | Field lll | CTIO | |||
3621 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | Blanco / M.Fernandez | 20 05 87 | Field lll | CTIO | |||
3622 | 18 05 45 | -31 10 08 | 58m | lV - N sens | RG 610 | Blanco / M.Fernandez | 21 05 87 | Field lll | CTIO | |||
3623 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1" - 2" | Blanco / M.Fernandez | 21 05 87 | Field lll | CTIO | ||
3624 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1" - 2" | Blanco / M.Fernandez | 21 05 87 | Field l | CTIO | ||
3625 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1" - 2" | Blanco / M.Fernandez | 21 05 87 | Field lll | CTIO | ||
3626 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1" - 2" | Blanco / M.Fernandez | 21 05 87 | Field ll | |||
3627 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1" - 2" | Blanco / M.Fernandez | 21 05 87 | Field lll | CTIO | ||
3628 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1" - 2" | Blanco / M.Fernandez | 21 05 87 | Field l | CTIO | ||
3629 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 1" - 2" | Blanco / M.Fernandez | 21 05 87 | Field lll | CTIO | ||
3630 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 2" | Blanco / M.Fernandez | 21 05 87 | Field ll | |||
3631 | 18 05 45 | -31 10 08 | 20m | lla - O | GG 385 | 2" - 3" | Blanco / M.Fernandez | 21 05 87 | Field lll | CTIO | ||
3632 | 18 10 24 | -29 33 01 | 20m | lla - D | GG 495 | 3" - 4" | Blanco / Bravo | 22 05 87 | Field lll | CTIO | ||
3633 | 18 10 24 | -29 33 01 | 20m | lla - O | GG 385 | 2" | Blanco / Bravo | 22 05 87 | Field lll | CTIO | ||
3634 | 18 10 24 | -29 33 01 | 20m | lla - D | GG 495 | 2" | Blanco / Bravo | 22 05 87 | Field lll | CTIO | ||
3635 | 18 10 24 | -29 33 01 | 20m | lla - O | GG 385 | 3" - 6" | Blanco / Bravo | 22 05 87 | Field lll | CTIO | ||
3636 | 18 10 24 | -29 33 01 | 20m | lla - O | GG 385 | Blanco / Bravo | 22 05 87 | Field lll | CTIO |
Last Updated on 8/27/99
By Guerra & Marin
December 1987 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3637 | 00 26 08 | -71 44 20 | 80m | lla - O | GG 385 | 1" - 2" | Graham / M.Fernandez | 12 12 87 | NGC 721 | |||
3638 | 06 30 12 | -64 17 30 | 70m | lla - O | GG 385 | 1" | Graham / M.Fernandez | 12 12 87 | NGC 2257 | |||
3639 | 00 26 08 | -71 44 20 | 75m | lla - O | GG 385 | 1" | Graham / M.Fernandez | 13 12 87 | NGC 121 | |||
3640 | 06 30 12 | -64 17 30 | 60m | lla - O | GG 385 | 1" | Graham / M.Fernandez | 13 12 87 | NGC 2257 | |||
3641 | 06 30 12 | -64 17 30 | 80m | lla - O | GG 385 | 1" | Graham / M.Fernandez | 13 12 87 | NGC 2257 | |||
3642 | 08 25 00 | -51 00 04 | 135m | llla - F | RG 610 | 1" | Graham / M.Fernandez | 13 12 87 | 4446 | |||
3643 | 00 26 08 | -71 44 20 | 75m | lla - O | GG 385 | 1" - 2" | Graham / M.Fernandez | 14 12 87 | NGC 121 | |||
3644 | 06 30 12 | -64 09 00 | 60m | lla - O | GG 385 | 2" - 3" | Graham / M.Fernandez | 14 12 87 | NGC 2257 | |||
3645 | 06 30 12 | -64 09 00 | 90m | lla - O | GG 385 | 1" - 2" | Graham / M.Fernandez | 14 12 87 | NGC 2257 | |||
3646 | 06 30 12 | -64 09 00 | 130m | llla - F | RG 610 | 1" - 2" | Graham / M.Fernandez | 14 12 87 | NGC 2257 | |||
3647 | 00 26 08 | -71 44 20 | 75m | lla - O | GG 385 | 1" | Graham / M.Fernandez | 15 12 87 | NGC 121 | |||
3648 | 06 30 12 | -64 17 30 | 60m | lla - O | GG 385 | 1" | Graham / M.Fernandez | 15 12 87 | NGC 2257 | |||
3649 | 06 30 12 | -64 17 30 | 75m | lla - O | GG 385 | 1" | Graham / M.Fernandez | 15 12 87 | NGC 2257 | |||
3650 | 06 30 12 | -64 17 30 | 75m | lla - O | GG 385 | 1" - 2" | Graham / M.Fernandez | 15 12 87 | NGC 2257 | |||
3651 | 00 26 08 | -71 44 20 | 90m | lla - O | GG 385 | 1" - 2" | Graham / M.Fernandez | 16 12 87 | NGC 121 | |||
3652 | 06 30 12 | -64 17 30 | 90m | lla - O | GG 385 | 2" | Graham / M.Fernandez | 16 12 87 | NGC 2257 | |||
3653 | 06 30 12 | -64 17 30 | 90m | lla - O | GG 385 | Graham / M.Fernandez | 16 12 87 | NGC 2257 | ||||
3654 | 05 35 31.5 | -69 16 27 | 1s 5s | UG 2 | Graham / M.Fernandez | 16 12 87 | SN 1987 | |||||
3655 | 05 35 31.5 | -69 16 27 | 60m | RG 2 | Graham / M.Fernandez | 16 12 87 | SN 1987 | |||||
3656 | (1) | 19 12 88 |
(1) NOTE: secondary f 7.5 comes back from Tucson, after refiguring
Last Updated on 8/27/99
By Jorge Marin
1989 Plate logs for 1.5-m telescope
March 1989 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3657 | zenith | 10s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | focus | ||||||
3658 | 06 42 45 | -45 11 24 | 300s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | E 3 | |||||
3659 | 06 42 45 | -45 11 24 | 1800s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | E 3 | |||||
3660 | zenith | 10s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | focus | ||||||
3661 | 08 07 33 | -34 43 20 | 5m | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | field | |||||
3662 | zenith | 10s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | focus | ||||||
3663 | 08 29 19 | -47 04 56 | 5m | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | field E 4 | |||||
3664 | 08 29 19 | -47 04 56 | 1800s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | field E 4 | |||||
3665 | zenith | 10s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | focus | ||||||
3666 | 11 10 03 | -46 42 40 | 5m | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | field E 5 | |||||
3667 | zenith | 10s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | focus | ||||||
3668 | 11 10 28 | -46 52 44 | 5m | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | field E 5 | |||||
3669 | 11 10 28 | -46 52 44 | 1800s | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | field E 5 | |||||
3670 | 11 10 28 | -46 52 44 | 10m | lla - D | Gonzalez / Saá / Tirado | 10 03 89 | field E 5 |
Last Updated on 8/27/99
By Guerra & Marin
June 1989 Plate logs for 1.5-m telescope
July 1989 Plate logs for 1.5-m telescope
Plate | N. N. | R. A. | Dec | Exp. Time | Emulsion | Filtro | Seeing | Observer | Date | Object | Remarks | CTIO |
3696 | 17 14 42 | -48 03 | 30m | 098 - 04 | RG 1 | 1" | Terndrup / Ugarte | 04 07 89 | Field #2 | |||
3697 | 17 41 30 | -40 40 | 30m | 098 - 04 | RG 1 | Terndrup / Ugarte | 04 07 89 | Field #4 | ||||
3698 | 17 45 24 | -39 25 | 30m | 098 - 04 | RG 1 | Terndrup / Ugarte | 04 07 89 | Field #5 | ||||
3699 | 17 58 12 | -35 00 | 30m | 098 - 04 | RG 1 | Terndrup / Ugarte | 04 07 89 | Field #7 | ||||
3700 | 17 59 00 | -34 50 | 30m | 098 - 04 | RG 1 | Terndrup / Ugarte | 04 07 89 | Field #8 | ||||
3701 | 17 51 30 | -37 33 | 30m | 098 - 04 | RG 1 | Terndrup / Ugarte | 04 07 89 | Field #6 | ||||
3702 | 18 03 00 | -33 30 | 30m | 098 - 04 | RG 1 | Terndrup / Ugarte | 04 07 89 | Field #10 | ||||
3703 | 18 48 36 | -13 22 | 30m | 098 - 04 | RG 1 | Terndrup / Ugarte | 04 07 89 | Field #20 | clear, valley fogged in | |||
3704 | 18 21 24 | -24 54 | 10m | lla - O baked | GG 385 | Terndrup / Ugarte | 04 07 89 | M 28 | ||||
3705 | 18 21 24 | -24 54 | 10m | lla - O baked | GG 385 | Terndrup / Ugarte | 04 07 89 | M 28 | ||||
3706 | 18 54 54 | -10 28 | 30m | 098 - 04 | RG 1 | Terndrup / Ugarte | 04 07 89 | Field #21 |
Last Updated on 8/27/99
By Guerra & Marin
1990 Plate logs for 1.5-m telescope
August 1990 Plate logs for 1.5-m telescope
The SMARTS Consortium operates four small telescopes (1.5-m [112], 1.3-m [72], 1.0-m [113] and 0.9-m [114]) on Cerro Tololo. Membership in SMARTS is open to individuals or institutions, including international partners.
Inquiries from potential new members of SMARTS at a variety of levels are always encouraged, as opportunities to join the consortium typically arise every year. Members can purchase time on the SMARTS telescopes at very reasonable rates for single use observing runs that span a few days or weeks, or for distributed observing over one or more semesters for time-domain science. Both user and service modes are available within the capabilities of the four SMARTS telescopes. Acceptance of a new member depends on the balance of resources and scientific programs associated with current members.
Current rates for SMARTS are $600 USD / night for the 0.9m (Classical user observing mode only) and $200 USD / hour [NOTE: this is per scheduled hour, not executed hour, and includes overheads from telescope pointing and exposure time] for the 1.3m and 1.5m (queue-scheduled service observing mode only).
Primary Members who contribute $25K USD or more are entitled to a seat on the SMARTS Management Council. Those who contribute less than $25K are considered Secondary Members and do not participate in the governance of SMARTS.
If you are interested in joining SMARTS, please contact Victoria Misenti [115] for more information.
AURA CONTRACT No. C77006A
SMARTS 2 AGREEMENT TO OPERATE SMALL TELESCOPES IN CHILE
Appendix D
Association of Universities for Research in Astronomy
Dr. William Smith, President
1200 New York Avenue NW
Suite 350
Washington DC, 20005
(202) 483-2101
wsmith@aura-astronomy.org [122]
Clark Enterline
Procurement Manager
NOAO
950 N. Cherry Avenue
PO Box 26732
Tucson, AZ 85726-6732
(520) 318-8277
centerline@noao.edu [123]
NOAO
SMARTS Program
R. Chris Smith
NOAO/CTIO
Casilla 603, La Serena, Chile
(56-51) 205200
csmith@noao.edu [124]
Charles Bailyn
Yale University, Department of Astronomy
PO Box 208101
New Haven, CT 06520-8101
(203) 432-3000
charles.bailyn@yale.edu [125]
Adopted by the SMARTS management council.
Amended by the SMARTS management council February 1, 2008 (to take effect as of October 1, 2007).
NOAO contact amended July 2011 due to change in personnel.
Proposal information
G. Schumacher
D. Geisler
Feb. 1991
some updates by A.R. Walker, Sept. 1998
Photo-electric Photometry is only offered on the 1.5-m telescope, at f/13/5 (10 arcsec/mm). Unfortunately, there is at present no CTIO staff member carrying out scientific programs with this equipment, and so we may be a little slow at finding the answers to your questions. Sorry!
We have several photomultiplier tubes (GaAs, S20, S11) normally operating in a dry-ice cooled cold-box. We also have the last working Varian InGaAsP photomultiplier in the world (purchased in 1978!!) which has high sensitivity to almost 1.2 microns, we restrict access to this tube due to its fragility and uniqueness. The photometers are simple devices containing an aperture wheel, filter wheel, and TV viewing of the aperture, all under computer control. The pulses from the photomultipliers are amplified by either SSR or EMI amplifier- discriminators and then counted on hardware contained in a PC, which also operates the instrument, and has various facilities for displaying the data, manipulating and storing it, and doing reductions. The remainder of this document describes the program. Note that this PC is on the mountain ethernet, so you can transfer your data files home with ease, or else write them to floppy disk.
The files utilized by the PC-ASCAP program are ordinary text files consisting of one line records, which can be produced using any text editor which does not leave any special control character in the file. The records themselves consists of various fields separated by any number of spaces. Free format number decoding is used throughout. Therefore, it is important not to use a space within a field, for example in a star identification. We recommend using the "_" (underbar) or "-" (dash) characters instead.
User file.
This file is mandatory and contains the basic information for observation. We recommend calling it by your name, e.g. Jastronomer. The examples illustrate a typical set-up: using the 1.5m telescope with the Hamamatsu tube in cold box 71 and the filters VBURI in positions 1-5. The following record types are used in this file:
Name: this record identifies the observer. For example:
Name: Joe Astronomer
Telescope: this record identifies the telescope. The telescopes with encoders are the 4.0m, 1.5m, 1.0m, and 0.9m. Any other name is accepted, e.g. 0.6m, but the position information is then taken from the right ascension and declination of the object, as given with the 'ident' command (see below), instead of from the telescope encoders. For example:
Telescope: 1.5m
Tube: this record identifies the photomultiplier in use. The last field in the record contains the maximum recommended count rate for the tube.
Tube: Hamamatsu 71 200000
In order to prevent damage to the phototube, there is a maximum recommended count rate for each tube that should not be exceeded. In general, this maximum count rate is 200,000 counts/sec. This is true of all of the GaAs tubes (RCA, Hamamatsu) - see page IV-28 of the Facilities Manual for the maximum recommended count rate if you are using a different tube. If the count exceeds the number given in the user file in the first second of observation, the program will insert the TV mirror, warn you that you have exceeded the maximum count rate and ask if you wish to continue. To be safe, answer "NO" and observe a fainter star. You can force the integration to continue by typing "YES" but PLEASE be careful as excessive exposure to extreme light levels can fry the tube. If you must observe this star, use the minimum integration time necessary.
Dead time: this record gives the dead time in nanoseconds, needed to correct for coincidence losses.
Dead time: 35
Filters: this record initiates the description of the filters in use. The description consists of the filter position in the filter wheel, an identification label and optional comments. The identification label should start with an alphabetic character, not a number.
Filters:
Precision: this record initiates the declaration of the precision value for each filter. You can omit this item if you are not using the automatic mode.
Precision:
Color equations: this record initiates the description of the color equations to be used in the quick look calculations. The equations are constructed utilizing the labels given in the filters record. You can omit this and following items if quick look is not desired.
Color equations:
U-B = 1.01*u - 1.01*b
B-V = 0.95*b - 0.95*v
V-R = 0.96*v - 0.96*r
R-I = 0.99*r - 0.99*i
V = 1.03*v - 0.03*b
NB - The order of these equations should be the same as that in the Standard file (see below).
Extinction coefficients: this record initiates the definition of the extinction coefficients.
Extinction coefficients:
v = 0.14
b = 0.23 - 0.024*b + 0.024*v
u = 0.50 - 0.024*b + 0.024*v
r = 0.085
i = 0.052 + 0.01*r - 0.01*i
Zero points: this record initiates the definition of zero point values.
Zero points:
U-B = 0.21
B-V = -0.38
V-R = -0.29
R-I = 1.20
V = 21.61
The next example shows a complete user file.
Name: Joe Astronomer
Telescope: 1.5m
Tube: Hamamatsu 71 200000
Dead time: 35
Filters:
Precision:
Color equations:
U-B = 1.01*u - 1.01*b
B-V = 0.95*b - 0.95*v
V-R = 0.96*v - 0.96*r
R-I = 0.99*r - 0.99*i
V = 1.03*v - 0.03*b
Extinction coefficients:
v = 0.14
b = 0.23 - 0.024*b + 0.024*v
u = 0.50 - 0.024*b + 0.024*v
r = 0.085
i = 0.052 + 0.01*r - 0.01*i
Zero points:
U-B = 0.21
B-V = -0.38
V-R = -0.29
R-I = 1.20
V = 21.61
Macros file
The macros file contains the definitions of the automated observing sequences. The macros have the same format as the old Tolnet version. In order to distinguish one macro from another they are separated by a record containing the word 'macro' followed by a number. This number is then used to invoke the macro with the 'X' command. The macro may be extended to several lines and can have an unlimited number of commands. The file must be called ' macros '. The number of macros is also unlimited (unlike the old version where there were only 10 available). Within a macro, the format is : * (star) or / (sky), followed by filter number, then a comma, followed by the desired number of observations, then a space, and another 4-character command. For example:
macro 1
*1,1 *2,1 *3,1 *4,1 *5,1
/5,1 /4,1 /3,1 /2,1 /1,1
macro 2
*1,2 *2,2 *3,2 *4,2 *5,2 /5,1 /4,1 /3,1 /2,1 /1,1
After observing the star and before observing sky, the program will halt, move the TV mirror to the field position, and wait until you locate a sky patch and press the space key before observing sky.
Objects file
The objects file contains the positions of the objects to be observed. Remember that spaces are used to separate fields and should not be used within a field.
Within the data records, the following order is used:
- Record Identifier: The exact content of this record is up to the user. This identifier should be given with the 'ident' command. It can be up to 8 characters.
- right ascension: 3 numbers: HH MM SS.SS, e.g. 12 34 45.123
- declination: 3 numbers: DD MM SS.SS, e.g. -30 41 32.3
- epoch: a number in years., e.g. 1990.0
The rest of the line may be used for comments, identifiers, etc. PC-ASCAP does not use this information.
The following is an example of an object file:
1 17 05 05.431 -64 59 56.12 2000.0 Center of field
2 17 03 32 -65 00 53 1950 V= 18.24, B-V= 0.35
Standard file
This file contains the star id, standard magnitude and the color values for the standard stars. The order of the indices should be the same as that given in the user file. Also, the star id should be identical to that used in the objects file and
Star U-B B-V V-R R-I V E101 0.091 0.087 0.038 0.084 7.704 E102 0.112 0.206 0.126 0.274 8.444 E103 0.098 0.086 0.037 0.085 9.657 E104 0.001 0.362 0.213 0.427 7.455
Data file
The data file is called 'ppdata.dat'. The data is normally written to the hard disk but you can also select the floppy drive as a backup medium. The format of the data is the same card image format as the old version of People's Photometry, so you don't have to change your reduction program! At the end of the night, you can write out your data to floppy using the command PPCOPY. For example:
PPCOPY ppdata.dat a:dec2590.dat
The format of the data is:
Column(s) Contents 1 0 if normal data record or 1 if a comment, in which case the comment appears in columns 6-80. 2-5 Record number. 6-13 Identification. 14 Standard flag: 1 if the star identification appears in your standard star (stand) file, 0 otherwise. 15 Object flag: 0 if star, 1 if sky. 16 Diaphram number (first diafram used =1, second =2, etc.). 17 Filter number. 20-21 Universal time hours. 22-23 Universal time minutes. 24-25 Universal time seconds. 26-28 Hour angle hours. 29-30 Hour angle minutes. 31-32 Hour angle seconds. 33-35 Declination degrees. 36-37 Declination minutes. 38-39 Declination seconds. 40 Reject flag: blank if not rejected, 1 if rejected. 41 Number of channels (=1). 42-45 Integration time (sec). 46-52 Counts. 67-68 Month. 69-70 Day. 71-72 Year. 73-74 Universal time tenths of seconds.
The $ level commands are those which accept parameters needed during data acquisition and logging. The commands are case insensitive and all responses require pressing the 'enter' key to be acted upon. A list of the available commands at any level appears on a window on the right-hand side of the screen. Following is a description of all implemented commands.
This command sets the clock to the Universal Time as given by the satellite receiver. In order to use this feature you need to be connected to the SUN computer named ctio1m (from the Sun, do "rlogin ctio1m"). Operation is as follows:
- Type the goes command at the PC terminal.
- Then type the goes command at the SUN terminal.
- On the PC screen you will see a time about 10 seconds ahead of the present time. When that time arrives the clock will be synchronized with the satellite time. There are ocassions when this command fails to terminate and the clock doesn't get synchronized at the shown time. In that case, strike any key at the PC terminal and repeat the operation again.
This command enables or disables backup of the data on a diskette. To enable backup type 'backup on'. To disable type 'backup off'. The backup status is permanently shown in the status window. For example:
backup on
It is a good idea to enable this feature, which will then cause the data to be written to floppy ~ every 10 records, naming the file something like a:dec2590.bck. However, since you may reject records during the night after they are written, you may also want to write the clean data to floppy at the end of the night using the PPCOPY feature (after you quit the program), naming the file a:dec2590.dat.
This command shows the present telescope coordinates on the screen. If printer logging is enabled they get typed on that medium too. The coordinates are presented in the order right ascension, declination and hour angle.
This command permits setting of the date. If no argument is given then the present date is shown on the screen. The format is month/day/year. For example:
date 09/18/90
With this command you give the program the size of the diafram (in mm) to be used. After given the command, the program positions the selected aperture inmediately. The acceptable arguments are: 0.7, 1.0, 1.4, 2.0, 2.8, 4.0, 5.6. See the Facilities Manual (Table IV-17) to determine the size of the apertures in arcseconds at your telescope. For example:
diaf 1.4
This command permits examining a directory content. After you type the command, you are requested for the name of the directory to be shown. To return to the command level, just press 'ESC'.
This command permits editing of a file content. If the file doesn't exist it is created. Otherwise the file content is presented in an edit panel.
The editor is a true screen editor (not a word processor) in that you use the arrows and pages keys to browse and insert text. To exit the editor press the ESC key. The following keys are supported:
ESC Quit editing DEL Delete character under cursor BACKSPACE Delete character to the left of cursor ALT-S Search for a string ALT-R Search for a string and replace it UP Moves the cursor up one character DOWN Moves the cursor down one character RIGHT Moves the cursor right one character LEFT Moves the cursor left one character HOME Moves to beginning of the current line END Moves to the end of the current line PGUP Moves up one page PGDN Moves down one page CTRL-PGUP Goes to the beginning of the text CTRL-PGDN Goes to the end of the text ALT-M Turns marking mode on or off. GRAY + Copies the marked block to the cut buffer. GRAY - Cuts the marked block to the cut buffer. INS Pastes the cut buffer at the current cursor location. DEL Deletes the marked block if there is one.
For example:
edit jastronomer
-Note. Be sure to use the "eq" command after editing your userfile to update the changes into the program, e.g. after changing the zero points at the beginning of the night.
This command is used to enter the limit of acceptable variability for the counts, C, according to:
|C - Mean| / Sigma < Eps.
If any count rate exceeds this criterion, integration will halt and an "Unstdy Counts" error message will appear. Check centering, etc. To continue, just press the space key. Be sure to reject the offending integration if appropriate.
To suppress this feature enter a value of 0. For example:
eps 10
This command permits rereading the equations for quick look contained in the user file. Normally you give this command after editing the user file, for example, after changing the zeropoints at the beginning of the night.
This command transfers control to the section of the program where data acquisition actually occurs. The runtime window is placed on the screen. For example:
go
The GO level commands for actual data acquisition are virtually identical to the old People's Photometry commands. They are largely single key instructions requiring no 'enter' key to perform its action. However, 'enter' must still be used with those commands requiring parameters, such as setting an integration time. Following is a list of GO level commands.
space continue integration after hold condition. 1-8 starts integration with selected filter. * group observations as star counts. / group observations as sky counts. - group observations as dark counts. ! force termination of present integration, and continue to next command if executing a macro. a selects automatic mode. (Integration terminates when the precision defined in the Precision Table is reached). b breaks integration or escapes from macro. Data is not recorded for the interrupted integration. c XXX enters the comment XXX (up to 72 characters). f shows the field on the TV screen. h holds an integration. Continue by striking the space bar. k kills the previous sky readings. m selects manual mode. n NN sets the number of integrations to NN per filter. r n-m sets the reject flag on records n-m. s stop and return to $ level commands. t n sets the integration time to n seconds. Allowed values are 1 to 30,000. v view the area of the diafram on the TV screen. x n starts macro n. z zap (terminate) present macro command. Can reinitiate present macro command with the Space bar.
This command transfers control to the section of the program where data acquisition actually occurs. The difference with the go command is that no data recording takes place.
This command is used to identify an object using up to 8 characters. The command groups the observations belonging to one object together, and failure to use it negates internal housekeeping functions. After receiving the command, the program checks the standard file to see if the object is a standard star or not. If it is, the program tells you so.
For telescopes lacking position encoders, or when the connection is disabled (see tcs command below) and if the id is not found in the objects file, then the program will ask for the coordinates of the object. The coordinates are requested in a formatted window. In order to escape from the window just press 'ESC'. For example:
i LMC-0635
This command allows editting of the macros file. After the command is given the file content is presented in an edit window (see edit command above). For example:
macros
This command selects the objects file. The file should be prepared according to the description given in the 'files' section. For example:
object obs24.coo
This command is used to change the precision values of any filter. After given the command you are presented with a window of precision values. To return to the command level press 'ESC'.
This command enables or disables logging of commands on the printer. To enable logging type 'printer on'. To disable logging type 'printer off'.
This command requests the calculation of quick look reductions. If no argument is given then the last object observed is used. Otherwise, the argument is taken as the first record number of the object to be calculated. For example:
q 274
This command terminates the program. After receiving the command, the program requests the user for confirmation. Respond 'yes' if you want to abandon the program. Use this command to terminate the program at the end of the night. If you quit the program during the night for whatever reason and then return, be sure to execute the "stand" command and set "backup" and "printer" on.
This command selects the standard stars file. The file should be prepared according to the description given in the 'files' section. Be sure to use this command again if, for whatever reason, you "Quit" the program and then return to it during the night. For example:
stand ubvrimag
This command enables or disables the connection to the telescope control system. Type 'tcs on' to enable. Type 'tcs off' to disable. For example:
tcs on
This command permits setting of the universal time into the computer. If no argument is given then the present time is shown on the screen. The format is hh:mm:ss. For example:
time 06:35:40
Figure 1 shows the run-time data display. It consists of a series of windows each showing specific pieces of information. Following is a description of each window.
Top left
This window displays the program name.
Top right
This window displays the date and universal time.
Middle left
This window displays the actual run-time information. Under 'object' it shows both '*' and '/', for star and sky respectively. Under 'filter' it shows the number of the actual filter being observed. Under 'time' it shows the total time of integration in seconds. Under 'counts/sec' it shows the rate for the present object being observed. Under 'counts' it shows the total counts already obtained for both star and sky for the selected filter. Under 'prec' it shows the present presicion obtained (in units of 0.1%), and finally under 'total (* - /)' is shown the total star counts minus the sky counts (=(Star count rate - Sky count rate)(both corrected for dead time) * ( total time observed on Star )). Thus, e.g., when this number reaches 10,000 you have achieved 1% accuracy from photon statistics.
Middle right
This window shows the status of the backup, printer and tcs options.
Bottom left
This is the actual command window.
Bottom right
This is the help window, where all possible commands available in the current task are shown. The window content changes as you select different levels of the program.
A full photometry reduction program is available on the SUN computers, both on the mountain and in La Serena, enabling you to obtain final transformed magnitudes and colors for program stars. After a little practice, one can reduce a night's worth of data in about an hour.
G. Schumacher
D. Geisler
Feb. 1991
Fiber echelle consists of the de-comissioned Blanco Echelle spectrograph [137] in fixed configuration connected by optical fiber to the CTIO 1.5-m telescope. The instrument was used in service mode in 2008-2010.
Spectral format: Fixed configuration covering wavelength range from 4010 to 7300 Angstroem without gaps. The order height is about 3 pixels FWHM.
Spectral resolution:
Efficiency: Estimated 1%. The star V=5 gives about 135 electrons/s in the extracted spectrum (standard slit setting 50 micron). Assuming 5-pixel height of the extracted spectrum and normal readout mode, the signal-to-noise ratio S/N near blaze maximum for exposure time t seconds and a star of magnitude V can be estimated as
S/N = Nph/sqrt(Nph + 18^2), Nph = 1.35 t 10^(-0.4V + 4)
See the plot below. Exposures longer than 20 min. are not recommended because of cosmic rays; take several exposures instead.
Detector: SITe, 2048x2048 pixels, 24-micron pixel size. Full readout in 27s (normal mode, gain 0.9 el/ADU) or 18s (fast mode, gain 3 el/ADU). Readout noise 8el (normal) and 9.5el (fast). Saturation level: 65536 counts in all modes (to be confirmed).
Comparison lamps: Thorium-Argon, Quartz (not simultaneous, light goes through the same fiber). Do not forget to take comparison exposures needed for your program!
Precise radial velocities: Iodine cell can be inserted in the beam before slit for precise radial-velolcity measurements. On bright stars, the precision can reach 3 m/s.
Entrance aperture: round, diameter 2.7 arcseconds.
Guiding: automatic, using light of the observed star falling outside entrance aperture.
Documentation: user's manual [138]
Time synchronization on the CTIO computers is done as follows:
Jim Hughes (jhughesATnoao.edu)
Current Schedules
Links
[1] http://www.astro.yale.edu/smarts/1.3m.html
[2] http://www.astro.yale.edu/smarts/ANDICAM/data.html
[3] http://www.astronomy.ohio-state.edu/ANDICAM/detectors.html
[4] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/kpno_b.pdf
[5] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/KPNO_B.txt
[6] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/kpno_v.pdf
[7] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/KPNO_V.txt
[8] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/kpno_i.pdf
[9] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/KPNO_I.txt
[10] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/andi_j.pdf
[11] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/J_andi.txt
[12] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/andi_h.pdf
[13] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/H_andi.txt
[14] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/andi_k.pdf
[15] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/K_andi.txt
[16] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/yalo_b.pdf
[17] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/B_YALO.txt
[18] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/yalo_r.pdf
[19] http://www.ctio.noao.edu/noao/sites/default/files/instruments/filters/R_YALO.txt
[20] http://www.astro.yale.edu/smarts/ANDICAM/mail.html
[21] http://www.astro.yale.edu/smarts/smarts13m/observer.html
[22] http://www.astro.yale.edu/smarts/smarts13m/optprocessing.html
[23] http://www.astro.yale.edu/smarts/ANDICAM/ObsLogs/
[24] http://www.astro.yale.edu/smarts/ANDICAM/Reports/Nightly/
[25] http://www.astro.yale.edu/smarts/smarts13m/procreps.html
[26] http://www.ctio.noao.edu/noao/content/13-m-photometric-standards
[27] http://www.astro.yale.edu/smarts/smarts13m/pg1323.html
[28] http://www.astro.yale.edu/smarts/smarts13m/ndfilters.html
[29] http://www.astro.yale.edu/smarts/smarts13m/queue.html
[30] http://www.astro.yale.edu/smarts/usage/usage13m2004b.dat
[31] http://www.astro.yale.edu/smarts/usage/usage13m2005a.dat
[32] http://www.astro.yale.edu/smarts/usage/usage13m2005b.dat
[33] http://www.astro.yale.edu/smarts/usage/usage13m2006a.dat
[34] http://www.astro.yale.edu/smarts/usage/usage13m2006b.dat
[35] http://www.ctio.noao.edu/noao/content/optical-processing-procedure
[36] http://www.astro.yale.edu/smarts/ANDICAM/Reports/Trouble/
[37] http://www.astro.yale.edu/smarts/ANDICAM/Reports/
[38] http://www.ctio.noao.edu/noao/content/SMARTS-Logs
[39] http://www.astronomy.ohio-state.edu/ANDICAM/detectors.html#sens
[40] http://www.ctio.noao.edu/noao/content/13-m-telescope
[41] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele13/optprocessing.txt
[42] http://www.ctio.noao.edu/noao/content/smarts-contacts
[43] http://www.astro.yale.edu/smarts/smarts13m/photrepsCCD.html
[44] http://www.astro.yale.edu/smarts/smarts13m/photrepsIR.html
[45] http://www.astro.yale.edu/smarts/smarts13m/ext.coeffsCCD
[46] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele13/ext.coeffsIR
[47] http://www.ctio.noao.edu/noao/content/13-m-smarts-photometric-calibrations-bvri
[48] http://www.ctio.noao.edu/noao/content/13-m-SMARTS-Photometric-Calibrations-JHK
[49] http://www.ctio.noao.edu/noao/content/smarts-consortium
[50] mailto:charles.bailyn@yale.edu
[51] mailto:victoria.gardner@yale.edu?subject=SMARTS%20ANDICAM%20observing
[52] mailto:depoy@astronomy.ohio-state.edu
[53] mailto:pogge@astronomy.ohio-state.edu
[54] mailto:michelle.buxton@yale.edu
[55] mailto:swt@astro.yale.edu
[56] mailto:csmith@noao.edu?subject=ANDICAM
[57] http://www.ctio.noao.edu/noao/content/andicam
[58] http://www.astro.yale.edu/cgi-bin/ANDICAM/Obs/obsentry.pl
[59] http://www.ctio.noao.edu/noao/content/ANDICAM-Contacts
[60] http://www.astro.yale.edu/smarts/ANDICAM/Obs/phase2.html
[61] http://www.astro.yale.edu/smarts/ANDICAM/Obs/obshelp.html
[62] http://www.astro.yale.edu/smarts/ANDICAM/Obs/moshelp.html
[63] http://www.astro.yale.edu/smarts/ANDICAM/Obs/ph2help.html
[64] http://www.astro.yale.edu/smarts/ANDICAM/Obs/mgrhelp.html
[65] http://www.astro.yale.edu/smarts/ANDICAM/Obs/oldobs.html
[66] http://www.ctio.noao.edu/noao/content/andicam-phase-ii-observing-tools
[67] http://www.ctio.noao.edu/noao/content/andicam-contacts
[68] http://www.ctio.noao.edu/noao/content/andicam-phase-ii-submission-instructions
[69] http://www.ctio.noao.edu/noao/content/andicam-phase-ii
[70] http://www.ctio.noao.edu/noao/content/andicam-filters
[71] https://www.astro-research.org/
[72] http://www.astro.yale.edu/smarts/13-m-telescope.htm
[73] http://www.ctio.noao.edu/noao/content/y4kcam
[74] http://www.astronomy.ohio-state.edu/Y4KCam/detector_ap7.html
[75] http://www.ctio.noao.edu/noao/content/ctio-3x3-inch-and-4x4-inch-filters
[76] http://www.astro.yale.edu/smarts/smarts1.0m.html
[77] http://www.astronomy.ohio-state.edu/Y4KCam/
[78] http://www.astronomy.ohio-state.edu/Y4KCam/detector.html
[79] http://www.itl.arizona.edu/
[80] http://www.astro-cam.com/
[81] http://www.astronomy.ohio-state.edu/Y4KCam/OSU4K/index.html#DQE
[82] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele10/y4kcam_bias_071210.jpg
[83] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele10/y4kcam_star_071210.jpg
[84] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele10/badpix.1.0m.pl.txt
[85] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele10/badpix.1.0m.2x2.pl.txt
[86] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele10/y4kshut_300ms.jpg
[87] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele10/y4k_xtalk.jpg
[88] http://www.ctio.noao.edu/noao/sites/default/files/instruments/imagers/y4kcam_xtalk.txt
[89] http://www.astronomy.ohio-state.edu/Y4KCam/Y4KObsguide.pdf
[90] http://www.ctio.noao.edu/noao/sites/default/files/1m_observing.pdf
[91] http://www2.lowell.edu/users/massey/obins/y4kcamred.html
[92] http://www.ctio.noao.edu/noao/sites/default/files/quadproc_head.txt
[93] http://www.ctio.noao.edu/noao/sites/default/files/quadproc_head_2x2.txt
[94] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele10/phot.txt
[95] http://www.ctio.noao.edu/noao/content/13-m-logs-2011
[96] http://www.ctio.noao.edu/noao/content/13-m-logs-2010
[97] http://www.ctio.noao.edu/noao/content/13-m-logs-2009
[98] http://www.ctio.noao.edu/noao/content/13-m-logs-2008
[99] http://www.ctio.noao.edu/noao/content/13-m-logs-2007
[100] http://www.ctio.noao.edu/noao/content/13-m-logs-2006
[101] http://www.ctio.noao.edu/noao/content/15-m-logs-2006a
[102] http://www.ctio.noao.edu/noao/content/15-m-logs-2005b
[103] http://www.ctio.noao.edu/noao/content/13-m-logs-2005
[104] http://www.ctio.noao.edu/noao/content/15-m-logs-2005a
[105] http://www.ctio.noao.edu/noao/content/15-m-logs-2004b
[106] http://www.ctio.noao.edu/noao/content/13-m-logs-2004
[107] http://www.ctio.noao.edu/noao/content/10-m-Logs-2004
[108] http://www.ctio.noao.edu/noao/content/15-m-logs-2004a
[109] http://www.ctio.noao.edu/noao/content/15-m-logs-2003b
[110] http://www.ctio.noao.edu/noao/content/13-m-logs-2003
[111] http://www.astro.sunysb.edu/fwalter/SMARTS/smarts_15msched.html
[112] http://www.astro.yale.edu/smarts/15-m-telescope.htm
[113] http://www.astro.yale.edu/smarts/10-m-telescope.htm
[114] http://www.chara.gsu.edu/~thenry/SMARTS/
[115] http://www.astro.yale.edu/smarts/contact.htm
[116] http://www.astro.yale.edu/smarts/operatingplan.htm
[117] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/SMARTS2MOU.v3.pdf
[118] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/SMARTSAppendixA.pdf
[119] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/SMARTSAppendixC.pdf
[120] http://www.ctio.noao.edu/noao/content/mou-appendix-d
[121] http://www.ctio.noao.edu/noao/content/smarts-telescopes-history
[122] mailto:wsmith@aura-astronomy.org
[123] mailto:centerline@noao.edu
[124] mailto:csmith@noao.edu?subject=SMARTS2%20Consortium
[125] mailto:charles.bailyn@yale.edu?subject=SMARTS2%20Consortium
[126] http://www.astro.yale.edu/smarts/observing.html
[127] http://www.ctio.noao.edu/noao/content/observing-through-noao
[128] http://www.astro.yale.edu/smarts/about.htm
[129] http://www.chara.gsu.edu/~thenry/SMARTS/smarts.dutiesproposers.user
[130] http://chiron.astro.yale.edu/
[131] http://www.ctio.noao.edu/noao/content/planning-executing-wrapping-your-run-ctio
[132] http://www.ctio.noao.edu/noao/content/visiting-astronomers-travel-guide
[133] http://www.ctio.noao.edu/noao/content/sky-conditions
[134] http://ast.noao.edu/data
[135] http://www.ctio.noao.edu/noao/content/Fiber-Echelle-Spectrograph
[136] http://www.ctio.noao.edu/noao/content/ASCAP
[137] http://www.ctio.noao.edu/spectrographs/4m_Echelle/4m_echelle.html
[138] http://www.ctio.noao.edu/noao/sites/default/files/instruments/spectrographs/ech_manual.pdf
[139] http://www.chara.gsu.edu/~thenry/SMARTS/schedule2012B.htm
[140] http://www.astro.yale.edu/smarts/schedules/sched10m2012b.txt
[141] http://www.astro.yale.edu/smarts/schedules/sched13m2012b.txt
[142] http://www.astro.yale.edu/smarts/schedules/sched15m2012b.txt
[143] http://www.astro.yale.edu/smarts/previous.htm