SMARTS Consortium

SMARTS

Small and Moderate Aperture Research Telescope System

[1]

The SMARTS Consortium operates four small telescopes (1.5-m [2], 1.3-m [3], 1.0-m [4] and 0.9-m [5]) on Cerro Tololo. Observations can be secured by purchasing time on the telescopes, and membership is open to individuals or institutions, including international partners. The primary website for SMARTS information is https://www.astro.gsu.edu/~thenry/SMARTS [6], and the primary contact is SMARTS Principal Scientist Todd Henry. Additional information can be found via the links below.

Observing through NOIRLab

The NOIRLab community (that is, anyone eligible to apply for time on any NOIRLab telescope) may apply for time on the SMARTS telescopes through the standard NOIRLab proposal procedure [7]. NOIRLab users are assigned approximately 15% of the total time the facilities are open, averaged over all telescopes.

Telescope	Instrument	Observing mode
SMARTS 1.5-meter [2] (60-inch)	CHIRON Spectrograph	service/queue mode
SMARTS 1.3-meter [3] (ex-2MASS)	(none)	available for new instrumentation as of August 2020
SMARTS 1.0-meter [4] (Yale)	Optical Imager	fully robotic
SMARTS 0.9-meter [5] (36-inch)	2K Optical Imager	classical observing, BVRI, ugriz, other filter combinations available

The Process of Applying

Choose the telescope and instrument combination

From the table above, select the appropriate telescope/instrument combination. Note that an instrument provided by a SMARTS Consortium member (e.g., at the 1.0m) may be dedicated mostly or entirely to a specific project, leaving little or no time for other users.

Precision photometry is best carried out on the 0.9m or 1.0m.
Wide-field imaging is best carried out on the 0.9m or 1.0m.
Precision astrometry is possible given the stability of the 0.9m instrument.
Narrow-band and unusual filters from the CTIO collection are most easily accomodated at the 0.9m.
High-resolution spectroscopy is done at the 1.5m. Queue observing makes it possible to carry out short, medium, or long term programs.

Choose the observing mode and required time

Using estimates of exposure time, period coverage, number of targets, etc.

Imaging/photometry programs that require observer intervention, or for other reasons should be done in classical (visiting astronomer) mode, should be carried out on the 0.9m. Note that at the 0.9m, you are the telescope operator. Mountain personnel will install your requested set-up in the afternoon and get you started operating the telescope in the beginning of the evening. If trouble occurs late at night, a limited amount of assistance can be called in, subject to aperture priority (which means that the 4m will be attended to first if it has trouble). New observers must arrive on the mountain at least one night early to familiarize themselves with the telescope, and if possible be accompanied by a veteran.
Synoptic observations can be carried out contemporaneously at the 0.9m or 1.0m for imaging and the 1.5m for spectroscopy.
Programs proposed to be done in service mode at the 1.0m (imaging) or 1.5m (spectroscopy) must be noted as such in the observing proposal. In addition, detailed procedures for carrying out your service observations must be coordinated with the SMARTS Operations Managers (Todd Henry for the 0.9m and 1.5m, Tyler Linder for the 1.0m).
There is no Director's Discretionary time as such on SMARTS telescopes. However, there may be some time not allocated to primary programs. Requests for this time may be submitted in accordance with the CTIO DD time policy. [8] Requests supported by the CTIO Director are forwarded to the SMARTS staff as a secondary time projects. Note that a favorable decision by the CTIO Director does not automatically result in time awarded, because programs from SMARTS Consortium institutions must be considered.

If granted time

You will be contacted by SMARTS personnel to arrange your observations. If you have not yet heard from someone a month before the beginning of the observing semester, please contact SMARTS Principal Scientist Todd Henry. It is best to get in touch well ahead of your run, so that everyone understands the procedures and special requirements, e.g., filters at the 0.9m. Keep in mind that graduate student SMARTS Fellows who are in charge of scheduling are carrying out the task on a part-time basis, and may not be as responsive as a dedicated operations crewmember.
If you are coming to Tololo in person, be sure to check to fill out the Travel Information Questionnaire [9] and the Visitor Support Questionnaire [10]so that the CTIO travel and mountain personnel know you're coming, and what you need. Check the information at Planning, Executing, Wrapping up your run at CTIO [11]. You should also review the details of operations, such as observing manuals, found at http://www.astro.gsu.edu/~thenry/SMARTS [12].

SMARTS History

We continue to update the history of SMARTS. Please contact Todd Henry if you have additional information.

19??: The YALO Consortium was formed by Yale, AURA, U. of Lisbon, and Ohio State University to operate the Yale 1.0m telescope at CTIO.
1998B: YALO queue observations with the optical detector ANDICAM began
1999: the IR array was installed on ANDICAM, enabling simultaneous optical and infared imaging
2001: NOAO announced that it would no longer operate the other small telescopes at CTIO as configured at the time (<2.0m)
2001 JUL: Charles Bailyn, PI of YALO, approached the community with the idea of forming a larger Consortium to maintain the small telescope capabilities.
2001 OCT: The SMARTS consortium was born at a meeting at the American Museum of Natural History. The product of that meeting was a commitment on the part of Consortium members to write a proposal to the NSF.
??? The NSF proposal was accepted, with the second and third year of operations to be awarded based on the success of the first year's effort.
2002 SEP 24: The YALO 1.0m project finished operations. ANDICAM moved to the 1.3m for the 2003A observing semester by a team led by Darren DePoy.
2003 FEB 01: SMARTS officially began its operation of the CTIO 0.9-m, 1.3-m and 1.5-m telescopes
2003 MAR: OSU installed a new 12-position filter wheel and CCD at the 1.0m.
2003 NOV: SMARTS operations renewed for second and third years.
2004 MAY 12: SMARTS operations at the 1.0m telescope began with the first visiting astronomer.
2004 MAY 28: The first SMARTS queue/service observing block began at the 1.0m telescope.
2005 APR: A new Telescope Control System for the 0.9m was installed.
2005 JULY 07: The Y4KCam began regular observing operations at the 1.0m telescope.
2006 JAN 09: The SMARTS2 Consortium Agreement took effect.
2006B: The SMARTS 1.5m telescope begins to run in full queue mode for the RC Spec and the CPAPIR.

History and pictures of the SMARTS telescopes [13]

SMARTS Telescopes' Histories

The SMARTS 0.9-meter telescope [5] (also called the 36" telescope) has a single-arm equatorial mount and was constructed in 1965 by Boller and Chivens. It is a closed-tube Cassegrain design and is currently equipped with a visible-light camera having a 2K CCD. It has found a great deal of use as a stable photometric and astrometric instrument and has proven to be a reliable and durable telescope. As of August 2020, it is operated in classical mode and is an ideal facility for student training. Click here for more details of the history of the 0.9m... [14]

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The Yale 1.0-meter telescope [4], originally sited in Bethany, CT, was moved to CTIO in 1972. Between 1998 and 2002 it was run by the YALO Consortium. The 1.0m has a very similar design to the 0.9m in optics and mounting. As pictured, the 1.0m sports the ANDICAM [18], which was later moved to the SMARTS 1.3-meter telescope. As of August 2020, it is operated in robotic mode with an optical imaging camera.

[19]

[20]

The SMARTS 1.3-meter telescope, formerly the southern-hemisphere 2MASS survey telescope, is a much more modern design than the other SMARTS telescopes, using a split-ring altitude-azimuth mount and an optical design optimized for work in the infrared. It fits very neatly into its dome. Here it is shown without the ANDICAM [18] optical/infrared imager. As of August 2020, it is closed, awaiting its next incarnation.

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[22]

The SMARTS 1.5-meter telescope [2] (also called the 60-inch telescope) is an open-tube Cassegrain on a single-arm equatorial mount. It has been operated with both imagers and spectrographs, and the option of two secondaries giving f/13.5 and f/8. As of August 2020, it is operated with a single instrument, the high-resolution optical spectrograph CHIRON [23]. The facility is run full time, primarily with CTIO staff as observers.

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[25]

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0.9-m History

Since (at least) 1999, the SMARTS 0.9-meter [5] telescope has utilized a single instrument, an optical camera with a CCD detector that is 2048 pixels on a side. The scale of the CCD is 401 milliarcseconds/pixel, thereby providing a full field of 13.69 arcminutes, or about 46% the width of the full Moon. The stability of the instrument configuration permits long-term studies that are impossible to do on most telescopes, including one of the largest astrometric programs in the world.

The facility continues to be upgraded, with recent efforts such as new motor bearings for the RA and Dec motors (2019), a new Mac observing station (2018), a new Torrent controller and software for the CCD (2016), and new floors, bathroom, and paint (2013).

The 0.9m [5] dome, located at Cerro Tololo Inter-american Observatory (CTIO) in the foothills of the Chilean Andes.


Constructed in 1965 by Boller & Chivens, the 0.9m [5] is a closed tube design telescope, with instruments attached at the bottom at the Cassegrain focus.


The 0.9 meter = 36 inch "eye" of the 0.9m [5] can be seen, with its attendant secondary mirror support.

The golden dewar contains the CCD detector used for science observations. Electronics and filters are housed in the surrounding black, silver, and gold boxes. The dewar is filled with liquid nitrogen, which has a temperature of 77 Kelvin, in order to keep the "background" low on the detector. The background is comprised of electrons, which are also used to detect light on the detector. So, if fewer electrons are free because of a lower detector temperature, faint signals that generate few electrons in the detector can be better measured.


The CCD can be seen through the final optical element in the light path, the dewar window. Occasionally, the dewar is disconnected from the black box that holds filters and additional optics used to focus images onto the CCD, primarily to clean the window.


The observing room is cozy, including a new floor (not shown) made of imported Peruvian tile.

SMARTS 0.9-m Telescope

SMARTS 0.9-meter telescope web page [6]

About the 0.9-m Telescope

The SMARTS 0.9-meter telescope is a Cassegrain telescope mounted on an off-axis, asymmetric mounting and used on the east side of the pier. As of August 2020 the 0.9m is used for direct imaging with a dedicated 2048x2046 CCD detector. A CCD-based autoguider, which looks at a small off-axis field, is permanently installed. The 0.9-m has been operated by the SMARTS Consortium since 2003 FEB 01.

Observing mode

Classical observing only. In special circumstances some service observing may be possible. Contact Todd Henry for information.

Instruments

Since (at least) 1999, the 0.9-m has been equipped with a dedicated 2048x2046 Tek2K CCD detector. Please refer to the Tek2K instrument page [27] for CCD characteristics.

Note that visitor instruments have been used at the 0.9-m for engineering, which provides a telescope amenable to many imaging applications.

Filters

There are two stacked filter wheels at the 0.9-m. The top wheel includes a color balance filter (for dome flats), neutral density filters, and open slots. The bottom filter wheel slot can hold wheels with 3x3 inch filters (up to 8 filters, typically at least BVRI) or 4x4 inch filters (up to 5 filters, typically ugriz).

See the Filter list [28] for more information on the available filters.

Time Synchronization

For projects that require accurate timing information, here is a quick overview on how the time ends up in the image headers.

There are two different header entries relating to time, UT and UTSHUT:

UT is read from the TCS. While there is a GPS receiver that displays accurate Universal Time in the 0.9-m console room, this information is currently not communicated to the TCS automatically. Instead, the UT should be checked and manually entered into the TCS at the beginning of each night. The absolute accuracy is therefore at best ~1 sec. The TCS clock may drift slightly during the night and is therefore not reliable for precise absolute or relative timing.

UTSHUT is taken from the Torrent controller's clock, which is synchronized to the (needs updating) ...

To check for the correct UT time on the web, try this link to the USNO Master Clock [29].

Tek2K

Tek2K is a 2K optical CCD imager installed on the SMARTS 0.9-meter telescope that provides a 13.6 arcminute field of view with 0.4 arcsecond pixels. Key capabilities of the imaging system at the 0.9-m can be found at http://www.astro.gsu.edu/~thenry/SMARTS/0.9m.capabilities [30].

Detector Parameters (f/13.5)
Pixels	2048x2046
Pixel Scale	0.401"/pixel
Field Size	13.6'x13.6'

CCD Parameters

The observer can control and change the CCD readout format and binning. The entire chip can be read out via a single amplifier, or to reduce the readout time, two (DUAL mode) or four (QUAD mode) amplifiers can be used. The region-of-interest (ROI) can also be adjusted to use an arbitrary section of the CCD. Observers should think carefully about whether or not they need the entire field (if not, read a ROI) or the resolution (if not, bin 2x2) because substantial gains in efficiency are possible by reducing the format or increasing the bin size.

A raw quad-amplifier picture looks a little unusual. Each quadrant has a slightly different electrical offset (ie overscan level), and the four overscan segments are in the center of the picture. The real time display colors any saturated (i.e., 65535 ADUs) pixel in red.

QUAD CCD pictures have to be trimmed and overscan-subtracted in a separate pre-processing IRAF task called quadproc (in the quad package). Note that even after the pictures are trimmed and overscan subtracted, the sky levels in each quadrant will not be identical (unless the sky level is zero). This is because each of the four CCD amplifiers has a slightly different gain. After the trimming and overscan correction with quadproc, the images can be processed (bias subtraction, flatfielding) in the standard manner.

Data Acquisition Procedures

A night assistant is not provided at the SMARTS 0.9-meter telescope. An Observer's Manual, including details about the telescope, instrument, telescope control system, and data acquistion system is provided in the observing room and at http://www.astro.gsu.edu/~thenry/SMARTS/ [6].

Sky flats and dome flats can be taken. Dome flat exposure times to reach a level of about 25,000 ADU are:

Filter	Exp Time (sec)
B	180
V	100
R	110
I	120

[31]	A sample "master" Bias frame (quad readout) after overscan correction and trimming with quadproc (click on the image for an expanded view). The frame was created by averaging 20 individual frames (rejection option "minmax").
[32]	A sample "master" Flatfield frame (quad readout, V filter) after overscan correction and trimming with quadproc (click on the image for an expanded view). The frame was created by median combining 10 individual frames (rejection option "avsigclip").

Crosstalk

When using multiple-amplifier readout, the signal from one amplifier can "leak" into the signal of another. Crosstalk is an additive effect and is proportional to the signal strength in a given amplifier. In the sample frame shown below, this effect shows up as negative (white) images of bright stars in the lower left and upper right quadrants. The white images in the upper right quadrant correspond to the (black) star images of the lower left quadrant (flip the upper right quadrant left-right and up-down).

[33]	A reduced 2048x2048 frame (quad readout) showing examples of "crosstalk" (click on the image for an expanded view).

SMARTS 1.5-m Telescope

About the SMARTS 1.5-meter Telescope

The 1.5-m telescope is mounted on an asymmetric, off-axis mount and is used on the east side of the pier. It is not possible to reverse the telescope over the pier.

CHIRON

The CHIRON [23] high-resolution spectrograph is the only instrument in use at the SMARTS 1.5-m telescope as of August 2020. In the past, the 1.5-m has also hosted the following (now retired) instruments: Bench Mounted Echelle (BME) Spectrograph, the 1.5-m RC Spectrograph, the Automated Single Channel Photometer (ASCAP), OSIRIS and CIRIM IR imagers, a Cass focus CCD (CFCCD) Imager and the CPAPIR wide-field IR Imager.

All Cassegrain instruments are mounted on an instrument rotator, and thus they may be placed at any position angle on the sky. However, rotation is performed manually and can only be done near zenith, so changing the PA usually requires at least 10 min. The angle can be read to ± 0.1 degree. Variable speed, D.C. motors have been incorporated into both the right ascension and declination drives in order to improve the efficiency of the telescope for infrared work.

Restricted View Towards the 4.0-m

The view of the 1.5-meter telescope is restricted when looking towards the SE by the dome of the 4.0-meter telescope. At the following declinations, exceeding the indicated hour angle will cause the view to be obstructed:

DEC (deg)	Hour Angle (h m)
-50	5:44 E
-55	5:30 E
-60	5:05 E
-65	4:55 E
-70	4:50 E
-75	4:10 E

Graph of theoretical image quality [34] over the FOV and sensitivity of focus with temperature change.

SMARTS Publications

Refereed [35]
Ph.D. Theses [36]
Telegrams & Conference Abstracts [37]
Acknowledging SMARTS [38]

Refereed

SMARTS refereed publications per year

Refereed Publications in the Yale website [39]

2004

2005

2006

2007

2008

2009

2010

Marscher, Alan P.; Jorstad, S. G.; Larionov, V. M.; Aller, M. F.; Aller, H. D.; Lähteenmäki, A.; et al. 2010ApJ...710L.126M
"Probing the Inner Jet of the Quasar PKS 1510-089 with Multi-Waveband Monitoring During Strong Gamma-Ray Activity" [235]

2011

Agudo, I.; Jorstad, S. G.; Marscher, A. P.; Larionov, V. M.; Gómez, J. L.; Lähteenmäki, A.; Gurwell, M.; Smith, P. S.; Wiesemeyer, H.; Thum, C.; Heidt, J.; Blinov, D. A.; D'Arcangelo, F. D.; Hagen-Thorn, V. A.; Morozova, D. A.; Nieppola, E.; Roca-Sogorb, M.; Schmidt, G. D.; Taylor, B.; Tornikoski, M.; Troitsky, I. S. 2011ApJ...726L..13A
"Location of γ-ray Flare Emission in the Jet of the BL Lacertae Object OJ287 More than 14 pc from the Central Engine" [247]

Clocchiatti, A.; Suntzeff, N. B.; Covarrubias, R.; Candia, P. 2011AJ....141..163C
"The Ultimate Light Curve of SN 1998bw/GRB 980425" [252]

Faherty, J.; Burgasser, A. J.; Walter, F. M.; van der Bliek, N. S.; Shara, M. M.; Cruz, K. L.; Vrba, F. J.; Schmidt, S. J.; West, A. A. 2011AAS...21722605F
"The Brown Dwarf Kinematics Project (BDKP): How Distances Both Advance and Complicate Our Understanding of the Brown Dwarf Population" [255]

Palma, N. I.; Böttcher, M.; de la Calle, I.; Agudo, I.; Aller, M.; Aller, H.; Bach, U.; Benítez, E.; Buemi, C. S.; Escande, L.; Gómez, J. L.; Gurwell, M. A.; Heidt, J.; Hiriart, D.; Jorstad, S. G.; Joshi, M.; Lähteenmäki, A.; Larionov, V. M.; Leto, P.; Li, Y.; López, J. M.; Lott, B.; Madejski, G.; Marscher, A. P.; Morozova, D. A.; Raiteri, C. M.; Roberts, V.; Tornikoski, M.; Trigilio, C.; Umana, G.; Villata, M.; Wylezalek, D. 2011ApJ...735...60P
"Multiwavelength Observations of the Gamma-Ray Blazar PKS 0528+134 in Quiescence" [261]

Piatti, A. E.; Clariá, J. J.; Parisi, M. C.; Ahumada, A. V. 2011PASP..123..519P
"First Estimates of the Fundamental Parameters of Three Large Magellanic Cloud Clusters" [262]

Rabinowitz, D.; Tourtellotte, S.; Rojo, Patricio; Hoyer, S.; Folatelli, G.; Coppi, P.; Baltay, C.; Bailyn, C. 2011ApJ...732...51R
"Discovery and Characterization of an Extremely Deep-eclipsing Cataclysmic Variable: LSQ172554.8-643839" [263]

Rubin, R. H.; Simpson, J. P.; O'Dell, C. R.; McNabb, I. A.; Colgan, S. W. J.; Zhuge, S. Y.; Ferland, G. J.; Hidalgo, S. A. 2011MNRAS.410.1320R
"Spitzer reveals what is behind Orion's Bar" [267]

Shih, I. C.; Charles, P. A.; Cornelisse, R. 2011MNRAS.412..120S
" Correlated optical/X-ray long-term variability in LMXB 4U 1636-536" [268]

Shin, I.-G.; Udalski, A.; Han, C.; Gould, A.; Dominik, M.; Fouqué, P.; Kubiak, M.; Szymanski, M. K.; Pietrzynki, G.; Soszynski, I.; Ulaczyk, K.; Wyrzykowski, L.; et al. 2011ApJ...735...85S
"OGLE-2005-BLG-018: Characterization of Full Physical and Orbital Parameters of a Gravitational Binary Lens" [269]

Skemer, A. J.; Close, L. M.; Szucs, L.; Apai, D.; Pascucci, I.; Biller, B. A. 2011ApJ...732..107S
"Evidence Against an Edge-on Disk Around the Extrasolar Planet, 2MASS 1207 b and a New Thick-cloud Explanation for Its Underluminosity" [270]

Winters, J. G.; Henry, T. J.; Jao, W.; Subasavage, J. P.; Finch, C. T.; Hambly, N. C. 2011AJ....141...21W
"The Solar Neighborhood. XXIII. CCD Photometric Distance Estimates of SCR Targets—77 M Dwarf Systems within 25 pc" [271]

Woitke, P.; Riaz, B.; Duchêne, G.; Pascucci, I.; Lyo, A.-R.; Dent, W. R. F.; Phillips, N.; Thi, W.-F.; Ménard, F.; Herczeg, G. J.; Bergin, E.; Brown, A.; Mora, A.; Kamp, I.; Aresu, G.; Brittain, S.; de Gregorio-Monsalvo, I.; Sandell, G. 2011A&A...534A..44W
"The unusual protoplanetary disk around the T Tauri star ET Chamaeleontis" [272]

2012

Ph.D. Theses

SMARTS Ph.D. Theses

2019 Silverstein, Michele L. "Sizing Up Red Dwarfs in the Solar Neighborhood" (PhD) Georgia State University

2017 Clements, Tiffany, D. "Nearby M Dwarf Stars and The Wide Main Sequence" (PhD) Georgia State University

2017 Chatelain, Joseph P. "De Ilii Coloribus: Photometric Study of the Largest Jupiter Trojan Asteroids" (PhD) Georgia State University

2015 Winters, Jennifer G. "Nearby Red Dwarfs & Their Dance Partners: Characterizing More Than 2000 Single & Multiple M Dwarfs Near the Sun" (PhD) Georgia State University

2013 Dieterich, Serge B. "Characterization of the Stellar/Substellar Boundary" (PhD) Georgia State University

2012 Riedel, Adric R. "Hiding in Plain Sight" (PhD) Georgia State University

2012 Richardson, Noel D. "Spectroscopy and Interferometry of the Winds of Luminous Blue Variables" (PhD) Georgia State University

2011 Williams, S.J. "Optical Spectroscopy of Massive Stars [275]" (PhD) Georgia State University

2011 Aragona, C. "Multiwavelength Studies of Gamma-ray Binaries Thesis (PhD) Lehigh University

2009 Cantrell, A. G. "Phase Shifts and Nonellipsoidal Light Curves: Challenges from Mass Determinations in X-ray Binary Stars" Thesis (PhD) Georgia State University [276]

2009 Dong, S. "Astrophysical Applications of Gravitational Microlensing" Thesis (PhD) Ohio State University [277]

2009 Poindexter, S. D. "Sharpening the Tools of Gravitational Microlensing" Thesis (PhD) Ohio State University [278]

2009 Raghavan, D. "A Survey of Stellar Families: Multiplicity of Solar-Type Stars" Thesis (PhD) Georgia State University [279]

2009 Trippe, M.L. "A Multi-Wavelength Investigation of Seyfert 1.8 and 1.9 Galaxies" Thesis (PhD) Georgia State University [280]

2008 Cobb, B.E. "Long-term observations of GRBs: the complex connection between GRBs and SNe" Thesis (PhD) Yale University [281]

2008 Morgan, C.W. "Quasar Structure from Microlensing in Gravitationally Lensed Quasars" Thesis (PhD) Ohio State University [282]

2008 Ryle, W.T. "The Link Between the Optical Variability of Blazars and their Black Hole Engines" Thesis (PhD) Georgia State University [283]

2007 Dunn, J.P. "Intrinsic Absorption with the Far Ultraviolet Spectroscopic Explorer" Thesis (PhD) Georgia State University [284]

2007 Subasavage, J.P. "White Dwarfs in the Solar Neighborhood" Thesis (PhD) Georgia State University [285]

2006 Marshall, K. "The X-ray Variability of Seyfert Galaxies" Thesis (PhD) Georgia State University [286]

2006 Osterman, A. "New Multiwavelength Variability and Optical Microvariability Investigations of X-ray and Radio Selected Blazars" Thesis (PhD) Georgia State University [287]

2006 Maitra, D. "State Transitions in Soft X-ray Transients" Thesis (PhD) Yale University [288]

2005 McFarland, J. P. "Rest Frame Variability Characteristics of Blazars" Thesis (PhD) Georgia State University [289]

2004 McSwain, M. V. "The Evolution of Massive Stars: The Be Star and Microquasar Phenomena" Thesis (PhD) Georgia State University [290]

2004 Jao, W. C. "Discovery and Characterization of the Highest Proper Motion Stars" Thesis (PhD) Georgia State University [291]

Telegrams & Conference Abstracts

SMARTS telegrams and conference abstracts per year

2011 [292]
2010 [293]
2009 [294]
2008 [295]
2007 [296]
2006 [297]
2005 [298]
2004 [299]
2003 [300]

2003

2004

2005

2006

2007

2008

2009

2010

2011

Bailyn, C. D.; Buxton, M. 2011AAS...21822905B
"Long Term Monitoring of Black Hole Binaries with SMARTS" [503]

Bonning, E.; Bailyn, C.; Buxton, M.; Chatterjee, R.; Coppi, P.; Isler, J.; Urry, C. M.; Maraschi, L.; Fossati, G. 2011ATel.3212....1B
"Optical and infrared observations of PKS 1124-186" [504]

Bonning, E.; Bailyn, C.; Buxton, M.; Chatterjee, R.; Coppi, P.; Isler, J.; Urry, C. M.; Maraschi, L.; Fossati, G. 2011ATel.3337....1B
"SMARTS optical and IR observations of PKS 1424-41" [505]

Chatterjee, R.; Bailyn, C. D.; Bonning, E. W.; Buxton, M.; Coppi, P.; Isler, J.; Urry, C. M.; Fossati, G.; Maraschi, L. 2011ATel.3591....1C
"Optical-IR Re-Brightening of the Blazar PKS 0208-512" [506]

Chatterjee, R.; Bailyn, C.; Bonning, E.; Buxton, M.; Coppi, P.; Isler, J.; Urry, C. M. 2011AAS...21832702C
"Similarity of Optical-IR and Gamma-Ray Variability Properties of Fermi Blazars" [507]

Cobb, B. E. 2011GCN.12081....1C
"GRB 110618A: SMARTS optical observations." [508]

Isler, J.; Bailyn, C.; Bonning, E.; Buxton, M.; Chatterjee, R.; Coppi, P.; Fossati, G.; Maraschi, L.; Scalzo, R.; Urry, C. 2011AAS...21840808I
"SMARTS Optical Spectroscopy of 3C 454.3" [509]

MacDonald, R. K. D.; Bailyn, C. D.; Cantrell, A. G. 2011AAS...21714420M
"Mass of the Black Hole in V4641 Sgr" [510]

Macias, P.; Orosz, J. A.; Bailyn, C. D.; Buxton, M. M.; Schechter, P. L.; Remillard, R. A.; McClintock, J. E.; Steiner, J. F. 2011AAS...21714304M
"A Refined Black Hole Mass for the X-ray Transient GRS 1009-45" [511]

Maitra, D.; Cantrell, A.; Markoff, S.; Falcke, H.; Miller, J.; Bailyn, C. 2011IAUS..275...82M
"Jets at lowest mass accretion rates" [512]

Rabinowitz, D. L.; Tourtellotte, S.; Baltay, C.; Bailyn, C.; Coppi, P.; Rojo, P.; Folatelli, G.; Hoyer, S. 2011AAS...21712604R
"An Extremely Deep-Eclipsing Cataclysmic Variable discovered with La Silla - QUEST" [513]

Wells Bonning, E.; Bailyn, C.; Buxton, M.; Chatterjee, R.; Coppi, P.; Fossati, G.; Isler, J.; Maraschi, L.; Urry, C. 2011AAS...21740801W
"The Exceptional Flaring Activity Of The Blazar 3C 454.3" [514]

Acknowledging SMARTS

We are tracking refereed publications and Ph.D.s awarded that use SMARTS telescopes and data. There are several things you can do to help continue the success of SMARTS:

1. When appropriate, a reference to SMARTS in the abstracts of papers is appreciated.

2. Please include a reference to SMARTS in your acknowledgements if you used any data from the SMARTS telescopes, such as:

This research has used data from the SMARTS [1.5m/1.3m/1.0m/0.9m] telescope, which is operated as part of the SMARTS Consortium.

3. Investigators who obtained time through NOIRLab should also use the usual NOIRLab acknowledgement [515].

4. Please notify the SMARTS Principal Scientist (as of August 2020, Todd Henry) of your publication or the successful completion of Ph.D. work by graduate students, with the student's name, dissertation title, and date of Ph.D.

Links
[1] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/smartsnewpic.JPG
[2] http://www.ctio.noao.edu/noao/content/15-m-telescope
[3] http://www.ctio.noao.edu/noao/content/13-m-telescope
[4] http://www.ctio.noao.edu/noao/content/10-m-telescope
[5] http://www.ctio.noao.edu/noao/content/09-m-telescope
[6] http://www.astro.gsu.edu/~thenry/SMARTS/
[7] http://ast.noao.edu/observing/proposal-info
[8] http://www.ctio.noao.edu/noao/content/directors-discretionary-dd-time
[9] http://www.ctio.noao.edu/noao/content/Travel-Information-Questionnaire
[10] http://www.ctio.noao.edu/noao/eform/submit/vistor-support-questionaire
[11] http://www.ctio.noao.edu/noao/content/Planning-Executing-Wrapping-your-run-CTIO
[12] http://www.astro.gsu.edu/~thenry/SMARTS
[13] http://www.ctio.noao.edu/noao/content/smarts-telescopes-history
[14] http://www.ctio.noao.edu/noao/content/09-m-history
[15] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/pointnine_3.gif
[16] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/point9_2.jpg
[17] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/point9_1.jpg
[18] http://www.ctio.noao.edu/noao/content/andicam
[19] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/one_1.jpg
[20] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/one_andicam.jpg
[21] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/oneptthree_1.jpg
[22] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/oneptthree_2.jpg
[23] http://www.ctio.noao.edu/noao/content/chiron
[24] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/oneptfive_1.jpg
[25] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/oneptfive_2.jpg
[26] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/oneptfive_3.jpg
[27] http://www.ctio.noao.edu/noao/content/Tek2K
[28] http://www.ctio.noao.edu/noao/content/ctio-3x3-inch-and-4x4-inch-filters
[29] http://tycho.usno.navy.mil/what1.html
[30] http://www.astro.gsu.edu/~thenry/SMARTS/0.9m.capabilities
[31] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele09/0.9zero.jpg
[32] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele09/0.9vflat.jpg
[33] http://www.ctio.noao.edu/noao/sites/default/files/telescopes/smarts/tele09/0.9crosstalk.jpg
[34] http://www.ctio.noao.edu/noao/sites/default/files/intranet/1.5-m-focus60.gif
[35] http://www.ctio.noao.edu/noao/content/refereed
[36] http://www.ctio.noao.edu/noao/content/phd-theses
[37] http://www.ctio.noao.edu/noao/content/telegrams-conference-abstracts
[38] http://www.ctio.noao.edu/noao/content/acknowledging-smarts
[39] http://www.astro.yale.edu/smarts/refereed.html
[40] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AJ....127..252B&,db_key=AST&,high=4050e3f24419515
[41] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...617..645B&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7028222
[42] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0408156
[43] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...616.1118C&,db_key=AST&,high=4050e3f24413433
[44] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...608L..93C&,db_key=AST&,high=4050e3f24419060
[45] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...603..595F&,db_key=AST&,high=3bc1f52f0203533
[46] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...605..368G&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7020158
[47] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AJ....128.2460H&,db_key=AST&,high=4050e3f24410133
[48] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0312626
[49] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AJ....128.3034K&,db_key=AST&,high=3bc1f52f0220870
[50] http://adsabs.harvard.edu/abs/2004ApJ...606..381L
[51] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...608..444M&,db_key=AST&,high=4050e3f24417396
[52] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...600..927M&,db_key=AST&,high=4050e3f24409986
[53] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0402085
[54] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJS..151..357S&db_key=AST&high=3d3c3a078103234
[55] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0410393
[56] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AJ....128.1872W&,db_key=AST&,high=4050e3f24409888
[57] http://www.astro.sunysb.edu/fwalter/PUBS/V1647Ori.ps
[58] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...632L..45B&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7003947
[59] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...635L..97B&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7027169
[60] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005MNRAS.364..179C&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7031672
[61] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005A%26A...442..917C&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7031672
[62] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005MNRAS.362..649C&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7031672
[63] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005MNRAS.360..655C&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7031672
[64] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...621L..61C&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7031672
[65] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0411621
[66] http://adsabs.harvard.edu/abs/2005ApJ...623L.117C
[67] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005AJ....130..337C&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7008554
[68] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005AJ....129..409D&,db_key=AST&,high=4050e3f24407790
[69] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...623..700D&,db_key=AST&,high=4050e3f24408429
[70] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...624..295&,db_key=AST&,high-426ea6271007384
[71] http://adsabs.harvard.edu/abs/2005PASP..117.1187H
[72] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005AJ....129.1954J&,db_key=AST&,high=4050e3f24410133
[73] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0502285
[74] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0507498
[75] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0501336
[76] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0509136
[77] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJS..161..118M&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7009131%22
[78] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...622.1052M&,db_key=AST&,high=4050e3f24411664
[79] http://xxx.lanl.gov/abs/astro-ph/0508151
[80] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005PASP..117..944S&,db_key=AST&,data_type=HTML&,format=&,high=44b7ee859714298
[81] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005AJ....130.1658S&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7010026
[82] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005AJ....129..413S&,db_key=AST&,high=4050e3f24410133
[83] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ApJ...627.1057T&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a23284
[84] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0505451
[85] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0609419
[86] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0510401
[87] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ApJ...643L..61B&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a21118
[88] http://xxx.lanl.gov/abs/astro-ph?papernum=0610619
[89] http://adsabs.harvard.edu/abs/2006MNRAS.368.1078C
[90] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ApJ...651L..85C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a09906
[91] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ApJ...645L.113C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a09906
[92] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0603582
[93] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006A%26A...446..279C&,db_key=AST&,data_type=HTML&,format=&,high=45db2332ab28695
[94] http://xxx.lanl.gov/abs/astro-ph/0606243
[95] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0509065
[96] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0608598
[97] http://adsabs.harvard.edu/abs/2006ApJ...637.1094F
[98] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ApJ...645..450F&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a11293
[99] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0601245
[100] http://adsabs.harvard.edu/abs/2006PASP..118..678G
[101] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?doi=10.1111%2Fj.1365-2966.2006.10314.x&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7023318
[102] http://adsabs.harvard.edu/abs/2006ApJ...644L..37G
[103] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0512039
[104] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006AJ....132.2360H&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a18027
[105] http://adsabs.harvard.edu/abs/2006ApJ...652..709H
[106] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0611275
[107] http://adsabs.harvard.edu/abs/2006ApJ...637L..73K
[108] http://arxiv.org/abs/astro-ph/0508070
[109] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0510531
[110] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ApJ...638..446M&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7021775
[111] http://arxiv.org/abs/astro-ph/0601523
[112] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006A%26A...460..415P&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10427
[113] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0601684
[114] http://xxx.lanl.gov/abs/astro-ph?papernum=0509401
[115] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ApJ...646..523R&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a18027%22
[116] http://adsabs.harvard.edu/abs/2006AJ....132..866R
[117] http://adsabs.harvard.edu/abs/2006A%26A...455..255S
[118] http://adsabs.harvard.edu/abs/2006Ap%26SS.304..303S
[119] http://adsabs.harvard.edu/abs/2006Natur.440..311S
[120] http://adsabs.harvard.edu/abs/2006Ap%26SS.304..401S
[121] http://adsabs.harvard.edu/abs/2006AJ....132..360W
[122] http://adsabs.harvard.edu/abs/2007AJ....133..387A
[123] http://adsabs.harvard.edu/abs/2007ApJS..168..128B
[124] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0708.4224
[125] http://adsabs.harvard.edu/abs/2007A%26A...468.1039B
[126] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2007AJ....133..284B&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a11777
[127] http://adsabs.harvard.edu/abs/2007AdSpR..40.1294B
[128] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2007astro.ph..1758C&,db_key=PRE&,data_type=HTML&,format=&,high=45db2332ab28864%22
[129] http://xxx.lanl.gov/abs/astro-ph/0611705
[130] http://xxx.lanl.gov/abs/astro-ph?papernum=0610617
[131] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0703341
[132] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0702240
[133] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0703316
[134] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0707.0028
[135] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0709.1178
[136] http://adsabs.harvard.edu/abs/2007AAS...211.6224G
[137] http://adsabs.harvard.edu/abs/2007AJ....134..241J
[138] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0406208
[139] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2007AJ....133...58K&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10644
[140] http://arxiv.org/abs/0705.1153
[141] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0710.0953
[142] http://adsabs.harvard.edu/cgi-bin/bib_query?2007ApJ...660..301M
[143] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0707.4500
[144] http://xxx.lanl.gov/abs/astro-ph/0610480
[145] http://arxiv.org/abs/astro-ph/0612045
[146] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2007AJ....133...26R&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a19345
[147] http://adsabs.harvard.edu/abs/2007A%26A...463..981R
[148] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0701055
[149] http://adsabs.harvard.edu/abs/2007ApJ...655..434S
[150] http://adsabs.harvard.edu/abs/2007ApJ...664.1154S
[151] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0704.0894
[152] http://adsabs.harvard.edu/abs/2007arXiv0705.3687T
[153] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0709.4373
[154] http://adsabs.harvard.edu/abs/2008ApJ...673L.159C
[155] http://adsabs.harvard.edu/abs/2008ApJ...674..329C
[156] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0801.2084
[157] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0802.3243
[158] http://adsabs.harvard.edu/abs/2008ApJ...677.1157C
[159] http://adsabs.harvard.edu/abs/2008AJ....136.1201D
[160] http://adsabs.harvard.edu/abs/2008A%26A...482L..35G
[161] http://www.sciencemag.org/cgi/content/abstract/319/5865/927
[162] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0805.4734
[163] http://adsabs.harvard.edu/abs/2008ApJ...688..537M
[164] http://adsabs.harvard.edu/abs/2008ApJ...677..880M
[165] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0710.0137
[166] http://adsabs.harvard.edu/abs/2008A%26A...485...95M
[167] http://adsabs.harvard.edu/abs/2008ApJ...676...80M
[168] http://adsabs.harvard.edu/abs/2008ApJ...689..755M
[169] http://adsabs.harvard.edu/abs/2008AJ....135.1946N
[170] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0711.2481
[171] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0707.0003
[172] http://adsabs.harvard.edu/abs/2008Icar..196..225S
[173] http://adsabs.harvard.edu/abs/2008Natur.453.1079S
[174] http://adsabs.harvard.edu/abs/2008AJ....136..899S
[175] http://adsabs.harvard.edu/abs/2008AJ....135.2048T
[176] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0709.3973
[177] http://adsabs.harvard.edu/abs/2008A%26A...488..481V
[178] http://adsabs.harvard.edu/abs/2008ApJ...682..492W
[179] http://adsabs.harvard.edu//abs/2009ApJ...698..514A
[180] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0907.3471
[181] http://adsabs.harvard.edu/abs/2009MNRAS.398..221B
[182] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0906.2235
[183] http://adsabs.harvard.edu/abs/2009ApJ...697.1290B
[184] http://adsabs.harvard.edu/abs/2009ApJ...695L.154B
[185] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0812.4582
[186] http://adsabs.harvard.edu/abs/2009AJ....137.3230C
[187] http://adsabs.harvard.edu/abs/2009A%26A...493...71C
[188] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0805.4492
[189] http://adsabs.harvard.edu/abs/2009MNRAS.tmp.1311C
[190] http://adsabs.harvard.edu/abs/2009ApJ...698.1826D
[191] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0804.1354
[192] http://adsabs.harvard.edu/abs/2009ApJ...699.1196G
[193] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0904.0249
[194] http://adsabs.harvard.edu/abs/2009MNRAS.400..317J
[195] http://adsabs.harvard.edu/abs/2009A%26A...505.1297H
[196] http://adsabs.harvard.edu/abs/2009AJ....137...34K
[197] http://adsabs.harvard.edu/abs/2009AJ....137.4186L
[198] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0911.4798
[199] http://adsabs.harvard.edu/abs/2009ApJ...695L..78L
[200] http://adsabs.harvard.edu/abs/2009AJ....137.3632L
[201] http://adsabs.harvard.edu/abs/2009ApJ...696..601M
[202] http://adsabs.harvard.edu/abs/2009ApJ...697..573O
[203] http://adsabs.harvard.edu/abs/2009BAAA...52..113P
[204] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0811.0768
[205] http://adsabs.harvard.edu/abs/2009ApJ...697..721S
[206] http://adsabs.harvard.edu/abs/2009AJ....137.4547S
[207] http://adsabs.harvard.edu//abs/2009AJ....138.1417T
[208] http://adsabs.harvard.edu/abs/2009MNRAS.tmp.1465T
[209] http://adsabs.harvard.edu//abs/2009ApJ...692.1489W
[210] http://adsabs.harvard.edu/abs/2009ApJ...703.2082Y
[211] http://adsabs.harvard.edu/abs/2010ApJ...709..251B
[212] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0911.2706
[213] http://adsabs.harvard.edu/abs/2010ApJ...718.1079B
[214] http://adsabs.harvard.edu//abs/2010ApJ...710.1127C
[215] http://iopscience.iop.org/1538-3881/140/3/677/
[216] http://adsabs.harvard.edu//abs/2010MNRAS.402.1863C
[217] http://adsabs.harvard.edu//abs/2010AJ....140..954C
[218] http://iopscience.iop.org/0004-637X/718/2/683
[219] http://adsabs.harvard.edu/abs/2010ApJ...718L.150C
[220] http://adsabs.harvard.edu/abs/2010AAS...21530305C
[221] http://adsabs.harvard.edu/abs/2010AJ....140.1766C
[222] http://adsabs.harvard.edu/abs/2010ApJ...719..979C
[223] http://adsabs.harvard.edu/abs/2010ApJ...709..278D
[224] http://adsabs.harvard.edu/abs/2010ApJ...714L.254E
[225] http://adsabs.harvard.edu/abs/2010AJ....140.1414E
[226] http://adsabs.harvard.edu/abs/2010AJ....139..176F
[227] http://adsabs.harvard.edu/abs/2010arXiv1005.0966F
[228] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0910.0475
[229] http://adsabs.harvard.edu/abs/2010AJ....140.2025H
[230] http://adsabs.harvard.edu/abs/2010ApJ...723..797H
[231] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0908.0529
[232] http://adsabs.harvard.edu/abs/2010ApJ...715..362J
[233] http://adsabs.harvard.edu/abs/2010MNRAS.tmp..346K
[234] http://adsabs.harvard.edu/abs/2010A%26A...524A..36K
[235] http://adsabs.harvard.edu/abs/2010ApJ...710L.126M
[236] http://adsabs.harvard.edu/abs/2010ApJ...710..117M
[237] http://adsabs.harvard.edu/abs/2010ApJ...712.1129M
[238] http://adsabs.harvard.edu/abs/2010AJ....139.1534R
[239] http://adsabs.harvard.edu/abs/2010MNRAS.405.1759R
[240] http://adsabs.harvard.edu/abs/2010ApJ...723...81R
[241] http://adsabs.harvard.edu/abs/2010AJ....140.1719S
[242] http://adsabs.harvard.edu/abs/2010Icar..207..699S
[243] http://adsabs.harvard.edu/abs/2010SPIE.7737E..31S
[244] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0912.1171
[245] http://adsabs.harvard.edu/abs/2010arXiv1004.2038T
[246] http://adsabs.harvard.edu/abs/2010A%26A...509A.102V
[247] http://adsabs.harvard.edu/abs/2011ApJ...726L..13A
[248] http://adsabs.harvard.edu//abs/2011MNRAS.415.1355A
[249] http://adsabs.harvard.edu/abs/2011A%26A...531A..73B
[250] http://adsabs.harvard.edu/abs/2011ApJ...739L..51B
[251] http://adsabs.harvard.edu/abs/2011AJ....142..127C
[252] http://adsabs.harvard.edu/abs/2011AJ....141..163C
[253] http://adsabs.harvard.edu/abs/2011MNRAS.412.2454D
[254] http://adsabs.harvard.edu/abs/2011A%26A...530A.108E
[255] http://adsabs.harvard.edu/abs/2011AAS...21722605F
[256] http://adsabs.harvard.edu/abs/2011ApJ...743...26F
[257] http://adsabs.harvard.edu/abs/2011A%26A...531A..61H
[258] http://adsabs.harvard.edu/abs/2011ApJ...743..118H
[259] http://adsabs.harvard.edu/abs/2011AJ....141..117J
[260] http://adsabs.harvard.edu/abs/2011AJ....142..107K
[261] http://adsabs.harvard.edu/abs/2011ApJ...735...60P
[262] http://adsabs.harvard.edu/abs/2011PASP..123..519P
[263] http://adsabs.harvard.edu/abs/2011ApJ...732...51R
[264] http://adsabs.harvard.edu/abs/2011ApJ...730...25R
[265] http://adsabs.harvard.edu/abs/2011AJ....142..201R
[266] http://adsabs.harvard.edu/abs/2011AJ....142..104R
[267] http://adsabs.harvard.edu/abs/2011MNRAS.410.1320R
[268] http://adsabs.harvard.edu/abs/2011MNRAS.412..120S
[269] http://adsabs.harvard.edu/abs/2011ApJ...735...85S
[270] http://adsabs.harvard.edu/abs/2011ApJ...732..107S
[271] http://adsabs.harvard.edu/abs/2011AJ....141...21W
[272] http://adsabs.harvard.edu/abs/2011A%26A...534A..44W
[273] http://adsabs.harvard.edu/abs/2012MNRAS.419.3608C
[274] http://adsabs.harvard.edu/abs/2012ApJ...745...41H
[275] http://digitalarchive.gsu.edu/phy_astr_diss/49/
[276] http://adsabs.harvard.edu/abs/2009PhDT.......199C
[277] http://www.astronomy.ohio-state.edu/Dept/Dissertations/Dong.pdf
[278] http://www.astronomy.ohio-state.edu/Dept/Dissertations/Poindexter.pdf
[279] http://digitalarchive.gsu.edu/phy_astr_diss/31/
[280] http://digitalarchive.gsu.edu/phy_astr_diss/35/
[281] http://adsabs.harvard.edu/abs/2008PhDT........26C
[282] http://www.astronomy.ohio-state.edu/Dept/Dissertations/MorganCW.pdf
[283] http://digitalarchive.gsu.edu/phy_astr_diss/25/
[284] http://digitalarchive.gsu.edu/phy_astr_diss/21/
[285] http://digitalarchive.gsu.edu/phy_astr_diss/15/
[286] http://adsabs.harvard.edu/abs/2006PhDT........24M
[287] http://digitalarchive.gsu.edu/phy_astr_diss/22/
[288] http://adsabs.harvard.edu/abs/2006PhDT........31M
[289] http://adsabs.harvard.edu/abs/2005PhDT........18M
[290] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005PASP..117..309M&,db_key=AST&,high=4050e3f24404777
[291] http://adsabs.harvard.edu/abs/2004PhDT........11J
[292] http://www.ctio.noao.edu/noao/content/2011-0
[293] http://www.ctio.noao.edu/noao/content/2010
[294] http://www.ctio.noao.edu/noao/content/2009-0
[295] http://www.ctio.noao.edu/noao/content/2008-0
[296] http://www.ctio.noao.edu/noao/content/2007-0
[297] http://www.ctio.noao.edu/noao/content/2006-0
[298] http://www.ctio.noao.edu/noao/content/2005-0
[299] http://www.ctio.noao.edu/noao/content/2004-0
[300] http://www.ctio.noao.edu/noao/content/2003
[301] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003GCN..2463....1B&,db_key=AST&,high=4050e3f24419515
[302] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003ATel..171....1B&db_key=AST&high=3f678aaa3c09114
[303] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003GCN..2486....1B&,db_key=AST&,high=4050e3f24419515
[304] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003GCN..2468....1B&,db_key=AST&,high=4050e3f24419515
[305] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003GCN..2481....1B&,db_key=AST&,high=4050e3f24419515
[306] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003GCN..2472....1B&,db_key=AST&,high=4050e3f24419515
[307] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003GCN..2068....1B&db_key=AST&high=3f678aaa3c07965
[308] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003IAUC.8185....1B&,db_key=AST&,high=4050e3f24415891
[309] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003GCN..2329....1B&,db_key=AST&,high=4050e3f24415891
[310] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003GCN..2316....1B&,db_key=AST&,high=4050e3f24415891
[311] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003ATel..206....1B&,db_key=AST&,high=4050e3f24419515
[312] http://adsabs.harvard.edu/abs/2003AAS...203.8103B
[313] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003ATel..170....1B&db_key=AST&high=3f678aaa3c09114
[314] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003SPIE.4841..827D&db_key=AST&high=3f678aaa3c08904%22
[315] http://adsabs.harvard.edu/abs/2003IAUC.8186....1E
[316] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003IAUC.8160....1L&,db_key=AST&,high=4050e3f24415891
[317] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003ATel..125....1M&db_key=AST&high=3f678aaa3c09114
[318] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003ala..conf....1M&db_key=AST&high=4050e3f24400315
[319] http://adsabs.harvard.edu/abs/2003DPS....35.3916R
[320] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003IAUC.8250....1V&,db_key=AST&,high=4050e3f24419515
[321] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003IAUC.8176....3W&,db_key=AST&,high=4050e3f24415891
[322] http://www.astronomerstelegram.org/?read=323
[323] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...20516501B&,db_key=AST&,high=4050e3f24424696
[324] http://adsabs.harvard.edu/abs/2004AAS...20515002B
[325] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.4304B&,db_key=AST&,high=4050e3f24400686
[326] http://adsabs.harvard.edu/abs/2004AAS...20516506B
[327] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004IAUC.8424....1B&,db_key=AST&,high=4050e3f24404223
[328] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004IAUC.8324....2B&,db_key=AST&,high=4050e3f24415891
[329] http://adsabs.harvard.edu/abs/2004DPS....36.0301B
[330] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ATel..316....1B&,db_key=AST&,high=4050e3f24415137
[331] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ATel..270....1B&,db_key=AST&,high=4050e3f24419515
[332] http://adsabs.harvard.edu/abs/2004AAS...20516504B
[333] http://adsabs.harvard.edu/abs/2004AIPC..714..146B
[334] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004GCN..2642....1C&,db_key=AST&,high=417fd0247128158
[335] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.5605D&,db_key=AST&,high=4050e3f24408429
[336] http://adsabs.harvard.edu/abs/2004IAUS..222...87D
[337] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ASPC..313..236F&db_key=AST&high=3bc1f52f0223427
[338] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.1106F&,db_key=AST&,high=3bc1f52f0207015
[339] http://adsabs.harvard.edu/abs/2004DPS....36.3406F
[340] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.3701H&,db_key=AST&,high=4050e3f24410133
[341] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ASPC..313..529H&db_key=AST&high=4050e3f24432389
[342] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.6003J&,db_key=AST&,high=4050e3f24431816
[343] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.4207K&,db_key=AST&,high=4050e3f24403046
[344] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004IAUC.8439....3K&,db_key=AST&,high=4050e3f24422539
[345] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004IAUC.8283....2K&,db_key=AST&,high=4050e3f24417465
[346] http://adsabs.harvard.edu/abs/2004AAS...20516502K
[347] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ATel..288....1M&,db_key=AST&,high=4050e3f24419515
[348] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ATel..279....1M&,db_key=AST&,high=4050e3f24419515
[349] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AIPC..714...56M&db_key=AST&high=4050e3f24404921
[350] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.7905M&,db_key=AST&,high=4050e3f24404173
[351] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.3307M&,db_key=AST&,high=4050e3f24404777
[352] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...205.1301M&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a01510%22
[353] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004IAUC.8295....2R&,db_key=AST&,high=4050e3f24414278
[354] http://adsabs.harvard.edu/abs/2004DPS....36.0302R
[355] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.4205R&,db_key=AST&,high=4050e3f24405910
[356] http://adsabs.harvard.edu/abs/2004IAUC.8369....2S
[357] http://adsabs.harvard.edu/abs/2004IAUC.8372....5S
[358] http://www.konkoly.hu/cgi-bin/IBVS?5508
[359] http://adsabs.harvard.edu/abs/2004AAS...20515001S
[360] http://adsabs.harvard.edu/abs/2004AAS...20516503S
[361] http://adsabs.harvard.edu/abs/2004AAS...20515003S
[362] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.6004S&,db_key=AST&,high=4050e3f24431960
[363] http://adsabs.harvard.edu/abs/2004IAUC.8283....1S
[364] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.5606T&,db_key=AST&,high=4050e3f24406327
[365] http://adsabs.harvard.edu/abs/2004HEAD....8.1005W
[366] http://adsabs.harvard.edu/abs/2004HEAD....8.2422W
[367] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003AAS...203.4504Z&,db_key=AST&,high=3bc1f52f0207313
[368] http://adsabs.harvard.edu/abs/2005AAS...20711412A
[369] http://adsabs.harvard.edu/abs/2005AAS...207.7412A
[370] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0510091
[371] http://www.astronomerstelegram.org/?read=485
[372] http://www.astronomerstelegram.org/?read=468
[373] http://www.astronomerstelegram.org/?read=418
[374] http://adsabs.harvard.edu/abs/2005AAS...207.7425C
[375] http://adsabs.harvard.edu/abs/2005AAS...207.7006C
[376] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..2981....1C&,db_key=AST&,high=4050e3f24424696
[377] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3104....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a01113
[378] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3208....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a06525
[379] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3506....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a07846
[380] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3693....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10995
[381] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3694....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10995
[382] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3708....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10995
[383] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3729....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10995
[384] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3988....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10995
[385] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3994....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10995
[386] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..4142....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a10995
[387] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005GCN..3110....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a01113
[388] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...205.1901G&,db_key=AST&,high=3bc1f52f0222512
[389] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...20516507H&,db_key=AST&,high=4050e3f24424696
[390] http://www.aspbooks.org/a/volumes/article_details/?paper_id=2340
[391] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005AAS...20712406J&,db_key=AST&,da
[392] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...205.5502J&,db_key=AST&,high=4050e3f24431816
[393] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...205.7111K&,db_key=AST&,high=3bc1f52f0227067
[394] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0412089
[395] http://www.astronomerstelegram.org/?read=450
[396] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005ATel..628....1M&,db_key=AST&,data_type=HTML&,format=&,high=430c8dba7010746%22
[397] http://www.aspbooks.org/a/volumes/article_details/?paper_id=2399%22
[398] http://www.aspbooks.org/a/volumes/article_details/?paper_id=2211%22
[399] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...20516508P&,db_key=AST&,high=4050e3f24424696
[400] http://adsabs.harvard.edu/abs/2005DPS....37.5612R
[401] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2005AAS...207.6804R&,db_key=AST&,da
[402] http://adsabs.harvard.edu/abs/2005DPS....37.5614S
[403] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...20516509S&,db_key=AST&,high=4050e3f24424696
[404] http://www.aspbooks.org/a/volumes/article_details/?paper_id=1548
[405] http://adsabs.harvard.edu/abs/2005IBVS.5627....1S
[406] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...20516503S&,db_key=AST&,high=4050e3f24424696
[407] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...205.5501S&,db_key=AST&,high=4050e3f24406153
[408] http://adsabs.harvard.edu/abs/2005AAS...207.7023W
[409] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...205.9206W&,db_key=AST&,high=3bc1f52f0229652
[410] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004AAS...20516505W&,db_key=AST&,high=4050e3f24424696
[411] http://adsabs.harvard.edu/abs/2006AAS...208.4410A
[412] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ATel..855....1B&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a12321
[413] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ATel..869....1B&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a12321%22
[414] http://adsabs.harvard.edu/abs/2006DPS....38.4419B
[415] http://adsabs.harvard.edu/abs/2006ATel..966....1B
[416] http://adsabs.harvard.edu/abs/2006AAS...20921706C
[417] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..4618....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[418] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..4869....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[419] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..4872....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[420] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..4970....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[421] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..4972....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[422] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5111....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[423] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5180....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[424] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5259....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[425] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5323....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[426] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5362....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[427] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5495....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[428] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5497....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[429] http://gcn.gsfc.nasa.gov/gcn3/5734.gcn3
[430] http://gcn.gsfc.nasa.gov/gcn3/5878.gcn3
[431] http://gcn.gsfc.nasa.gov/gcn3/5935.gcn3
[432] http://gcn.gsfc.nasa.gov/gcn3/5938.gcn3
[433] http://gcn.gsfc.nasa.gov/gcn3/5961.gcn3
[434] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..4837....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[435] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5282....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[436] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5465....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[437] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006GCN..5525....1C&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a28100
[438] http://adsabs.harvard.edu/abs/2006AAS...208.2602F
[439] http://adsabs.harvard.edu/abs/2006IAUS..240E.158G
[440] http://adsabs.harvard.edu/abs/2006AAS...208.2601H
[441] http://adsabs.harvard.edu/abs/2006AAS...209.2404H
[442] http://adsabs.harvard.edu/abs/2006AAS...209.2907K
[443] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006AAS...20922806M&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a00575%22
[444] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ATel..712....1M&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a12321
[445] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ATel..706....1M&,db_key=AST&,data_type=HTML&,format=&,high=45632ee49a12321
[446] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0609051
[447] http://adsabs.harvard.edu/abs/2006AAS...20919606P
[448] http://adsabs.harvard.edu/abs/2006DPS....38.4004R
[449] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006IAUS..240E.137R&,db_key=AST&,da
[450] http://adsabs.harvard.edu/abs/2006IAUS..240E.178S
[451] http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006AAS...20910305S&,db_key=AST&,da
[452] http://adsabs.harvard.edu/abs/2007ATel.1109....1B
[453] http://adsabs.harvard.edu/abs/2007GCN..6236....1C
[454] http://adsabs.harvard.edu/abs/2007GCN..6296....1C
[455] http://adsabs.harvard.edu/abs/2007GCN..6347....1C
[456] http://adsabs.harvard.edu/abs/2007GCN..6391....1C
[457] http://www.aspbooks.org/a/volumes/article_details/?paper_id=4821
[458] http://adsabs.harvard.edu/abs/2007IAUS..240Q.330G
[459] http://adsabs.harvard.edu/abs/2007AAS...21113416H
[460] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0609112
[461] http://adsabs.harvard.edu/abs/2007ATel.1080....1M
[462] http://adsabs.harvard.edu/abs/2007ATel.1218....1M
[463] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0702115
[464] http://www.aspbooks.org/a/volumes/article_details/?paper_id=3360
[465] http://adsabs.harvard.edu/abs/2007AAS...211.4615M
[466] http://www.aspbooks.org/a/volumes/article_details/?paper_id=3958
[467] http://adsabs.harvard.edu/abs/2007IAUS..240..386S
[468] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0610946
[469] http://adsabs.harvard.edu/abs/2006AAS...20915616T
[470] http://adsabs.harvard.edu/abs/2007IAUC.8800....2W
[471] http://adsabs.harvard.edu/abs/2007ATel.1119....1W
[472] http://adsabs.harvard.edu/abs/2008AIPC.1010..174B
[473] http://adsabs.harvard.edu/abs/2008ATel.1751....1B
[474] http://adsabs.harvard.edu/abs/2008ATel.1746....1B
[475] http://adsabs.harvard.edu/abs/2008AIPC.1010...69C
[476] http://adsabs.harvard.edu/abs/2008IAUS..248..490C
[477] http://adsabs.harvard.edu/abs/2008ATel.1816....1H
[478] http://adsabs.harvard.edu/abs/2008AIPC.1053..201K
[479] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0707.3275
[480] http://adsabs.harvard.edu/abs/2008ATel.1778....1M
[481] http://adsabs.harvard.edu/abs/2008AIPC.1010...23M
[482] http://adsabs.harvard.edu/abs/2009ATel.2162....1B
[483] http://adsabs.harvard.edu/abs/2009ATel.2332....1B
[484] http://adsabs.harvard.edu/abs/2009ATel.2207....1B
[485] http://adsabs.harvard.edu/abs/2009ATel.2181....1B
[486] http://adsabs.harvard.edu/abs/2009ATel.2155....1B
[487] http://adsabs.harvard.edu/abs/2009ATel.1899....1B
[488] http://adsabs.harvard.edu/abs/2009AAS...21335206C
[489] http://adsabs.harvard.edu/abs/2009amos.confE..25C
[490] http://adsabs.harvard.edu/abs/2009ATel.2210....1D
[491] http://adsabs.harvard.edu/abs/2009ATel.2010....1M
[492] http://adsabs.harvard.edu/abs/2008IAUC.8951....3P
[493] http://adsabs.harvard.edu/abs/2009AAS...21332004S
[494] http://adsabs.harvard.edu/abs/2010ATel.2392....1B
[495] http://adsabs.harvard.edu/abs/2010ATel.2640....1B
[496] http://adsabs.harvard.edu/abs/2010ATel.2522....1B
[497] http://adsabs.harvard.edu/abs/2010ATel.2549....1B
[498] http://adsabs.harvard.edu//abs/2010AAS...21542416M
[499] http://adsabs.harvard.edu/abs/2010ATel.2507....1P
[500] http://adsabs.harvard.edu/abs/2010ATel.2660....1P
[501] http://adsabs.harvard.edu//abs/2010ATel.2560....1R
[502] http://adsabs.harvard.edu/abs/2010ATel.2547....1R
[503] http://adsabs.harvard.edu/abs/2011AAS...21822905B
[504] http://adsabs.harvard.edu/abs/2011ATel.3212....1B
[505] http://adsabs.harvard.edu/abs/2011ATel.3337....1B
[506] http://adsabs.harvard.edu/abs/2011ATel.3591....1C
[507] http://adsabs.harvard.edu/abs/2011AAS...21832702C
[508] http://gcn.gsfc.nasa.gov/gcn/gcn3/12081.gcn3
[509] http://adsabs.harvard.edu/abs/2011AAS...21840808I
[510] http://adsabs.harvard.edu/abs/2011AAS...21714420M
[511] http://adsabs.harvard.edu/abs/2011AAS...21714304M
[512] http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1010.4296
[513] http://adsabs.harvard.edu/abs/2011AAS...21712604R
[514] http://adsabs.harvard.edu/abs/2011AAS...21740801W
[515] http://www.noao.edu/credit.html