Limitations of SAM. UV light is not transmitted to the science imager, so SAM is "blind" in the U band. The correction in the B band is not so good, while the sky background in B is contaminated by the faint UV leakage of the B-filter. The SAM imager has a distortion that might affect image recombination if large dithers are used. Targets for laser operation must be defined in advance, reducing the flexibility. SAM can deliver poor resolution under unfavorable conditions.
The instrument setup form [5] must be filled to define the filters, one week before the run. SAM+SAMI have a filter wheel with 7 slots for the 3-inch square filters (normally loaded with Bessell B,V.R,I filters) and can also use the SOI filter wheel that has 5 positions for 4-inch square filters (e.g. Sloan g',r', i', z' or narrow-band). Any filters used at SOI can be also used with SAM. However, SAM has only one filter wheel, filters can be changed only during the day.
Think about the strategy. Do you need dithers? There are pros, cons, and restrictions (contact the support scientists to learn more). What is the worst acceptable image quality needed to reach your science goals? Do you need photometric standards? They can be observed rapidly in open loop. What binning to use in SAMI (usually 2x2, pixel 0.091 arcsec)? Think about a backup program (using SAM or other SOAR instrument) for the case of poor seeing or technical problems. Fill the instrument setup forms for your backup program, too.
Think -► propose -► prepare -► observe -► reduce the data -► publish!
Links
[1] http://www.ctio.noirlab.edu/soar/content/performance
[2] mailto:soarnight@ctio.noao.edu
[3] mailto:atokovinin@ctio.noao.edu
[4] mailto:cbriceno@ctio.noao.edu
[5] http://www.ctio.noao.edu/SOAR/Forms/INST/setup.php
[6] http://www.ctio.noirlab.edu/soar/sites/default/files/SAM/archive/sami-manual.pdf
[7] http://www.ctio.noao.edu/new/Telescopes/SOAR/Instruments/SAM/archive/sami-sw.pdf
[8] http://www.ctio.noirlab.edu/soar/content/reducing-your-sam-images