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TELESCOPE:   SOAR
SEMESTER:    2016B
CODE:        146012990104
PI:          Kalari
TITLE:       Stellar initial mass function and metallicity of the Magellanic Bridge cluster NGC796
STARTDATE:   2016-11-05
ENDDATE:     2016-11-05
SUBMIT:      2016-10-27.10:26:08
OBSERVER:    Kalari
OBSERVEREM:  venukalari@gmail.com
INSTITUTION: Chile
INSTRUMENT:  SAMI
STARTDATE:   2016-11-05
FILTERS:     BVRIHalpha
OBJFILE:     SAMI_targets.txt
FINDFILE: charts.zip
FINDURL:
INSTRUCT.BOT The targets (open clusters at 60 kpc) span the magnitude range 13-25, but fit inside a 3arcmin square FoV. We plan exposures in BVRI and Halpha for our science. We plan to use the 4 square wheel with 5 slots. The exposure times planned are 0.1, 1, 10, 100, 200, 200x6 to span the magnitude range requested. Longer exposures in Halpha are requested. We estimate at least 2 hours per target with our exposure times in all filters. In total we (optimistically) estimate we can observe 4-5 targets in the night. We also request standard photometric standards for calibration. We mark our targets in order of priority. INSTRUCT.EOT SAMI.EOT