Back to Observer_Setup_Calendar_
TELESCOPE:   SOAR
SEMESTER:    2018B
CODE:        0095
PI:          J. Allyn Smith
TITLE:       Targeted Samples of the Hot Stellar Content in the Southern Sky
STARTDATE:   2018-09-28
ENDDATE:     2018-10-02
SUBMIT:      2018-09-18.19:54:22
OBSERVER:    Sahar Allam and Douglas Tucker
OBSERVEREM:  sallam@fnal.gov, dtucker@fnal.gov
INSTITUTION: NOAO
INSTRUMENT:  Goodman HTS
STARTDATE:   2018-09-28
CAMERA:      Blue Camera
GRATINGS:    400
FILTERS:     None
OBJFILE:     
FINDFILE:
FINDURL: http://data.darkenergysurvey.org/public_calib/DESCalibObsRuns/SOAR-Sep2018/Targets/WhiteDwarfCandidates/ssawdcat.desfootprint.round13.html
INSTRUCT.BOT We request the Blue camera and the WD_400 grating configuration for our program. In detail, this is the setup we request: --------------------------------------------------- Camera: Blue CCD ROI Mode: Spectroscopic, 2x2 CCD Read: 200kHz ATTN 2 Mask: 1-arcsec slit Grating: 400lines/mm ("SYZY_400") Set Mode: 400_WD (400lines/mm, set for c. 3500A-7500A, and scattered light feature moved to c. 3600A) --------------------------------------------------- The main target list can be found here: http://data.darkenergysurvey.org/public_calib/DESCalibObsRuns/SOAR-Sep2018/Targets/WhiteDwarfCandidates/ssawdcat.desfootprint.round13.goodman_targetlist.txt The corresponding Finding Chart URL can be found here: http://data.darkenergysurvey.org/public_calib/DESCalibObsRuns/SOAR-Sep2018/Targets/WhiteDwarfCandidates/ssawdcat.desfootprint.round13.html Both will likely be updated in the days before the start of the run. We will be observing remotely from Fermilab. Since this program uses an almost identical setup as for our gravitational wave optical counterpart target-of-opportunity follow-up program (PI: Marcelle Soares-Santos), we will also take the opportunity during this run to train some observers for that program. (The observers being trained will also be observing remotely with us at Fermilab.) INSTRUCT.EOT Goodman_HTS.EOT