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TELESCOPE:   SOAR
SEMESTER:    2014B
CODE:        UNC
PI:          UNC
TITLE:       UNC
STARTDATE:   2014-10-23
ENDDATE:     2014-10-24
SUBMIT:      2014-10-21.14:40:15
OBSERVER:    Katie Eckert, David Stark, Ashley Bittner, Sheila Kannappan, Ryan Beauchemin
OBSERVEREM:  keckert@physics.unc.edu, dstark@physics.unc.edu, sheila@physics.unc.edu, abittner@live.unc.edu,beauchem@live.unc.edu
INSTITUTION: UNC
INSTRUMENT:  Goodman HTS
STARTDATE:   2014-10-23
FILTERS:     
GRATINGS:    400/1200/2100
OBJFILE:     targetlist_forsoar_102114.txt
FINDFILE:
FINDURL:
INSTRUCT.BOT We will require dome flats during our calibrations in the afternoon. We also need the image slicer to be installed if it is not already, and we will be using the ADC, both during calibrations and through the night. INSTRUCT.EOT Goodman_HTS.EOT