Wf/pc SV Calibration Through Observation of Field of Stars

Details Wf/pc SV Calibration Through Observation of Field of Stars Wf/pc SV Calibration Through Observation of Field of Stars

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3236w&link_type=abstract

HST Proposal ID #3236

Physics

Hst Proposal Id #3236

Scientific paper

The objective of this calibration test is to observe a field of stars that will allow an adequate number of calibrated stars to appear in each CCD to efficiently produce an instrument-defined photmetric system for each filter. The selected field is in the outer regions of the globular clusters NGC 5139 Revised 1/9/90 by PStanley to expand out SEQ to avoid AFTER conflicts during transformation. Mod'ed by JAW 2 Sept 90 to do post flood cals. Modified 3/20/91 - Removed Internal Calibrations, removed monitoring sequence, removed UV filters, removed repeats.

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