Wf/pc SV Calibration Through Observation of Field of Stars - Son of 1321 8/27/90

Details Wf/pc SV Calibration Through Observation of Field of Stars - Son of 1321 8/27/90 Wf/pc SV Calibration Through Observation of Field of Stars - Son of 1321 8/27/90

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3053w&link_type=abstract

HST Proposal ID #3053

Physics

Hst Proposal Id #3053

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 fields lie in the outer regions of the globular clusters NGC 5139 and NGC 6752. Ground-based measurements of these fields have been made with a detector and filter set identical to the WF/PC. Revised 11/8/89 by PStanley to correct Cycle 0 line list. Revised 1/9/90 by PStanley to expand out SEQ to avoid AFTER conflicts during transformation.

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