Wf/pc Sat Observation: Crowded Field Photometry in AN Intermediate-Distance Cepheid Galaxy

Details Wf/pc Sat Observation: Crowded Field Photometry in AN Intermediate-Distance Cepheid Galaxy Wf/pc Sat Observation: Crowded Field Photometry in AN Intermediate-Distance Cepheid Galaxy

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3010w&link_type=abstract

HST Proposal ID #3010

Physics

Hst Proposal Id #3010

Scientific paper

The purpose of this calibration test is to take data of known crowded star fields and determine the effects on standard automatic data reduction programs. The data will be taken in at two wavelength extremes to isolate the point spread function dependency for this analysis. The PSF must be measured once per WF/PC SAT "campaign" or if the mirror position has changed or more than 7 days have passed since the last calibration.

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