Wf/pc Sat OBSERVATION:LMC Young Cluster Photometry

Details Wf/pc Sat OBSERVATION:LMC Young Cluster Photometry Wf/pc Sat OBSERVATION:LMC Young Cluster Photometry

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3008w&link_type=abstract

HST Proposal ID #3008

Physics

Hst Proposal Id #3008

Scientific paper

The purpose of this calibration test is to provide realistic data for stellar photometry over a range of crowding. Two exposure series are taken with the telescope moved between them to test the effects of PSF variability over the field. The target is a moderately crowded field in NGC 1850 in the LMC. PSF exposures are taken in NGC 188, in Proposal 3013. 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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