Sat/hsp 2: Effect of Jitter on Hsp Photometry

Details Sat/hsp 2: Effect of Jitter on Hsp Photometry Sat/hsp 2: Effect of Jitter on Hsp Photometry

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3007w&link_type=abstract

HST Proposal ID #3007

Physics

Hst Proposal Id #3007

Scientific paper

Using a bright target in the CVZ from the HSP SV program which measures the short-term photometric stability of the HSP (SV 1389), the effect of FGS jitter on HSP photometry is determined by taking a 1 hour time series on the target in a 1-arcsec science aperture. The test is performed for two apertures on the UV1 detector and one on the POL detector. This test must be preceeded by the aperture location calibration (OV 1504) and the SV target acquisition test (SV 1381). This test must preceed SV 1389. This may be run optionally at any time, to assess the current state of HST jitter, but MUST be run after the final jitter fix is in in order to estimate the effect of permanent residual jitter on HSP science observations. Revision history: created by R. White 12 July 1990 jwp&apple, change VIS to UV1. jwp, 07 Jan 1991, minor fixes

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