Contamination: Tie SMOV Stars to Cycle 7 Star

Details Contamination: Tie SMOV Stars to Cycle 7 Star Contamination: Tie SMOV Stars to Cycle 7 Star

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7805b&link_type=abstract

HST Proposal ID #7805

Physics

Hst Proposal Id #7805

Scientific paper

Because of the lack of a perfect flat field correction and because of positioning differences on the CCD in SMOV, apparent changes in sensitivity appear in the response to the fundamental pure hydrogen WD standard stars G191B2B and GD153. Now that the pointing procedures and thermal conditions have stabilized, observation of these stars are needed to tie the SMOV calibration to the GO era and to the new cycle7 monitoring star AGK+81D266.

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