CTE measurement and photometric accuracy for extended sources

Details CTE measurement and photometric accuracy for extended sources CTE measurement and photometric accuracy for extended sources

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003hst..prop10038m&link_type=abstract

HST Proposal ID #10038

Computer Science

Hst Proposal Id #10038

Scientific paper

This is a follow-up study to proposal 8839 to study STIS CTE calibration for extended objects. This takes images of galaxies to measure the effects of CTE on the isophotes of galaxies. The aim is to image small {2-3"} extended sources in a suitably rich galaxy cluster. The target, A1689, has been observed by WFPC2 in the WF2 and WF4 chips {in Feb 2000}, so that cross-instrument comparison will be straightforward. One orbit is needed per amplifier, i.e. two orbits total.

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