WFC3/UVIS external and internal CTE monitor

Details WFC3/UVIS external and internal CTE monitor WFC3/UVIS external and internal CTE monitor

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11924k&link_type=abstract

HST Proposal ID #11924. Cycle 17

Astronomy and Astrophysics

Astronomy

Scientific paper

CCD detector Charge Transfer Inefficiency {CTI} induced losses in photometry and astrometry will be measured using observations of the rich open cluster NGC6791 and with the EPER {Extended Pixel Edge Response} method using tungsten lamp flat field exposures. Although we do not expect to see CTE effects at the outset of Cycle 17, this CTE monitoring program is the first of a multi-cycle program to monitor and establish CTE-induced losses with time. We expect to measure CTE effects with a precision comparable to the ACS measurements.;

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