CCD Geometric Distortion

Details CCD Geometric Distortion CCD Geometric Distortion

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hst..prop.9028m&link_type=abstract

HST Proposal ID #9028

Physics

Hst Proposal Id #9028

Scientific paper

The geometric distortion of the WFC and HRC detectors will be measured using multiple pointing observations of globular cluster 47 Tucanae thus imaging moderately dense stellar fields. Centroid position of stars will be used to tie down the geometric distortion to about 0.2 pixels across the field of each detector. These high quality baseline measurements of the distortion will be ideal for diagnosing any temporal variations in later calibration campaigns.

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