UVIS Fringing

Physics

Scientific paper

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Scientific paper

Multiple pointing observations of the globular cluster Omega Centauri {NGC 5139} in the narrow band filters F656N and F953N will be used to verify the fringing model developed during various tests {TV3} and its impact on photometric accuracy. By measuring the relative changes in brighteness of a star at different positions on the detector, we will determine the local variations induced by the fringing pattern.;

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