Next: Introduction
Ivan K. Baldry
Timothy R. Bedding
Hans Kjeldsen
Chatterton Astronomy Dept, School of Physics, University of Sydney,
NSW 2006
Anglo-Australian Observatory, P.O.Box 296, Epping, NSW 1710
Institute of Physics and Astronomy, University of Aarhus,
DK-8000 Aarhus C, Denmark
Abstract:
CCDs can deviate significantly from being linear detectors. We
describe methods of accurately determining non-linearities, so that
corrections can be applied to CCD data. Two CCDs that have been
used on the 74inch Telescope at Mt. Stromlo Observatory are used
as examples. They have a 5% and a 1.5% change in gain between 0
and 40000 ADU, which can degrade astronomical results if not
corrected for.
Keywords:
instrumentation: detectors -- techniques: image processing
Ivan Baldry
2005-05-23