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Astronomy and Astrophysics Supplement Series, Vol. 116, No. 3, April 1996, 367-371
Detection of scattered light in telescopes
F. Grundahl and A.N. Sørensen
Send offprint requests to: F. Grundahl; fgj@obs.aau.dk
Institute of Physics and Astronomy, University of Aarhus, DK-8000 Århus C, Denmark
Received August 29; accepted September 25, 1995
Abstract:
We present a simple, but powerful method to test for the presence of scattered light in telescopes. Scattered light can seriously hamper any attempt to achieve a proper flat fielding of CCD data. The method consists of making a pinhole camera (camera obscura) by placing a pinhole mask in front of the CCD window. Exposing the CCD in this configuration gives an image of the light sources in the optical path. Tests made at the Nordic Optical Telescope have led to a reduction of large scale flat field variations due to scattered light from a total of
5% to
below 1% by improving the telescope baffles.
Key words: instruments: miscellaneous --- telescopes
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