EDP Sciences Journals List
Free access article

Issue A&A Suppl. Ser.
Volume 116, Number 2, April_II 1996
Page(s) 367 - 371
DOI 10.1051/aas:1996119

Detection of scattered light in telescopes DOI: 10.1051/aas:1996119
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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