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Effects of Shutter Timing on CCD Photometry

Published online by Cambridge University Press:  07 August 2017

D. Galadí-Enríquez
Affiliation:
Dept. d'Astronomia i Meteorologia, Universitat de Barcelona
C. Jordi
Affiliation:
Dept. d'Astronomia i Meteorologia, Universitat de Barcelona
E. Trullols
Affiliation:
Dept. d'Astronomia i Meteorologia, Universitat de Barcelona

Extract

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CCD-shutters take some time to open and close. This results in a difference between the recorded and real exposure times. The pixel-to-pixel pattern δ(x, y) in which this difference varies depends on the characteristics of the device. These timing errors affect photometric measurements in two ways: directly, since the recorded exposure time is not the real one, and indirectly, via the flatfielding process, because the shutter effect is mixed up with the flatfield pattern. The direct effect may be negligible when exposure times are long. The indirect effect is present irrespective of the exposure times of the frames, if flatfield exposure times are short.

Type
Section II — Poster Papers
Copyright
Copyright © Kluwer 1995 

References

Stetson, P. B. 1989 Highlights of Astronomy 8, 635.Google Scholar
Surma, P. 1993 A&A 278, 654.Google Scholar