Reference : Modelling the Fringing of the FORS2 CCD
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/108059
Modelling the Fringing of the FORS2 CCD
English
Walsh, J. R. [ESA, Space Telescope European Co-ordinating Facility, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany]
Kuntschner, H. [ESO, Alonso de Cordóva 3107, Vitacura, Santiago, Chile]
Jehin, Emmanuel mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image]
Kaufer, A. [ESO, Alonso de Cordóva 3107, Vitacura, Santiago, Chile]
O'Brien, K. [ESO, Alonso de Cordóva 3107, Vitacura, Santiago, Chile]
Riquelme, M. [ESO, Alonso de Cordóva 3107, Vitacura, Santiago, Chile]
Smette, A. [> > > >]
Kerber, Florian [> > > >]
2008
The 2007 ESO Instrument Calibration Workshop
Kaufer, A.
Springer-Verlag
ESO ASTROPHYSICS SYMPOSIA
63
Yes
No
International
978-3-540-76962-0
Heidelberg
Germany
The 2007 ESO Instrument Calibration Workshop
23-26 January 2007
Andreas Kaufer, Florian Kerber, R Hanuschik, F Patat, M Peron, M Romaniello, M Sterzik
Garching
Germany
[en] Thinned CCD detectors display fringing which arises from the interference of multiply reflected light in the layers of the CCD. If the layer construction - the thicknesses and refractive indexes of the layers - is known, then the observed fringing can be accurately modelled and used to correct imaging and spectroscopic data for its effects. In practice the specifications on the actual deposited layer thicknesses may not be known to sufficient accuracy to predict the fringe behaviour. Thus calibration data, in the form of monochromatic flat fields, is required and can be modelled using the technique outlined by Malamuth et al. 2003, which has been applied to ACS CCDs.
Researchers
http://hdl.handle.net/2268/108059
10.1007/978-3-540-76963-7_9
http://adsabs.harvard.edu/abs/2008eic..work...63W

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