TY  - STD
AU  - Crouzet N, Guillot T.
PY  - 2007//
TI  - Front- vs. back-illuminated CCD cameras for photometric surveys: a noise budget analysis
PB  - WILEY-VCH Verlag
KW  - instrumentation: detectors
KW  - methods: numerica
KW  - technique: photometric
KW  -
N2  - Abstract : Exoplanetary transit and stellar oscillation surveys require a very high precision photometry. The instrumental noise has therefore to be minimized. First, we perform a semi-analytical model of different noise sources. We show that the noise due the CCD electrodes can be overcome using a Gaussian PSF (Point Spread Function) of full width half maximum larger than 1.6 pixels. We also find that for a PSF size of a few pixels, the photometric aperture has to be at least 2.5 times larger than the PSF full width half maximum. Then, we compare a front- with a back-illuminated CCD through a Monte-Carlo simulation. Both cameras give the same results for a PSF full width half maximum larger than 1.5 pixels. All these simulations are applied to the A STEP (Antarctica Search for Transiting Extrasolar Planets) project. As a result, we choose a front-illuminated camera for A STEP because of its better resolution and lower price, and we will use a PSF larger than 1.6 pixels. (© 2007 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)
SN  - 1521-3994
UR  - http://dx.doi.org/10.1002/asna.200710820
N1  - exported from refbase (http://publi.ipev.fr/polar_references/show.php?record=1585), last updated on Fri, 05 Jul 2024 22:35:59 +0200
ID  - CrouzetN2007
ER  -