Notes et articles sur la correction des transitoires de la caméra infrarouge LW-CAM embarquée sur le satellite ISO
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Cette liste est partielle. Manque au moins : ceci et le
livre ISO-CAM et un article sur le traitement de cartes
Spitzer 180 um présenté au GRETSI 2005 (Th. Rodet et al.).
Documentation en français :
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Correction des transitoires de la caméra infrarouge du satellite ISO
A. Coulais & A. Abergel
vol. T-1, GRETSI'1999, Septembre 1999, pp. 147-150
HTML, Dvi, Gzip-PostScript (294 Ko), PDF (437 ko)
Résumé : ce papier en français présente brièvement les résultats obtenus pour modéliser et corriger les effets transitoires (rémanence)
de la caméra infrarouge ISO CAM.
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Correction par bloc des transitoires de la cam éra infrarouge ISOPHOT C-100 avec un modèle non linéaire dissymétrique
A. Coulais, J.-F. Giovannelli, J. See, F. Balleux et A. Abergel
GRETSI'2001, Septembre 2001
HTML, Dvi, Gzip-PostScript (54 Ko), PDF(113 Ko)
Résumé : A propos du modèle et de la méthode de correction bloc par bloc développés pour PHOT C-100.
Documentation en anglais :
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Transient correction of the ISOCAM data with the Fouks-Schubert model: first results
A. Coulais & A. Abergel
The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427, October 1998.
HTML, Dvi, Gzip-PostScript (420 Ko), PDF (384 Ko)
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Local summary : Short introduction to the use of one of the Fouks model to ISOCAM data.
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Transient correction of the LW-ISOCAM data for low contrasted illumination
A. Coulais & A. Abergel
Astronomy and Astrophysics Supplement Serie, vol. 141, February 2000, pp. 533-544.
HTML, Dvi, Gzip-PostScript (420 Ko), PDF (384 Ko)
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Local summary : Full explanation of the use of one of the Fouks model to ISOCAM data.
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Transient response of IR detectors used in space astronomy : what we have learned from ISO satellite
A. Coulais, B. Fouks, J.-F. Giovannelli, A. Abergel, and J. Sée
Infrared Spaceborne Remote Sensing VIII, S. M. and A. B., eds.,
vol. 4131, San Diego, USA, August 2000, SPIE, pp. 205-217.
HTML, Dvi, Gzip-PostScript (120 Ko), PDF (356 Ko)
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Local summary : The paper summarizes the state of the art of transient models for most of the ISO detectors,
contains a first version of a model for CAM point source transient, gives somes indications about block by
block transient correction, from a general point of view but also in the specific case of PHOT C-100.
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Current status of modeling of point sources transient response for LW-ISOCAM
A. Coulais & B. Fouks
Conference : The Calibration Legacy of the ISO Mission, VILSPA, Spain,
February 2001 (ESA SP-481)
HTML, Dvi, Gzip-PostScript (114 Ko), PDF (345 Ko)
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Local summary : This paper summarizes the state of the art of transient models for CAM point source transient
in Feb. 2001. Some interesting examples are shown. The new model, developped at the end of 2001, is described here !
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Transient correction for ISOPHOT C-100 detector
A. Coulais, J. See, J.-F. Giovannelli, B. Stepnik F. Balleux & A. Abergel
Conference : The Calibration Legacy of the ISO Mission, VILSPA, Spain,
February 2001 (ESA SP-481)
HTML, Dvi, Gzip-PostScript (210 Ko), PDF (594 Ko)
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Local summary : Devoted on extensive processing of PHOT C-100 data with the block by block decribed previously,
this paper explains the problems we have encoutered during the processing of these PHOT C-100 data sets, and how to check
if the observing modes are OK or not.
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The importance of ground based tests for space experiments using low background IR photodetectors
A. Coulais & A. Abergel
Conference : The Calibration Legacy of the ISO Mission, VILSPA, Spain,
February 2001 (ESA SP-481)
HTML, Dvi, Gzip-PostScript (38 Ko), PDF (147 Ko)
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Local summary : This paper reviews the behavior of most of the ISO systems (CAM, PHT, LWS and SWS) and detectors.
Several possible causes of problems are considered, in optical, electronical and detectors sub-systems. We explain that,
since the transients are reproducible and the glitches (related to hit of high energetic particles), if all other parts
(optical, electonic, temperature control, ...) are without missconception, the transient models ensure that glitches
appear to be the only limiting factor. We explain also how to check such whole system with the help of the detector
transients during ground based tests. This paper may be useful for any team currently involved with development of such
system.
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Transient effects of IR photodetectors: the lessons from ISO
A. Coulais, A. Abergel & B. Fouks
Conference : Far-Infrared, Sub-MM and MM Detector Workshop, Monterey, CA, USA
1-3 April 2002
Wolf J., Farhoomand J. and McCreight C.R. (eds.), NASA/CP-211408, 2002
HTML, Dvi, Gzip-PostScript (146 Ko), PDF (139 Ko)
Les autres manuscripts de cette session sont
accessibles en ligne
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Local summary : This paper is an overview of transient models for most Si:Ga and Ge:Ga detectors on-board the ISO
satellite. We focused on the applications of physical models provided by Fouks' theory. This paper should be useful for
SIRTF (MIPS), Astro-F (FIR) and Herschel satellites to begin as soon as possible to consider the use of physical models
in order to remove the transient effects in they Ge:Ga detectors.
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Frequently--Ask Questions about Fouks models and transient correction methods for LW-ISOCAM
A. Coulais & A. Abergel
Conference : Exploiting the ISO Data Archive - Infrared Astronomy in the Internet Age, Parador de Siguenza, Spain
24-27 June 2002 (ESA SP-511)
HTML, Dvi, Gzip-PostScript (30 Ko), PDF (92 Ko)
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Local summary : The goal of this paper was to recall the limitations of the model and of the correction method
for ISOCAM, after 4 years of sucessful use.
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Accurate physical model for direct modeling of point source transients for ISOCAM LW detector
B. Fouks, A. Coulais & J. Normand
Conference : Exploiting the ISO Data Archive - Infrared Astronomy in the Internet Age, Parador de Siguenza, Spain
24-27 June 2002 (ESA SP-511)
HTML, Dvi, Gzip-PostScript (211 Ko), PDF (333 Ko)
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Local summary : This paper presents briefly the current status of the modelization of point source transients
for ISOCAM (Si:Ga detector). Even the model is highly accurates, the correction method is not trivial. We show
adjustements and explain the limits of the new model for point sources and of the current correction method.
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Non-linear transient models and transient corrections methods for IR low-background photo-detectors
A. Coulais, J. Malaizé, J.-F. Giovannelli, T. Rodet, A. Abergel, B. Wells, M. Patrashin, H. Kaneda & B. Fouks
Conference : Astronomical Data Analysis Software and Systems (ADASS) XIII
Conference held 12-15 October, 2003 in Strasbourg, France.
Edited by Francois Ochsenbein, Mark G. Allen and Daniel Egret.
12-15 October, 2003 (ASP Conference Proceedings, Vol. 314. San Francisco: Astronomical Society of the Pacific, 2004., p.566ASP SP-511).
HTML, Dvi, Gzip-PostScript (92 Ko), PDF (176 Ko)
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Local summary : This paper presents briefly the current progress of the modelization of Si:Ga and Ge:Ga detectors.
Published summary