Astron. Astrophys. Suppl. Ser. 134, 135-148
J.L. Starck 1 - A. Abergel 2 - H. Aussel 1 - M. Sauvage 1 - R. Gastaud 1 - A. Claret 1 - X. Desert 2 - C. Delattre 1 - E. Pantin 1
Send offprint request: jstarck@cea.fr
1 - DAPNIA/SEI-SAP, CEA-Saclay, 91191 Gif-sur-Yvette Cedex,
France
2 -
IAS, Université Paris-Sud, Bât. 121, 91405 Orsay Cedex, France
Received November 12, 1997; accepted July 8, 1998
The ISOCAM infrared camera is one of the four instruments on board the
ISO (Infrared Space Observatory) spacecraft which was launched
successfully on 1995 November 17. It operates in the 2.5 - 18 m
range, and was developed by the ISOCAM consortium lead by the French
Service d'Astrophysique of CEA Saclay. This paper presents different
algorithms which can be used for the calibration of ISOCAM data.
Advantages and limitations of each method are also outlined. A range
of examples illustrates the results.
Key words: methods: data analysis -- instrumentation: interferometers -- infrared: general
Copyright The European Southern Observatory (ESO)