Titlebook: Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow; 3-28 August 1998 F. Casoli,J. Lequeux,F

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Data Analysis with ISOCAM,1995 November 17 and ended its life in May, 1998. It operated in the 2.5 – 18 μm range, and was developed by the ISOCAM consortium lead by the French Service d’Astrophysique of CEA Saclay. This paper reviews different algorithms which can be used for the calibration and analysis of ISOCAM data.

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ISO Observations of Solar-System Objects,te have been performed on all classes of solar-system objects. Several important discoveries have been achieved, in particular with the Short-Wavelength Spectrometer. In spite of difficult observability constraints, spectra of Mars have been recorded with SWS and LWS. They have been used for a retri

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Stars and Galactic Structure,branches away from the main sequence; what white dwarfs and red giants are and why these differ from main-sequence stars; what the atomic abundances are and how stars make atoms heavier than helium: such questions have occupied the minds of astrophysicists in the first 2/3 of this century and the sa

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Normal Galaxies in the Infrared,nosity distribution. In such galaxies, the visible and ultraviolet is the only direct window onto the photospheres of stars, whereas the rest of the spectrum reflects reprocessed light from stars (Fig. 1). Dust in the interstellar medium reprocesses part of the stellar luminosity into infrared emiss