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FIRBACK Far Infrared Survey with ISO: Data Reduction, Analysis and First Results

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arxiv astro-ph/9902122 v2 pith:JZUURD7N submitted 1999-02-08 astro-ph

Herve Dole , Guilaine Lagache , Jean-Loup Puget , Richard Gispert , H. Aussel , F.R. Bouchet , C. Ciliegi , D.L. Clements
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C. Cesarsky F-X Desert D. Elbaz A. Franceschini B. Guiderdoni M. Harwit R. Laureijs D. Lemke R. McMahon A.F.M. Moorwood S. Oliver W.T. Reach M. Rowan-Robinson M. Stickel
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keywords firbackinfraredresultsanalysisdatafirstmicronsreduction
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FIRBACK is one of the deepest cosmological surveys performed in the far infrared, using ISOPHOT. We describe this survey, its data reduction and analysis. We present the maps of fields at 175 microns. We point out some first results: source identifications with radio and mid infrared, and source counts at 175 microns. These two results suggest that half of the FIRBACK sources are probably at redshifts greater than 1. We also present briefly the large follow-up program.

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