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

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dc.creatorDole, Herve
dc.creatorLagache, Guilaine
dc.creatorPuget, Jean-Loup
dc.creatorGispert, Richard
dc.creatorAussel, H.
dc.creatorBouchet, F. R.
dc.creatorCiliegi, C.
dc.creatorClements, D. L.
dc.creatorCesarsky, C.
dc.creatorDesert, F-X
dc.creatorElbaz, D.
dc.creatorFranceschini, A.
dc.creatorGuiderdoni, B.
dc.creatorHarwit, M.
dc.creatorLaureijs, R.
dc.creatorLemke, D.
dc.creatorMcMahon, R.
dc.creatorMoorwood, A. F. M.
dc.creatorOliver, S.
dc.creatorReach, W. T.
dc.creatorRowan-Robinson, M.
dc.creatorStickel, M.
dc.date1999-02-08
dc.date1999-03-04
dc.date.accessioned2026-07-07T02:30:22Z
dc.date.available2026-07-07T02:30:22Z
dc.descriptionFIRBACK 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.
dc.descriptionsmall cosmetic changes: 5 pages, 5 figures, to appear in the ISO conference "The Universe as seen by ISO", 1998, UNESCO, Paris; also available at http://wwwfirback.ias.fr
dc.identifierhttps://arxiv.org/abs/astro-ph/9902122
dc.identifierhttp://arxiv.org/abs/astro-ph/9902122
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13791
dc.subjectAstrophysics
dc.titleFIRBACK Far Infrared Survey with ISO: Data Reduction, Analysis and First Results
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