Far-Infrared Source Counts and the Diffuse Infrared Background

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dc.creatorPuget, Jean-Loup
dc.creatorLagache, Guilaine
dc.date2001-01-08
dc.date.accessioned2026-07-07T01:57:17Z
dc.date.available2026-07-07T01:57:17Z
dc.descriptionThe cosmic far-infrared background is now well measured from 140 micron to 1 mm. Uncertainties remain at 100 micron (and even more at 60 micron). These are dominated by limitations of the zodiacal model. The nature of sources dominating the background near its maximum are beginning to be studied through deep surveys carried out with ISOPHOT. These surveys show very steep number counts and fluctuations of the background due to unresolved sources.
dc.descriptionTo appear in ASP Conference Series, (IAU 204, Extragalactic IR background)
dc.identifierhttps://arxiv.org/abs/astro-ph/0101105
dc.identifierhttp://arxiv.org/abs/astro-ph/0101105
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2330
dc.subjectAstrophysics
dc.titleFar-Infrared Source Counts and the Diffuse Infrared Background
dc.typetext

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