A local infrared perspective to deeper ISO surveys

dc.creatorAlexander, D. M.
dc.creatorAussel, H.
dc.date2000-02-09
dc.date.accessioned2026-07-07T01:52:12Z
dc.date.available2026-07-07T01:52:12Z
dc.descriptionWe present new techniques to produce IRAS 12 micron samples of galaxies and stars. We show that previous IRAS 12 micron samples are incompatible for detailed comparison with ISO surveys and review their problems. We provide a stellar infrared diagnostic diagram to distinguish galaxies from stars without using longer wavelength IRAS colour criteria and produce complete 12 micron samples of galaxies and stars. This new technique allows us to estimate the contribution of non-dusty galaxies to the IRAS 12 micron counts and produce a true local mid-infrared extragalactic sample compatible with ISO surveys. We present our initial analysis and results.
dc.description8 pages, 3 figures, to be published in the Springer Lecture Notes of Physics Series as part of the proceedings for "ISO Surveys of a Dusty Universe," a workshop held at Ringberg Castle, Germany, November 8 - 12, 1999. Requires latex style files for this series: cl2emult.cls, cropmark.sty, lnp.sty, sprmindx.sty, subeqnar.sty (included with submission)
dc.identifierhttps://arxiv.org/abs/astro-ph/0002200
dc.identifierhttp://arxiv.org/abs/astro-ph/0002200
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/546
dc.subjectAstrophysics
dc.titleA local infrared perspective to deeper ISO surveys
dc.typetext

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