The Herschel galaxy reference survey

dc.creatorBoselli, Alessandro
dc.creatorgroup, the SPIRE extragalactic
dc.date2006-11-07
dc.date.accessioned2026-07-07T07:30:42Z
dc.date.available2026-07-07T07:30:42Z
dc.descriptionIn order to study the dust properties of different galaxies in the nearby Universe, the SPIRE extragalactic group selected a volume limited (15$<$ $D$ $<$25 Mpc), complete sample of 313 galaxies spanning the whole range in morphological type (from ellipticals to late-type spirals) and luminosity (8.5 $<$ log $L_H$ $<$ 12 L$_H\odot$, -22 $<$ $M_B$ $<$ -16) extracted from 2MASS, to be observed in guaranteed time with Herschel. The 250-360-520 $μ$m SPIRE data, combined with those collected at other frequencies, will be used to trace the dust properties of normal galaxies and provide a reference sample for studies at high redshift.
dc.descriptionProceeding of the SF2A (invited talk), Paris, 26-30/06/2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0611209
dc.identifierhttp://arxiv.org/abs/astro-ph/0611209
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118490
dc.subjectAstrophysics
dc.titleThe Herschel galaxy reference survey
dc.typetext

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