Galaxy formation & evolution: the far-ir/sub-mm view

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dc.creatorCirasuolo, M.
dc.creatorDunlop, J. S.
dc.date2008-10-07
dc.date.accessioned2026-07-07T10:08:26Z
dc.date.available2026-07-07T10:08:26Z
dc.descriptionWe review our current knowledge of the population of high-redshift sub-mm/mm galaxies, with particular emphasis on recent results from the SCUBA HAlf Degree Extragalactic Survey (SHADES). All available evidence indicates that these objects form the high-redshift, high-luminosity, high-mass tail of the dusty starforming galaxy population revealed at lower redshifts and luminosities by Spitzer. Current theoretical models of galaxy formation struggle to reproduce these extreme objects in the numbers indicated by current surveys.
dc.description8 pages, 5 figures, to appear in ASP Conference Series (Proceedings of the 1st Subaru International Conference "Panoramic Views of Galaxy Formation and Evolution", held in Hayama, Japan, 10-15 December 2007
dc.identifierhttps://arxiv.org/abs/0810.1290
dc.identifierhttp://arxiv.org/abs/0810.1290
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/170991
dc.subjectAstrophysics
dc.titleGalaxy formation & evolution: the far-ir/sub-mm view
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