Extremely red galaxies in the Phoenix Deep Survey

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dc.creatorHopkins, A. M.
dc.creatorAfonso, J.
dc.creatorGeorgakakis, A.
dc.creatorSullivan, M.
dc.creatorMobasher, B.
dc.creatorCram, L. E.
dc.date2003-09-04
dc.date.accessioned2026-07-07T02:09:25Z
dc.date.available2026-07-07T02:09:25Z
dc.descriptionThe Phoenix Deep Survey (PDS) is a multiwavelength survey based on deep 1.4 GHz radio observations used to identify a large sample of star forming galaxies to z=1. Here we present an exploration of the evolutionary constraints on the star-forming population imposed by the 1.4 GHz source counts, followed by an analysis of the average properties of extremely red galaxies in the PDS, by using the "stacking" technique.
dc.description4 pages, 3 figures, "Multiwavelength Cosmology" Mykonos, June 2003, conference proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0309147
dc.identifierhttp://arxiv.org/abs/astro-ph/0309147
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6427
dc.subjectAstrophysics
dc.titleExtremely red galaxies in the Phoenix Deep Survey
dc.typetext

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