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Extremely red galaxies in the Phoenix Deep Survey

A. M. Hopkins·J. Afonso·A. Georgakakis·M. Sullivan·B. Mobasher·L. E. Cram
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Abstract

The 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.

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A. M. Hopkins, J. Afonso, A. Georgakakis, M. Sullivan, B. Mobasher, L. E. Cram. 2003-09-04. Extremely red galaxies in the Phoenix Deep Survey. https://arxiv.org/abs/astro-ph/0309147

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