Extremely red galaxies in the Phoenix Deep Survey

(2) University of Lisbon; (3) National Athens Observatory; (4) University of Durham; (5) STScI; (6) Australian Research Council); A. Georgakakis (3); A. M. Hopkins (1); B. Mobasher (5); J. Afonso (2); L. E. Cram (6) ((1) University of Pittsburgh

arxiv: astro-ph/0309147 · v1 · submitted 2003-09-04 · 🌌 astro-ph

Extremely red galaxies in the Phoenix Deep Survey

A. M. Hopkins (1) , J. Afonso (2) , A. Georgakakis (3) , M. Sullivan (4) , B. Mobasher (5) , L. E. Cram (6) ((1) University of Pittsburgh , (2) University of Lisbon , (3) National Athens Observatory

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(4) University of Durham (5) STScI (6) Australian Research Council)

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keywords deepgalaxiessurveyextremelyphoenixanalysisaverageconstraints

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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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Extremely red galaxies in the Phoenix Deep Survey

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