Extremely red galaxies in the Phoenix Deep Survey
Astrophysics
2007-05-23 v1
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.
Keywords
Cite
@article{arxiv.astro-ph/0309147,
title = {Extremely red galaxies in the Phoenix Deep Survey},
author = {A. M. Hopkins and J. Afonso and A. Georgakakis and M. Sullivan and B. Mobasher and L. E. Cram},
journal= {arXiv preprint arXiv:astro-ph/0309147},
year = {2007}
}
Comments
4 pages, 3 figures, "Multiwavelength Cosmology" Mykonos, June 2003, conference proceedings