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The Phoenix Deep Survey: Evolution of Star Forming Galaxies

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. Photometric redshifts are estimated for the optical counterparts to the radio-detected galaxies, and their uncertainties quantified by comparison with spectroscopic redshift measurements. The photometric redshift estimates and associated best-fitting spectral energy distributions are used in a stacking analysis exploring the mean radio properties of U-band selected galaxies. Average flux densities of a few microJy are measured.

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A. M. Hopkins, J. Afonso, A. Georgakakis, M. Sullivan, B. Mobasher, L. E. Cram. 2003-12-01. The Phoenix Deep Survey: Evolution of Star Forming Galaxies. https://arxiv.org/abs/astro-ph/0312035

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