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 μJy are measured.
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Hopkins, A., Afonso, J., Georgakakis, A., Sullivan, M., Mobasher, B., Cram, L. The Phoenix Deep Survey: Evolution of Star Forming Galaxies. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_6
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DOI: https://doi.org/10.1007/10995020_6
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-25665-6
Online ISBN: 978-3-540-31641-1
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