The Phoenix Deep Survey: Evolution of Star Forming Galaxies
| dc.creator | Hopkins, A. M. | |
| dc.creator | Afonso, J. | |
| dc.creator | Georgakakis, A. | |
| dc.creator | Sullivan, M. | |
| dc.creator | Mobasher, B. | |
| dc.creator | Cram, L. E. | |
| dc.date | 2003-12-01 | |
| dc.date.accessioned | 2026-07-25T19:12:18Z | |
| dc.description | 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. | |
| dc.description | 6 pages, 3 figures, in "Multiwavelength Mapping of Galaxy Formation and Evolution" Venice, October 2003, conference proceedings | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0312035 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0312035 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/62471 | |
| dc.subject | Astrophysics | |
| dc.title | The Phoenix Deep Survey: Evolution of Star Forming Galaxies | |
| dc.type | text |