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The Phoenix Deep Survey: A Deep Microjansky Radio Survey | | J. Afonso
; B. Mobasher
; A. Hopkins
; L. Cram
; | | Date: |
5 Sep 1999 | | Subject: | astro-ph | | Affiliation: | Imperial College), B. Mobasher (Imperial College), A. Hopkins (Australia Telescope National Facility), L. Cram (University of Sydney | | Abstract: | The study of the nature of faint radio sources is of great importance since a significant fraction of these objects is thought to be composed of actively star-forming galaxies. Due to the increased sensitivity of radio telescopes, we are now not only able to catalogue large numbers of these sources in the sub-millijansky regime, but also to start the study of the nature of increasingly fainter microjansky sources. This paper presents a new very deep 1.4 GHz radio survey made as a part of the Phoenix Deep Survey, a project aimed to study the nature of the faintest radio sources. With a limiting sensitivity of 45 microJy, this new survey has allowed us to assemble a large number of sources with 1.4 GHz flux densities below 100 microJy. The resulting source counts and the analysis of the optical properties of the faintest radio sources are presented. | | Source: | arXiv, astro-ph/9909095 | | Services: | Forum | Review | PDF | Favorites | |
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