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The Phoenix radio survey: the angular correlation function
A. Georgakakis, B. Mobasher, L. Cram +2
Using the Phoenix radio survey, a homogeneous survey selected at 1.4GHz and covering an area of ~3deg^2, we analyse the clustering of the sub-mJy radio population using angular cor…
The Phoenix survey: the pairing fraction of faint radio sources
A. Georgakakis, B. Mobasher, L. Cram +1
The significance of tidal interactions in the evolution of the faint radio population (sub-mJy) is studied using a deep and homogeneous radio survey (1.4 GHz), covering an area of…
The Behind The Plane Survey
Will Saunders, Kenton d'Mellow, Brent Tully +7
We have extended the PSCz to cover 93% of the sky, the practical limit for any catalogue based on the Point Source Catalog. The galaxy identifications are complete, and the core of…
The Phoenix Deep Survey: A Deep Microjansky Radio Survey
J. Afonso, B. Mobasher, A. Hopkins +1
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…
The Phoenix survey: optical and near-infrared observations of faint radio sources
A. Georgakakis, B. Mobasher, L. Cram +3
Using a deep Australia Telescope Compact Array (ATCA) radio survey covering an area of ~3deg^{2} to a 4σsensitivity of \ge 100 \muJy at 1.4GHz, we study the nature of faint radio g…
Stellar Population of Ellipticals in Different Environments: Near-infrared Spectroscopic Observations
Philip James, Bahram Mobasher
Near-infrared spectra of 50 elliptical galaxies in the Pisces, A2199 and A2634 clusters, and in the general field, have been obtained. The strength of the CO (2.3 micron) absorptio…