activity
19982008
most citedThe Phoenix Deep Survey: The 1.4 GHz microJansky catalogue

174 citations · 495 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph2008★ 2 cited

The Phoenix Deep Survey: Extremely Red Galaxies and Cluster Candidates

Anthony G. Smith, Andrew M. Hopkins, Richard W. Hunstead +6

We present the results of a study of a sample of 375 Extremely Red Galaxies (ERGs) in the Phoenix Deep Survey, 273 of which constitute a subsample which is 80% complete to K_s = 18…

astro-ph2004★ 51 cited

The Phoenix Deep Survey: spectroscopic catalog

J. Afonso, A. Georgakakis, C. Almeida +4

The Phoenix Deep Survey is a multi-wavelength survey based on deep 1.4 GHz radio imaging, reaching well into the sub-100 microJy level. One of the aims of this survey is to charact…

astro-ph2003★ 4 cited

Faint 1.4 GHz sources in the 2dF Galaxy Redshift Survey

B. H. P. Chan, L. E. Cram, E. M. Sadler +4

The Australia Telescope Compact Array (ATCA) has been used to survey at 1.4GHz, a small region (< 3 sq deg) overlapping with the 2dF Galaxy Redshift Survey (Colless et al. 2001, MN…

astro-ph2003★ 36 cited

The Phoenix Deep Survey: X-ray properties of faint radio sources

A. Georgakakis, A. M. Hopkins, M. Sullivan +4

In this paper we use a 50ks XMM-Newton pointing overlapping with the Phoenix Deep Survey, a homogeneous radio survey reaching muJy sensitivities, to explore the X-ray properties an…

astro-ph2002★ 174 cited

The Phoenix Deep Survey: The 1.4 GHz microJansky catalogue

A. M. Hopkins, J. Afonso, B. Chan +3

The initial Phoenix Deep Survey (PDS) observations with the Australia Telescope Compact Array have been supplemented by additional 1.4 GHz observations over the past few years. Her…

astro-ph2001★ 140 cited

A Comparison of Independent Star Formation Diagnostics for a UV-Selected Sample of Nearby Galaxies

Mark Sullivan, Bahram Mobasher, Ben Chan +4

We present results from a decimetric radio survey undertaken with the Very Large Array as part of a longer term goal to inter-compare star formation and dust extinction diagnostics…