activity
19982004
most citedTowards a resolution of the discrepancy between different estimators of star formation rate

225 citations · 699 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph2004★ 19 cited

The Phoenix Deep Survey: Optical and near infrared imaging catalogs

Mark Sullivan, Andrew Hopkins, Jose Afonso +5

The Phoenix Deep Survey is a multi-wavelength galaxy survey based on deep 1.4 GHz radio imaging (Hopkins et al., 2003). The primary goal of this survey is to investigate the proper…

astro-ph2003★ 62 cited

Archetypal analysis of galaxy spectra

B. H. P. Chan, D. A. Mitchell, L. E. Cram

Archetypal analysis represents each individual member of a set of data vectors as a mixture (a constrained linear combination) of the pure types or archetypes of the data set. The…

astro-ph2001★ 37 cited

Discovery of an extremely red galaxy at z=0.65 with dusty star-formation and nuclear activity

J. Afonso, B. Mobasher, B. Chan +1

In the course of the follow-up multiwavelength study of a deep radio survey we have discovered that the milli-Jansky radio source PDFJ011423 is a low-redshift (z = 0.65) extremely…

astro-ph2001★ 225 cited

Towards a resolution of the discrepancy between different estimators of star formation rate

A. M. Hopkins, A. J. Connolly, D. B. Haarsma +1

Different wavelength regimes and methods for estimating the space density of the star-formation rate (SFR) result in discrepant values. While it is recognised that ultra-violet (UV…

astro-ph2000★ 11 cited

Microjansky radio sources in DC0107-46 (Abell 2877)

A. Hopkins, A. Georgakakis, L. Cram +2

The cluster DC0107-46 (Abell 2877) lies within the Phoenix Deep Survey, made at 1.4 GHz with the Australia Telescope Compact Array. Of 89 known optical cluster members, 70 lie with…

astro-ph1999★ 1 cited

What will the next generation radio telescope detect at 1.4 GHz?

A. Hopkins, R. Windhorst, L. Cram +1

An international project is underway to design and build a radio telescope with an effective collecting area two orders of magnitude greater than the largest existing instruments.…