1.2k citations
- ARC Centre of Excellence for Gravitational Wave DiscoveryAU155 papers
- Australian National UniversityAU124 papers
- ARC Centre of Excellence for All-sky AstrophysicsAU117 papers
- Centre for Quantum Computation and Communication TechnologyAU108 papers
- ASTRO-3DAU104 papers
- Swinburne University of TechnologyAU99 papers
- Griffith UniversityAU90 papers
- International Centre for Radio Astronomy ResearchAU90 papers
- The University of MelbourneAU89 papers
- UNSW SydneyAU85 papers
- The University of Western AustraliaAU81 papers
- Monash UniversityAU80 papers
5 papers · 1 filter
Radio Properties of EROs in the Phoenix Deep Survey
J. Afonso, A. M. Hopkins, M. Sullivan +3
Insensitive to dust obscuration, radio wavelengths are ideal to study star-forming galaxies free of dust induced biases. Using data from the Phoenix Deep Survey, we have identified…
The Phoenix Deep Survey: Evolution of Star Forming Galaxies
A. M. Hopkins, J. Afonso, A. Georgakakis +3
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 reds…
Growth models, random matrices and Painleve transcendents
Peter J. Forrester
The Hammersley process relates to the statistical properties of the maximum length of all up/right paths connecting random points of a given density in the unit square from (0,0) t…
Extremely red galaxies in the Phoenix Deep Survey
A. M. Hopkins, J. Afonso, A. Georgakakis +3
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. Here we present…
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…