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Rosse Telescope

Garret Cotter

Professor of Physics

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Pulsars, transients and relativistic astrophysics
  • The Square Kilometre Array (SKA)
  • Gamma-ray astronomy
Garret.Cotter@physics.ox.ac.uk
Telephone: 01865 (2)73604
Denys Wilkinson Building, room Dalitz 4
  • About
  • Publications

MRC B1221-423: a compact steep-spectrum radio source in a merging galaxy

(2004)

Authors:

Helen M Johnston, Richard W Hunstead, Garret Cotter, Elaine M Sadler
More details from the publisher

The radio source population at high frequency: follow-up of the 15-GHz 9C survey

(2004)

Authors:

RC Bolton, G Cotter, GG Pooley, JM Riley, EM Waldram, CJ Chandler, BS Mason, TJ Pearson, ACS Readhead
More details from the publisher

MRC B1221–423: Forming an AGN in a merger

Proceedings of the International Astronomical Union Cambridge University Press (CUP) 2004:IAUS222 (2004) 451-452

Authors:

Helen Johnston, Richard Hunstead, Elaine Sadler, Garret Cotter, Raffaella Morganti
More details from the publisher

PAH features in Infrared Luminous Galaxies: Results from Michelle

Symposium - International Astronomical Union Cambridge University Press (CUP) 217 (2004) 216-217

Authors:

MS Clemens, B Nikolic, P Alexander, G Cotter, MS Longair
More details from the publisher

Searching for clusters with SUMSS

Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias 17 (2003) 263

Authors:

HJ Buttery, G Cotter, RW Hunstead, EM Sadler

Abstract:

Searches for statistical overdensities of radio sources in the NRAO VLA Sky Survey (NVSS) survey have led to the detection of high redshift clusters of galaxies (Cotter et al. 2002; Croft et al. 2001). We have carried out a similar search for overdensities using the Sydney University Molonglo Sky Survey (SUMSS). Radio observations at 20/13 cm have been made of these candidates at the Australia Telescope Compact Array (ATCA) revealing sources of diffuse cluster emission as well as groups of FR1 sources showing structures associated with clusters, indicating a cluster "hit-rate" of about 70%.
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