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91探花
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

CGRaBS: An all-sky survey of gamma-ray blazar candidates

Astrophysical Journal Supplement Series 175:1 (2008) 97-104

Authors:

SE Healey, RW Romani, G Cotter, PF Michelson, EF Schlafly, ACS Readhead, P Giommi, S Chaty, IA Grenier, LC Weintraub

Abstract:

We describe a uniform all-sky survey of bright blazars, selected primarily by their flat radio spectra, that is designed to provide a large catalog of likely 纬-ray active galactic nuclei (AGNs). The defined sample has 1625 targets with radio and X-ray properties similar to those of the EGRET blazars, spread uniformly across the |b| > 10掳 sky. We also report progress toward optical characterization of the sample; of objects with known R < 23, 85% have been classified and 81% have measured redshifts. One goal of this program is to focus attention on the most interesting (e.g., high-redshift, high-luminosity,...) sources for intensive multiwavelength study during the observations by the Large Area Telescope (LAT) on GLAST. 漏 2008. The American Astronomical Society. All rights reserved.

Characteristics of EGRET blazars in the VLBA Imaging and Polarimetry Survey (VIPS)

Astrophysical Journal 671:2 (2007) 1355-1364

Authors:

GB Taylor, SE Healey, JF Helmboldt, S Tremblay, CD Fassnacht, RC Walker, LO Sjouwerman, TJ Pearson, ACS Readhead, L Weintraub, N Gehrels, RW Romani, PF Michelson, RD Blandford, G Cotter

Abstract:

We examine the radio properties of EGRET-detected blazars observed as part of the VLBA Imaging and Polarimetry Survey (VIPS). VIPS has a flux limit roughly an order of magnitude below the MOJAVE survey and most other samples that have been used to study the properties of EGRET blazars. At lower flux levels, radio flux density does not directly correlate with gamma-ray flux density. We do find that the EGRET-detected blazars tend to have higher brightness temperatures, greater core fractions, and possibly larger than average jet opening angles. A weak correlation is also found with jet length and with polarization. All of the well-established trends can be explained by systematically larger Doppler factors in the gamma-ray-loud blazars, consistent with the measurements of higher apparent velocities found in monitoring programs carried out at radio frequencies above 10 GHz. 漏 2007. The American Astronomical Society. All rights reserved.

CGRaBS: An All-Sky Survey of Gamma-Ray Blazar Candidates

(2007)

Authors:

Stephen E Healey, Roger W Romani, Garret Cotter, Peter F Michelson, Edward F Schlafly, Anthony CS Readhead, Paolo Giommi, Sylvain Chaty, Isabelle A Grenier, Lawrence C Weintraub

Characteristics of EGRET Blazars in the VLBA Imaging and Polarimetry Survey (VIPS)

(2007)

Authors:

GB Taylor, SE Healey, JF Helmboldt, S Tremblay, CD Fassnacht, RC Walker, LO Sjouwerman, TJ Pearson, ACS Readhead, L Weintraub, N Gehrels, RW Romani, PF Michelson, RD Blandford, G Cotter

Spectroscopic follow-up of a cluster candidate at z = 1.45

(2007)

Authors:

Caroline van Breukelen, Garret Cotter, Steve Rawlings, Tony Readhead, David Bonfield, Lee Clewley, Rob Ivison, Matt Jarvis, Chris Simpson, Mike Watson

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