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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 705
  • About
  • Publications

The Balmer-dominated Bow Shock and Wind Nebula Structure of Gamma-ray Pulsar PSR J1741-2054

(2010)

Authors:

Roger W Romani, Michael S Shaw, Fernando Camilo, Garret Cotter, Gregory R Sivakoff
More details from the publisher

The extraordinary radio galaxy MRC B1221-423: probing deeper at radio and optical wavelengths

(2010)

Authors:

Helen M Johnston, Jess W Broderick, Garret Cotter, Raffaella Morganti, Richard W Hunstead
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The extraordinary radio galaxy MRC B1221-423: Probing deeper at radio and optical wavelengths

Monthly Notices of the Royal Astronomical Society 407:2 (2010) 721-733

Authors:

HM Johnston, JW Broderick, G Cotter, R Morganti, RW Hunstead

Abstract:

We present optical spectra and high-resolution multiwavelength radio observations of the compact steep-spectrum radio source MRC B1221-423 (z = 0.1706). MRC B1221-423 is a very young (∼105 yr), powerful radio source which is undergoing a tidal interaction with a companion galaxy. We find strong evidence of interaction between the active galactic nucleus (AGN) and its environment. The radio morphology is highly distorted, showing a dramatic interaction between the radio jet and the host galaxy, with the jet being turned almost back on itself. H i observations show strong absorption against the nucleus at an infall velocity of ∼250 km s-1 compared to the stellar velocity, as well as a second, broader component which may represent gas falling into the nucleus. Optical spectra show that star formation is taking place across the whole system. Broad optical emission lines in the nucleus show evidence of outflow. Our observations confirm that MRC B1221-423 is a young radio source in a gas-rich nuclear environment, and that there was a time delay of a few times 100 Myr between the onset of star formation and the triggering of the AGN. © 2010 The Authors. Journal compilation © 2010 RAS.
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The first catalog of active galactic nuclei detected by the Fermi large area telescope

Astrophysical Journal 715:1 (2010) 429-457

Authors:

AA Abdo, M Ackermann, M Ajello, A Allafort, E Antolini, WB Atwood, M Axelsson, L Baldini, J Ballet, G Barbiellini, D Bastieri, BM Baughman, K Bechtol, R Bellazzini, B Berenji, RD Blandford, ED Bloom, JR Bogart, E Bonamente, AW Borgland, A Bouvier, J Bregeon, A Brez, M Brigida, P Bruel, R Buehler, TH Burnett, S Buson, GA Caliandro, RA Cameron, A Cannon, PA Caraveo, S Carrigan, JM Casandjian, E Cavazzuti, C Cecchi, O Çelik, A Celotti, E Charles, A Chekhtman, AW Chen, CC Cheung, J Chiang, S Ciprini, R Claus, J Cohen-Tanugi, J Conrad, L Costamante, G Cotter, S Cutini, V D'Elia, CD Dermer, A De Angelis, F De Palma, A De Rosa, SW Digel, E Do Couto E Silva, PS Drell, R Dubois, D Dumora, L Escande, C Farnier, C Favuzzi, SJ Fegan, EC Ferrara, WB Focke, P Fortin, M Frailis, Y Fukazawa, S Funk, P Fusco, F Gargano, D Gasparrini, N Gehrels, S Germani, B Giebels, N Giglietto, P Giommi, F Giordano, M Giroletti, T Glanzman, G Godfrey, P Grandi, IA Grenier, MH Grondin, JE Grove, S Guiriec, D Hadasch, AK Harding, M Hayashida, E Hays, SE Healey, AB Hill, D Horan, RE Hughes, G Iafrate, R Itoh, G Jóhannesson, AS Johnson, RP Johnson

Abstract:

We present the first catalog of active galactic nuclei (AGNs) detected by the Large Area Telescope (LAT), corresponding to 11 months of data collected in scientific operation mode. The First LAT AGN Catalog (1LAC) includes 671 γ-ray sources located at high Galactic latitudes (|b|>10°) that are detected with a test statistic greater than 25 and associated statistically with AGNs. Some LAT sources are associated with multiple AGNs, and consequently, the catalog includes 709 AGNs, comprising 300 BL Lacertae objects, 296 flat-spectrum radio quasars, 41 AGNs of other types, and 72 AGNs of unknown type. We also classify the blazars based on their spectral energy distributions as archival radio, optical, and X-ray data permit. In addition to the formal 1LAC sample, we provide AGN associations for 51 low-latitude LAT sources and AGN "affiliations" (unquantified counterpart candidates) for 104 high-latitude LAT sources without AGN associations. The overlap of the 1LAC with existing γ-ray AGN catalogs (LBAS, EGRET, AGILE, Swift, INTEGRAL, TeVCat) is briefly discussed. Various properties - such as γ-ray fluxes and photon power-law spectral indices, redshifts, γ-ray luminosities, variability, and archival radio luminosities - and their correlations are presented and discussed for the different blazar classes. We compare the 1LAC results with predictions regarding the γ-ray AGN populations, and we comment on the power of the sample to address the question of the blazar sequence. © 2010. The American Astronomical Society. All rights reserved..
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Optical Spectroscopy of Bright Fermi LAT Blazars

(2009)

Authors:

Michael S Shaw, Roger W Romani, Stephen E Healey, Garret Cotter, Peter F Michelson, Anthony CS Readhead
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