GOODS-Herschel: radio-excess signature of hidden AGN activity in distant star-forming galaxies
A. Del Moro,David M. Alexander,James Mullaney,James Mullaney,Emanuele Daddi,Maurilio Pannella,Franz E. Bauer,Franz E. Bauer,Alexandra Pope,M. Dickinson,David Elbaz,Pieter Barthel,M. A. Garrett,M. A. Garrett,M. A. Garrett,W. N. Brandt,Vassilis Charmandaris,Ranga-Ram Chary,Kalliopi Dasyra,Kalliopi Dasyra,Roberto Gilli,Ryan C. Hickox,Ho Seong Hwang,Rob Ivison,Stéphanie Juneau,E. Le Floc'h,Birong Luo,Glenn Morrison,Emmanouel Rovilos,Emmanouel Rovilos,Mark Sargent,Yongquan Xue,Yongquan Xue +32 more
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TLDR
In this paper, a spectral energy distribution (SED) fitting approach was proposed to select radio-excess sources amongst distant star-forming galaxies in the GOODS-Herschel (North) field and to reveal the presence of hidden, highly obscured AGN.Citations
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Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population
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Active galactic nuclei: what’s in a name?
Paolo Padovani,David M. Alexander,Roberto J. Assef,B. De Marco,Paolo Giommi,Ryan C. Hickox,Gordon T. Richards,Vernesa Smolčić,Evanthia Hatziminaoglou,V. Mainieri,Mara Salvato +10 more
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Cosmic X-ray surveys of distant active galaxies
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TL;DR: In this paper, the authors review results from cosmic X-ray surveys of active galactic nuclei (AGNs) over the past 15 years that have dramatically improved our understanding of growing supermassive black holes in the distant universe.
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A two-parameter model for the infrared/submillimeter/radio spectral energy distributions of galaxies and active galactic nuclei
TL;DR: In this paper, a two-parameter semi-empirical model for the spectral energy distributions of galaxies with contributions to their infrared-submillimeter-radio emission from both star formation and accretion disk-powered activity is presented.
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A Two-Parameter Model for the Infrared/Submillimeter/Radio Spectral Energy Distributions of Galaxies and AGN
TL;DR: In this paper, a two-parameter semi-empirical model is presented for the spectral energy distributions of galaxies with contributions to their infrared-submillimeter-radio emission from both star formation and accretion disk-powered activity.
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