Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power

E. Kalfountzou; J. A. Stevens; M. J. Jarvis; M. J. Hardcastle; D. Wilner; M. Elvis; M. J. Page; M. Trichas; D. J. B. Smith

doi:10.1093/mnras/stx1333

Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power

E. Kalfountzou, J. A. Stevens, M. J. Jarvis, M. J. Hardcastle, D. Wilner, M. Elvis, M. J. Page, M. Trichas, D. J. B. Smith

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Abstract

Several studies support the existence of a link between the AGN and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the AGN and the host galaxy. A drawback of previous surveys of AGN is that they are fundamentally limited by the degeneracy between redshift and luminosity in flux-density limited samples. To overcome this limitation, we present far-infrared Herschel observations of 74 radio-loud quasars (RLQs), 72 radio-quiet quasars (RQQs) and 27 radio galaxies (RGs), selected at 0.9z

Original language	English
Journal	Monthly Notices of the Royal Astronomical Society (MNRAS)
Volume	471
Issue number	1
Early online date	1 Jun 2017
DOIs	https://doi.org/10.1093/mnras/stx1333
Publication status	Published - 11 Oct 2017

Keywords

astro-ph.GA

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title = "Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power",

abstract = "Several studies support the existence of a link between the AGN and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the AGN and the host galaxy. A drawback of previous surveys of AGN is that they are fundamentally limited by the degeneracy between redshift and luminosity in flux-density limited samples. To overcome this limitation, we present far-infrared Herschel observations of 74 radio-loud quasars (RLQs), 72 radio-quiet quasars (RQQs) and 27 radio galaxies (RGs), selected at 0.9z",

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T1 - Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power

AU - Kalfountzou, E.

AU - Stevens, J. A.

AU - Jarvis, M. J.

AU - Hardcastle, M. J.

AU - Wilner, D.

AU - Elvis, M.

AU - Page, M. J.

AU - Trichas, M.

AU - Smith, D. J. B.

N1 - This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. ©: 2017 The Author (s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

PY - 2017/10/11

Y1 - 2017/10/11

N2 - Several studies support the existence of a link between the AGN and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the AGN and the host galaxy. A drawback of previous surveys of AGN is that they are fundamentally limited by the degeneracy between redshift and luminosity in flux-density limited samples. To overcome this limitation, we present far-infrared Herschel observations of 74 radio-loud quasars (RLQs), 72 radio-quiet quasars (RQQs) and 27 radio galaxies (RGs), selected at 0.9z

AB - Several studies support the existence of a link between the AGN and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the AGN and the host galaxy. A drawback of previous surveys of AGN is that they are fundamentally limited by the degeneracy between redshift and luminosity in flux-density limited samples. To overcome this limitation, we present far-infrared Herschel observations of 74 radio-loud quasars (RLQs), 72 radio-quiet quasars (RQQs) and 27 radio galaxies (RGs), selected at 0.9z

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DO - 10.1093/mnras/stx1333

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JO - Monthly Notices of the Royal Astronomical Society (MNRAS)

JF - Monthly Notices of the Royal Astronomical Society (MNRAS)

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Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power

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