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

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        Author
        Kalfountzou, E.
        Stevens, J. A.
        Jarvis, M. J.
        Hardcastle, M. J.
        Wilner, D.
        Elvis, M.
        Page, M. J.
        Trichas, M.
        Smith, D. J. B.
        Attention
        2299/19463
        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
        Publication date
        2017-10-11
        Published in
        Monthly Notices of the Royal Astronomical Society
        Published version
        https://doi.org/10.1093/mnras/stx1333
        Other links
        http://hdl.handle.net/2299/19463
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