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