http://arxiv.org/abs/2211.13031
The far-IR/sub-mm wavelength range contains a wealth of diagnostic information that is important for understanding the role of radio AGN in galaxy evolution. Here we present the results of Herschel PACS and SPIRE observations of a complete sample of 46 powerful 2Jy radio AGN at intermediate redshifts (0.05 < z < 0.7), which represent the deepest pointed observations of a major sample of radio AGN undertaken by Herschel. In order to assess the importance of non-thermal synchrotron emission at far-IR wavelengths, we also present new APEX sub-mm and ALMA mm data. We find that the overall incidence of non-thermal contamination in the PACS bands ($<$200$\mu$m) is in the range 28 — 43%; however, this rises to 30 — 72% for wavelengths ($> $200$\mu$m) sampled by the SPIRE instrument. Non-thermal contamination is strongest in objects with compact CSS/GPS or extended FRI radio morphologies, and in those with type 1 optical spectra. Considering thermal dust emission, we find strong correlations between the 100 and 160$\mu$m monochromatic luminosities and AGN power indicators, providing further evidence that radiation from the AGN may be an important heating source for the far-IR emitting dust. Clearly, AGN contamination — whether by the direct emission from synchrotron-emitting lobes and cores, or via radiative heating of the cool dust — needs to be carefully considered when using the far-IR continuum to measure the star formation rates in the host galaxies of radio AGN.
D. Dicken, C. Tadhunter, N. Nesvadba, et. al.
Thu, 24 Nov 22
47/71
Comments: 22 pages, 8 figures, Accepted in MNRAS