251 citations · 723 across the 15 of their papers we have counts for
15 papers
Deep Herschel observations of the 2Jy sample: assessing the non-thermal and AGN contributions to the far-IR continuum
D. Dicken, C. N. Tadhunter, N. P. H. Nesvadba +5
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 re…
Quantifying the cool ISM in radio AGNs: evidence for late-time re-triggering by galaxy mergers and interactions
E. Bernhard, C. N. Tadhunter, J. C. S. Pierce +4
We use deep Herschel observations of the complete 2Jy sample of powerful radio AGNs in the local universe (0.05 < z < 0.7) to probe their cool interstellar medium (ISM) contents an…
Taking snapshots of the jet-ISM interplay: The case of PKS0023-26
Raffaella Morganti, Tom Oosterloo, Clive Tadhunter +2
We present high angular resolution ALMA CO(2-1) and 1.7 mm continuum observations of the far-infrared-bright galaxy PKS0023-26, which hosts a young radio source and a luminous opti…
The post-Herschel view of intrinsic AGN emission: constructing templates for galaxy and AGN emission at IR wavelengths
E. Bernhard, C. Tadhunter, J. R. Mullaney +3
Measuring the star-forming properties of AGN hosts is key to our understanding of galaxy formation and evolution. However, this topic remains debated, partly due to the difficultie…
The evolving AGN duty cycle in galaxies since z3 as encoded in the X-ray luminosity function
I. Delvecchio, E. Daddi, J. Aird +10
We present a new modeling of the X-ray luminosity function (XLF) of Active Galactic Nuclei (AGN) out to z3, dissecting the contribution of main-sequence (MS) and starburst (S…
A binning-free method reveals a continuous relationship between galaxies' AGN power and offset from main sequence
L. P. Grimmett, J. R. Mullaney, E. P. Bernhard +5
Studies investigating the relationship between AGN power and the star formation rates (SFRs) of their host galaxies often rely on averaging techniques -- such as stacking -- to inc…