A binning-free method reveals a continuous relationship between galaxies' AGN power and offset from main sequence
Artikel i vetenskaplig tidskrift, 2020

Studies investigating the relationship between active galactic nucleus (AGN) power and the star formation rates (SFRs) of their host galaxies often rely on averaging techniques - such as stacking - to incorporate information from non-detections. However, averages, and especially means, can be strongly affected by outliers and can therefore give a misleading indication of the 'typical' case. Recently, a number of studies have taken a step further by binning their sample in terms of AGN power (approximated by the 2-10 keV luminosity of the AGN), and investigating how the SFR distribution differs between these bins. These bin thresholds are often weakly motivated, and binning implicitly assumes that sources within the same bin have similar (or even identical) properties. In this paper, we investigate whether the distribution of host SFRs - relative to the locus of the star-forming main sequence (i.e. RMS) - changes continuously as a function of AGN power. We achieve this by using a hierarchical Bayesian model that completely removes the need to bin in AGN power. In doing so, we find strong evidence that the RMS distribution changes with 2-10 keV X-ray luminosity. The results suggest that higher X-ray luminosity AGNs have a tighter physical connection to the star-forming process than lower X-ray luminosity AGNs, at least within the 0.8 < z< 1.2 redshift range considered here.

galaxies: evolution

methods: statistical

galaxies: statistics

Författare

L. P. Grimmett

University of Sheffield

J. R. Mullaney

University of Sheffield

E. P. Bernhard

University of Sheffield

C. M. Harrison

Newcastle University

D. M. Alexander

Durham University

Flora Stanley

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

V. A. Masoura

Natl Observ Athens

K. Walters

University of Sheffield

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 495 1 1392-1402

Ämneskategorier

Astronomi, astrofysik och kosmologi

Sannolikhetsteori och statistik

DOI

10.1093/mnras/staa1255

Mer information

Senast uppdaterat

2020-07-01