A unified multiwavelength model of galaxy formation
We present a new version of the galform semi-analytical model of galaxy formation. This
brings together several previous developments of galform into a single unified model …
brings together several previous developments of galform into a single unified model …
Black hole variability and the star formation–active galactic nucleus connection: do all star-forming galaxies host an active galactic nucleus?
We investigate the effect of active galactic nucleus (AGN) variability on the observed
connection between star formation and black hole accretion in extragalactic surveys. Recent …
connection between star formation and black hole accretion in extragalactic surveys. Recent …
A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations
In large-scale cosmological hydrodynamic simulations simplified sub-grid models for gas
accretion on to black holes and AGN feedback are commonly used. Such models typically …
accretion on to black holes and AGN feedback are commonly used. Such models typically …
Semi-analytic forecasts for JWST – V. AGN luminosity functions and helium reionization at z = 2–7
Active galactic nuclei (AGN) forming in the early universe are thought to be the primary
source of hard ionizing photons contributing to the reionization of intergalactic helium …
source of hard ionizing photons contributing to the reionization of intergalactic helium …
The (black hole)-bulge mass scaling relation at low masses
Several recent papers have reported on the occurrence of active galactic nuclei (AGNs)
containing undermassive black holes relative to a linear scaling relation between black hole …
containing undermassive black holes relative to a linear scaling relation between black hole …
Comparison of the star formation in X-ray-selected AGN in eFEDS with that of star-forming galaxies
We use approximately 1800 X-ray active galactic nuclei (AGN) in the eROSITA Final
Equatorial-Depth Survey (eFEDS) that span over two orders of magnitude in X-ray …
Equatorial-Depth Survey (eFEDS) that span over two orders of magnitude in X-ray …
Observational constraints on the specific accretion-rate distribution of X-ray-selected AGNs
This paper estimates the specific accretion-rate distribution of AGNs using a sample of 4821
X-ray sources from both deep and shallow surveys. The specific accretion-rate distribution is …
X-ray sources from both deep and shallow surveys. The specific accretion-rate distribution is …
Detailed shape and evolutionary behavior of the X-ray luminosity function of active galactic nuclei
We construct the rest-frame 2–10 keV intrinsic X-ray luminosity function (XLF) of active
galactic nuclei (AGNs) from a combination of X-ray surveys from the all-sky Swift BAT survey …
galactic nuclei (AGNs) from a combination of X-ray surveys from the all-sky Swift BAT survey …
The role of AGN and obscuration in the position of the host galaxy relative to the main sequence
We use X-ray active galactic nuclei (AGN) observed by the Chandra X-ray Observatory
within the 9.3 deg 2 Boötes field of the NDWFS to study whether there is a correlation …
within the 9.3 deg 2 Boötes field of the NDWFS to study whether there is a correlation …
Star formation of X-ray AGN in COSMOS: The role of AGN activity and galaxy stellar mass
We use approximately 1000 X-ray sources in the COSMOS-Legacy survey and study the
position of the AGN relative to the star forming main sequence (MS). We also construct a …
position of the AGN relative to the star forming main sequence (MS). We also construct a …