The coevolution of galaxies and supermassive black holes: insights from surveys of the contemporary universe
TM Heckman, PN Best - Annual Review of Astronomy and …, 2014 - annualreviews.org
We summarize what large surveys of the contemporary Universe have taught us about the
physics and phenomenology of the processes that link the formation and evolution of …
physics and phenomenology of the processes that link the formation and evolution of …
Observational evidence for intermediate-mass black holes
M Mezcua - International Journal of Modern Physics D, 2017 - World Scientific
Intermediate-mass black holes (IMBHs), with masses in the range 1 0 0–1 0 6 M⊙, are the
link between stellar-mass BHs and supermassive BHs (SMBHs). They are thought to be the …
link between stellar-mass BHs and supermassive BHs (SMBHs). They are thought to be the …
The bolometric quasar luminosity function at z = 0–7
In this paper, we provide updated constraints on the bolometric quasar luminosity function
(QLF) from z= 0 to z= 7. The constraints are based on an observational compilation that …
(QLF) from z= 0 to z= 7. The constraints are based on an observational compilation that …
The ASTRID simulation: the evolution of supermassive black holes
We present the evolution of black holes (BHs) and their relationship with their host galaxies
in Astrid, a large-volume cosmological hydrodynamical simulation with box size 250 h …
in Astrid, a large-volume cosmological hydrodynamical simulation with box size 250 h …
AGN wind scaling relations and the co-evolution of black holes and galaxies
Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as
the main mechanism responsible for regulating star formation in active galactic nucleus …
the main mechanism responsible for regulating star formation in active galactic nucleus …
Relations between central black hole mass and total galaxy stellar mass in the local universe
AE Reines, M Volonteri - The Astrophysical Journal, 2015 - iopscience.iop.org
Scaling relations between central black hole (BH) mass and host galaxy properties are of
fundamental importance to studies of BH and galaxy evolution throughout cosmic time. Here …
fundamental importance to studies of BH and galaxy evolution throughout cosmic time. Here …
The final SDSS high-redshift quasar sample of 52 quasars at z> 5.7
We present the discovery of nine quasars at $ z\sim 6$ identified in the Sloan Digital Sky
Survey (SDSS) imaging data. This completes our survey of $ z\sim 6$ quasars in the SDSS …
Survey (SDSS) imaging data. This completes our survey of $ z\sim 6$ quasars in the SDSS …
Cosmic reionization after Planck: Could quasars do it all?
We assess a model of late cosmic reionization in which the ionizing background radiation
arises entirely from high-redshift quasars and other active galactic nuclei (AGNs). The low …
arises entirely from high-redshift quasars and other active galactic nuclei (AGNs). The low …
The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z∼ 5
J Aird, AL Coil, A Georgakakis, K Nandra… - Monthly Notices of …, 2015 - academic.oup.com
We present new measurements of the evolution of the X-ray luminosity functions (XLFs) of
unabsorbed and absorbed active galactic nuclei (AGNs) out to z∼ 5. We construct samples …
unabsorbed and absorbed active galactic nuclei (AGNs) out to z∼ 5. We construct samples …
Nuclear activity versus star formation: emission-line diagnostics at ultraviolet and optical wavelengths
A Feltre, S Charlot, J Gutkin - Monthly Notices of the Royal …, 2016 - academic.oup.com
In the context of observations of the rest-frame ultraviolet and optical emission from distant
galaxies, we explore the emission-line properties of photoionization models of active and …
galaxies, we explore the emission-line properties of photoionization models of active and …