Coevolution (or not) of supermassive black holes and host galaxies

J Kormendy, LC Ho - Annual Review of Astronomy and …, 2013 - annualreviews.org
Supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of
spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by …

What drives the growth of black holes?

DM Alexander, RC Hickox - New Astronomy Reviews, 2012 - Elsevier
Massive black holes (BHs) are at once exotic and yet ubiquitous, residing at the centers of
massive galaxies in the local Universe. Recent years have seen remarkable advances in …

JADES-The diverse population of infant black holes at 4< z< 11: Merging, tiny, poor, but mighty

R Maiolino, J Scholtz, E Curtis-Lake, S Carniani… - Astronomy & …, 2024 - aanda.org
Spectroscopy with the James Webb Space Telescope has opened the possibility of
identifying moderate-luminosity active galactic nuclei (AGNs) in the early Universe, at and …

The X–shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars

EP Farina, JT Schindler, F Walter… - The Astrophysical …, 2022 - iopscience.iop.org
We present measurements of black hole masses and Eddington ratios (λ Edd) for a sample
of 38 bright (M 1450<− 24.4 mag) quasars at 5.8≲ z≲ 7.5, derived from Very Large …

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 …

An ALMA [C II] Survey of 27 Quasars at z> 5.94

R Decarli, F Walter, BP Venemans… - The Astrophysical …, 2018 - iopscience.iop.org
An ALMA [C ii] Survey of 27 Quasars at z > 5.94 - IOPscience Skip to content IOP Science
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The Illustris simulation: the evolving population of black holes across cosmic time

D Sijacki, M Vogelsberger, S Genel… - Monthly Notices of …, 2015 - academic.oup.com
We study the properties of black holes and their host galaxies across cosmic time in the
Illustris simulation. Illustris is a large-scale cosmological hydrodynamical simulation which …

The low-luminosity end of the radius–luminosity relationship for active galactic nuclei

MC Bentz, KD Denney, CJ Grier, AJ Barth… - The Astrophysical …, 2013 - iopscience.iop.org
We present an updated and revised analysis of the relationship between the Hβ broad-line
region (BLR) radius and the luminosity of the active galactic nucleus (AGN). Specifically, we …

A preferential growth channel for supermassive black holes in elliptical galaxies at z≲ 2

D Farrah, S Petty, KS Croker, G Tarlé… - The Astrophysical …, 2023 - iopscience.iop.org
The assembly of stellar and supermassive black hole (SMBH) mass in elliptical galaxies
since z∼ 1 can help to diagnose the origins of locally observed correlations between SMBH …

The mass relations between supermassive black holes and their host galaxies at 1< z< 2 with HST-WFC3

X Ding, J Silverman, T Treu, A Schulze… - The Astrophysical …, 2020 - iopscience.iop.org
Correlations between the mass of a supermassive black hole (SMBH) and the properties of
its host galaxy (eg, total stellar mass M*, luminosity L host) suggest an evolutionary …