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The supermassive black holes observed at the centers of almost all present-day galaxies, had a profound impact on their environment. I highlight the principle of self-regulation, by which supermassive black holes grow until they release…

Astrophysics · Physics 2009-11-10 Abraham Loeb

The existence of supermassive black holes as early as z ~ 7 is one of the great unsolved problems in cosmological structure formation. One leading theory argues that they are born during catastrophic baryon collapse in z ~ 15 protogalaxies…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 Daniel J. Whalen , Wesley Even , Joseph Smidt , Alexander Heger , K. -J. Chen , Chris L. Fryer , Massimo Stiavelli , Hao Xu , Candace C. Joggerst

The first observations of the James Webb Space Telescope (JWST) have identified six massive galaxy candidates with the stellar masses $M_\ast\gtrsim 10^{10}\,M_\odot$ at high redshifts $7.4\lesssim z\lesssim 9.1$, with two most massive…

Cosmology and Nongalactic Astrophysics · Physics 2023-06-09 Bing-Yu Su , Nan Li , Lei Feng

I review some recent progress made in our understanding of galaxy evolution and the cosmic history of star formation. Like bookends, the results obtained from deep ground-based spectroscopy and from the Hubble Deep Field imaging survey put…

Astrophysics · Physics 2009-10-28 Piero Madau

Recent JWST observations indicate that massive quiescent galaxies (stellar mass $M_{*}\gtrsim 10^{10}~\mathrm{M_\odot}$) at high redshift ($z\gtrsim 6$) are more abundant than predicted by most existing galaxy formation simulations and…

Astrophysics of Galaxies · Physics 2026-01-22 Evgenii Chaikin , Joop Schaye , Filip Huško , Cedric G. Lacey , Sylvia Ploeckinger , Matthieu Schaller

The observational evidence that Super-Massive Black Holes ($M_{\bullet} \sim 10^{9-10} \, \mathrm{M_{\odot}}$) are already in place less than $1 \, \mathrm{Gyr}$ after the Big Bang poses stringent time constraints on the growth efficiency…

Astrophysics of Galaxies · Physics 2015-07-22 Fabio Pacucci , Marta Volonteri , Andrea Ferrara

In this white paper we explore the capabilities required to identify and study supermassive black holes formed from heavy seeds ($\mathrm{M_{\bullet}} \sim 10^4 - 10^6 \, \mathrm{M_{\odot}}$) in the early Universe. To obtain an unequivocal…

We discuss currently available observational constraints on the reionization history of the intergalactic medium (IGM), and the extent to which accreting black holes (BHs) can help explain these observations. We show new evidence, based on…

Astrophysics · Physics 2009-11-10 Zoltan Haiman , Mark Dijkstra , Andrei Mesinger

The assembly of the first super massive black holes (SMBHs) at $z \gtrsim 6$ is still a subject of intense debate. If black holes (BHs) grow at their Eddington rate, they must start from $\gtrsim 10^4 \, M_\odot$ seeds formed by the direct…

Astrophysics of Galaxies · Physics 2016-03-03 Edwige Pezzulli , Rosa Valiante , Raffaella Schneider

One of the key open questions in cosmology today pertains to understanding when, where and how super massive black holes form, while it is clear that mergers likely play a significant role in the growth cycles of black holes, how…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Kevin Schawinski , Meg Urry , Ezequiel Treister , Brooke Simmons , Priyamvada Natarajan , Eilat Glikman

Super-Eddington accretion has been suggested as a possible formation pathway of $10^9 \, M_\odot$ supermassive black holes (SMBHs) 800 Myr after the Big Bang. However, stellar feedback from BH seed progenitors and winds from BH accretion…

Astrophysics of Galaxies · Physics 2017-06-29 Edwige Pezzulli , Marta Volonteri , Raffaella Schneider , Rosa Valiante

If supermassive black holes (SMBHs) are the energy sources that power quasars and active galactic nuclei, then QSO SDSS 1148+5251, the quasar with the highest redshift (z_QSO=6.43), hosts a supermassive black hole formed within 0.9 Gyr…

Astrophysics · Physics 2009-11-10 Stuart L. Shapiro

One of the main themes in extragalactic astronomy for the next decade will be the evolution of galaxies over cosmic time. Many future observatories, including JWST, ALMA, GMT, TMT and E-ELT will intensively observe starlight over a broad…

JWST has revealed the apparent evolution of the black hole (BH)-stellar mass ($M_\mathrm{BH}$-$M_\rm{\ast}$) relation in the early Universe, while remaining consistent with the BH-dynamical mass ($M_\mathrm{BH}$-$M_\mathrm{dyn}$) relation.…

Deep space observations of the James Webb Space Telescope (JWST) have revealed that the structure and masses of very early Universe galaxies at high redshifts (z~15), existing at ~0.3 Gyr after the BigBang, maybe as evolved as the galaxies…

Cosmology and Nongalactic Astrophysics · Physics 2023-09-26 Rajendra Gupta

The James Webb Space Telescope (JWST) has revealed a previously unknown population of compact, red galaxies at $z \sim 5$, known as "Little Red Dots" (LRDs). With effective radii of $\sim 100$ pc and stellar masses of $10^9-10^{11} \,…

Astrophysics of Galaxies · Physics 2025-11-14 Fabio Pacucci , Lars Hernquist , Michiko Fujii

Supermassive black holes (SMBHs) are thought to originate from early Universe seed black holes of mass $M_\mathrm{BH} \sim 10^2$-10$^5$ M$_{\odot}$ and grown through cosmic time. Such seeds could be powering the active galactic nuclei (AGN)…

Astrophysics of Galaxies · Physics 2024-09-02 M. Mezcua , M. Siudek , H. Suh , Valiante , D. Spinoso , S. Bonoli

I begin by summarizing the evidence that there is a close relationship between the evolution of galaxies and supermassive black holes. They evidently share a common fuel source, and feedback from the black hole may be needed to suppress…

Astrophysics · Physics 2015-05-13 T. M. Heckman

Understanding the formation and growth of supermassive black holes (SMBHs) at high redshift represents a major challenge for theoretical models. In this work we investigate the early evolution of the first SMBHs by constraining their…

Astrophysics of Galaxies · Physics 2022-01-19 Alessandro Trinca , Raffaella Schneider , Rosa Valiante , Luca Graziani , Luca Zappacosta , Francesco Shankar

Supermassive black hole (SMBH) growth plausibly occurs via runaway astrophysical black hole mergers in nuclear star clusters that form intermediate mass black hole seeds at high redshifts. Such a model yields an order-of-magnitude higher…

High Energy Astrophysical Phenomena · Physics 2026-03-18 Konstantinos Kritos , Joseph Silk