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Main Author: Barai, Paramita
Format: Recurso digital
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Published: Zenodo 2026
Online Access:https://doi.org/10.5281/zenodo.18804799
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author Barai, Paramita
author_facet Barai, Paramita
contents Supermassive Black Holes (SMBHs) at the centers of high-z quasars are observed to have grown to masses >= 10^9 Msun by redshifts z=6-7. Recent JWST observations are additionally revealing the existence of central intermediate-mass BHs (10^7 - 10^8 Msun) at even earlier epochs z~10-12; some of which sources have BH mass comparable to the mass of the host galaxy. At the same time, very recent JWST observations have detected a population of normal-mass central SMBHs at z~3-5, with the mean SMBH-to stellar mass ratio consistent with the local relation. The formation of such supermassive (overmassive and normal-mass) BHs at the centers of their host galaxies involves unresolved questions.
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_18804799
institution Zenodo
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publishDate 2026
publisher Zenodo
record_format zenodo
spellingShingle Growth of Central Massive Black Holes and Feedback on Host Galaxies using Cosmological Simulations
Barai, Paramita
Supermassive Black Holes (SMBHs) at the centers of high-z quasars are observed to have grown to masses >= 10^9 Msun by redshifts z=6-7. Recent JWST observations are additionally revealing the existence of central intermediate-mass BHs (10^7 - 10^8 Msun) at even earlier epochs z~10-12; some of which sources have BH mass comparable to the mass of the host galaxy. At the same time, very recent JWST observations have detected a population of normal-mass central SMBHs at z~3-5, with the mean SMBH-to stellar mass ratio consistent with the local relation. The formation of such supermassive (overmassive and normal-mass) BHs at the centers of their host galaxies involves unresolved questions.
title Growth of Central Massive Black Holes and Feedback on Host Galaxies using Cosmological Simulations
url https://doi.org/10.5281/zenodo.18804799