Extreme Values of Black Hole to Stellar Mass Ratio for High-Redshift Galaxies

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Heather, Cameron, Chantavat, Teeraparb, Chongchitnan, Siri, Silk, Joseph
Format: Preprint
Published: 2026
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866913000952168448
author Heather, Cameron
Chantavat, Teeraparb
Chongchitnan, Siri
Silk, Joseph
author_facet Heather, Cameron
Chantavat, Teeraparb
Chongchitnan, Siri
Silk, Joseph
contents With recent data from the \emph{James Webb Space Telescope} (JWST), it is possible to calculate the mass of the supermassive black holes at the centre of galaxies, and the stellar mass of the host galaxies at $z \gtrsim 5$. In this work, we apply the method of extreme-value statistics to calculate the distributions of extreme black hole and stellar mass for the redshift range $3.5 \lesssim z \lesssim 8.5$. We sample these distributions to obtain a prediction for the black hole to stellar mass ratio of $\sim0.24$ over this redshift range, with the median in each bin varying in the range $0.18-0.35$. Our predictions are consistent with the highest observed values of the ratio from JWST observations of high-redshift galaxies.
format Preprint
id arxiv_https___arxiv_org_abs_2604_02568
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Extreme Values of Black Hole to Stellar Mass Ratio for High-Redshift Galaxies
Heather, Cameron
Chantavat, Teeraparb
Chongchitnan, Siri
Silk, Joseph
Astrophysics of Galaxies
Cosmology and Nongalactic Astrophysics
With recent data from the \emph{James Webb Space Telescope} (JWST), it is possible to calculate the mass of the supermassive black holes at the centre of galaxies, and the stellar mass of the host galaxies at $z \gtrsim 5$. In this work, we apply the method of extreme-value statistics to calculate the distributions of extreme black hole and stellar mass for the redshift range $3.5 \lesssim z \lesssim 8.5$. We sample these distributions to obtain a prediction for the black hole to stellar mass ratio of $\sim0.24$ over this redshift range, with the median in each bin varying in the range $0.18-0.35$. Our predictions are consistent with the highest observed values of the ratio from JWST observations of high-redshift galaxies.
title Extreme Values of Black Hole to Stellar Mass Ratio for High-Redshift Galaxies
topic Astrophysics of Galaxies
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2604.02568