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The Black Hole Masses of High-Redshift Quasars

R. J McLure·M. J. Jarvis
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Abstract

A reliable method for estimating the black-hole masses of high-redshift quasars would provide crucial new information for understanding the nature and cosmological evolution of quasars. In this proceedings we summarize the results of our recent paper (McLure & Jarvis 2002) which provides a virial black-hole mass estimator based on rest-frame UV observables, thereby allowing reliable black-hole mass estimates to be obtained out to redshifts of $z\sim2.5$ from optical spectra alone.

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R. J McLure, M. J. Jarvis. 2003-02-21. The Black Hole Masses of High-Redshift Quasars. https://arxiv.org/abs/astro-ph/0302457

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