Journal
ASTROPHYSICAL JOURNAL
Volume 627, Issue 1, Pages L1-L4Publisher
IOP PUBLISHING LTD
DOI: 10.1086/432159
Keywords
galaxies : high redshift; large scale structure of universe; quasars : general
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We use the clustering of galaxies around distant active galactic nuclei ( AGNs) to derive an estimate of the relationship between galaxy and black hole mass that obtained during the ancient quasar epoch, at redshifts, when giant black holes accreted much of their mass. Neither the mean relationship nor its scatter 2 <= z <= 3 differs significantly from what is observed in the local universe, at least over the ranges of apparent magnitude (16 less than or similar to G(AB) less than or similar to 26) and black hole mass (10(6) M-circle dot less than or similar to M-BH less than or similar to 10(10.5) M-circle dot) that we are able to probe.
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