Abstract:Abstract.We study the evolution of the MBH /M h ost relation up to z = 3 for a sample of 96 quasars with known host galaxy luminosities. Black hole masses are estimated assuming virial equilibrium in the broad-line regions, while the host galaxy masses are inferred from their luminosities. With this data, we are able to pin down the evolution of the M B H /M h ost relation over 85% of the age of the universe. While the MBH /L h ost relation remains nearly unchanged, taking into account the aging of the stellar… Show more
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