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Evolution of the MBH–σ and MBH–Lbulge Relations
J. H. Woo (Seoul National University), Nicola Bennert (University of California, Santa Barbara), Tommaso Treu (University of California, Santa Barbara), Matthew A. Malkan (University of California, Los Angeles), Roger D. Blandford (Kavli Institute for Particle Astrophysics and Cosmology, Stanford University)
Abstract: Abstract To constrain the origin of scaling relations between black hole mass and galaxy properties, i.e., stellar velocity dispersion and bulge luminosity, we investigate the evolution of scaling relations in the past 6 Gyrs. Over the last three years, we have obtained high signal-to-noise ratio Keck spectra of ~ 50 intermediate luminosity broad-line AGNs at z ~ 0.4 and z ~ 0.6, to measure stellar velocity dispersion, and HST (ACS and NICMOS) images of the same objects (~ 40 so far), to measure bulge luminosity from the two-dimensional AGN-galaxy decomposition analysis. In this paper, we will summarize the main results on the MBH–σ and MBH–bulge luminosity relations and their evolution to the present-day universe. The measured scaling relations show that the relations have evolved significantly in the past 6 billion years, and that black hole growth predates the final galaxy assembly.