Secular Evolution and a Non-evolving Black-hole-to-galaxy Mass Ratio in the Last 7 Gyr
Cisternas, M. and Jahnke, K. and Bongiorno, A. and Inskip, K.~J. and Impey, C.~D. and Koekemoer, A.~M. and Merloni, A. and Salvato, M. and Trump, J.~R
Keywords
galaxies: active, galaxies: evolution, galaxies: nuclei
Abstract
We present new constraints on the ratio of black hole (BH) mass to total galaxy stellar mass at 0.3
