Distant Quasars: Black hole mass growth and dust emission

  • Jun, Hyunsung D. (Jet Propulsion Laboratory)
  • Published : 2015.04.10

Abstract

The massive limit of black holes (BHs) is observed as present day ten billion solar masses. We search for observational signatures of BHs that become extremely massive (EMBHs, 1-10 billion solar masses). I will report on the evolution of active galactic nuclei (AGNs) through the growth of BH mass and their dust emission strength. First, we measured 26 EMBH masses of quasars at 1

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