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The Demographics of Broad-line Quasars in the Mass-Luminosity Plane. II. Black Hole Mass and Eddington Ratio Functions

  • Authors: Brandon C. Kelly and Yue Shen

Kelly & Shen 2013 The Astrophysical Journal 764 45.

  • Provider: AAS Journals

Caption: Figure 7.

Constraints on the maximum mass that could be observed in a broad-line quasar as a function of redshift. Symbols are as in Figure 5. The maximum value of M BH for quasars implied by our BHMF is M max BH ~ 4 × 10 10M , although values of 10 10 < M max BH/ M < 10 11 are consistent within the uncertainties. However, as discussed in the text the values of M max BH we derive are highly sensitive to our adopted prior constraints, and the values shown should be treated as lower limits.

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