The Bolometric Quasar Luminosity Function at z = 0-7

Understand

In this paper, we provide updated constraints on the bolometric quasar luminosity function (QLF) from $z=0$ to $z=7$.

• The constraints are based on an observational compilation that includes observations in the rest-frame IR, B band, UV, soft and hard X-ray in past decades.
• Our method follows Hopkins et al.
• 2007 with an updated quasar SED model and bolometric and extinction corrections.