Quasar Luminosity Function at z = 7
arXiv:2305.11225 · doi:10.3847/2041-8213/acd69f
Abstract
We present the quasar luminosity function (LF) at , measured with 35 spectroscopically confirmed quasars at . The sample of 22 quasars from the Subaru High- Exploration of Low-Luminosity Quasars (SHELLQs) project, combined with 13 brighter quasars in the literature, covers an unprecedentedly wide range of rest-frame ultraviolet magnitudes over . We found that the binned LF flattens significantly toward the faint end populated by the SHELLQs quasars. A maximum likelihood fit to a double power-law model has a break magnitude , a characteristic density Gpc mag, and a bright-end slope , when the faint-end slope is fixed to as observed at . The overall LF shape remains remarkably similar from to , while the amplitude decreases substantially toward higher redshifts, with a clear indication of an accelerating decline at . The estimated ionizing photon density, s Mpc, is less than 1 % of the critical rate to keep the intergalactic medium ionized at , and thus indicates that quasars are not a major contributor to cosmic reionization.
The Astrophysical Journal Letters, in press
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