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Table · dataset · 2023

PS1 z>5.6 QSO Survey. III. z~6 quasar LF

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We present the z~6 type-1 quasar luminosity function (QLF), based on the Pan-STARRS1 (PS1) quasar survey.

Description

The PS1 sample includes 125 quasars at z~5.7-6.2, with -28<~M_1450_<~-25. With the addition of 48 fainter quasars from the SHELLQs survey, we evaluate the z~6 QLF over -28<~M_1450_<~-22.

Adopting a double power law with an exponential evolution of the quasar density ({Phi}(z){propto}10^k(z-6)^; k=-0.7), we use a maximum likelihood method to model our data. We find a break magnitude of M^*^=-26.38_-0.60_^+0.79^mag, a faint-end slope of {alpha}=-1.70_-0.19_^+0.29^, and a steep bright-end slope of {beta}=-3.84_-1.21_^+0.63^. Based on our new QLF model, we determine the quasar comoving spatial density at z~6 to be n(M_1450_{<}-26)=1.16_-0.12_^+0.13^cGpc^-3^.

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In comparison with the literature, we find the quasar density to evolve with a constant value of k~-0.7, from z~7 to z~4. Additionally, we derive an ionizing emissivity of {epsilon}_912_(z=6)=7.23_-1.02_^+1.65^x10^22^erg/s/Hz/cMpc^3^, based on the QLF measurement. Given standard assumptions, and the recent measurement of the mean free path by Becker+ 2021MNRAS.508.1853B at z~6, we calculate an HI photoionizing rate of {Gamma}HI(z=6)~6x10^-16^s^-1^, strongly disfavoring a dominant role of quasars in hydrogen reionization.

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