TY - JOUR

T1 - Demographics of z similar to 6 quasars in the black hole mass-luminosity plane

AU - Wu, Jin

AU - Shen, Yue

AU - Jiang, Linhua

AU - Banados, Eduardo

AU - Fan, Xiaohui

AU - Ho, Luis C.

AU - Vestergaard, Marianne

AU - Wang, Feige

AU - Wang, Shu

AU - Wu, Xue-Bing

AU - Yang, Jinyi

PY - 2022/10/18

Y1 - 2022/10/18

N2 - We study the demographics of z similar to 6 broad-line quasars in the black hole (BH) mass-luminosity plane using a sample of more than 100 quasars at 5.7 < z < 6.5. These quasars have well-quantified selection functions and nearly one-third of them also have virial BH masses estimated from near-IR spectroscopy. We use forward modelling of parametrized intrinsic distributions of BH masses and Eddington ratios, and account for the sample flux limits and measurement uncertainties of the BH masses and luminosities. We find significant differences between the intrinsic and observed distributions of the quantities due to measurement uncertainties and sample flux limits. There is also marginal evidence that the virial BH masses are susceptible to a positive luminosity-dependent bias (BH mass is overestimated when luminosity is above the average), and that the mean Eddington ratio increases with BH mass. Our models provide reliable constraints on the z similar to 6 BH mass function at M-BH > 10(8.5) M-circle dot, with a median 1 sigma uncertainty of similar to 0.5 dex in abundance. The intrinsic Eddington ratio distribution of M-BH > 10(8.5) M-circle dot quasars can be approximated by a mass-dependent Schechter model, with a broad peak around log (L-bol/L-Edd)similar to -0.9. We also find that, at 4.5 less than or similar to z less than or similar to 6, the number densities of more massive BHs tend to decline more rapidly with increasing redshift, contrary to the trend at 2.5 less than or similar to z less than or similar to 4.5 reported previously.

AB - We study the demographics of z similar to 6 broad-line quasars in the black hole (BH) mass-luminosity plane using a sample of more than 100 quasars at 5.7 < z < 6.5. These quasars have well-quantified selection functions and nearly one-third of them also have virial BH masses estimated from near-IR spectroscopy. We use forward modelling of parametrized intrinsic distributions of BH masses and Eddington ratios, and account for the sample flux limits and measurement uncertainties of the BH masses and luminosities. We find significant differences between the intrinsic and observed distributions of the quantities due to measurement uncertainties and sample flux limits. There is also marginal evidence that the virial BH masses are susceptible to a positive luminosity-dependent bias (BH mass is overestimated when luminosity is above the average), and that the mean Eddington ratio increases with BH mass. Our models provide reliable constraints on the z similar to 6 BH mass function at M-BH > 10(8.5) M-circle dot, with a median 1 sigma uncertainty of similar to 0.5 dex in abundance. The intrinsic Eddington ratio distribution of M-BH > 10(8.5) M-circle dot quasars can be approximated by a mass-dependent Schechter model, with a broad peak around log (L-bol/L-Edd)similar to -0.9. We also find that, at 4.5 less than or similar to z less than or similar to 6, the number densities of more massive BHs tend to decline more rapidly with increasing redshift, contrary to the trend at 2.5 less than or similar to z less than or similar to 4.5 reported previously.

KW - methods: statistical

KW - galaxies: active

KW - quasars: supermassive black holes

KW - DIGITAL SKY SURVEY

KW - REVERBERATION MAPPING PROJECT

KW - NEAR-INFRARED SPECTROSCOPY

KW - ACTIVE GALACTIC NUCLEI

KW - QSO REDSHIFT SURVEY

KW - HIGH-Z EXPLORATION

KW - DISTANT QUASARS

KW - LINE WIDTHS

KW - EVOLUTION

KW - GALAXIES

U2 - 10.1093/mnras/stac2833

DO - 10.1093/mnras/stac2833

M3 - Journal article

VL - 517

SP - 2659

EP - 2676

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 2

ER -