Mapping the Growth of Supermassive Black Holes as a Function of Galaxy Stellar Mass and Redshift
Fan Zou, Zhibo Yu, W. N. Brandt, Hyungsuk Tak, Guang Yang, Qingling Ni
arXiv:2404.00097v1 Announce Type: new
Abstract: The growth of supermassive black holes is strongly linked to their galaxies. It has been shown that the population mean black-hole accretion rate ($overline{mathrm{BHAR}}$) primarily correlates with the galaxy stellar mass ($M_star$) and redshift for the general galaxy population. This work aims to provide the best measurements of $overline{mathrm{BHAR}}$ as a function of $M_star$ and redshift over ranges of $10^{9.5}arXiv:2404.00097v1 Announce Type: new
Abstract: The growth of supermassive black holes is strongly linked to their galaxies. It has been shown that the population mean black-hole accretion rate ($overline{mathrm{BHAR}}$) primarily correlates with the galaxy stellar mass ($M_star$) and redshift for the general galaxy population. This work aims to provide the best measurements of $overline{mathrm{BHAR}}$ as a function of $M_star$ and redshift over ranges of $10^{9.5}