Black Hole Growth Is Mainly Linked to Host-galaxy Stellar Mass Rather Than Star Formation Rate - Yang, G.; Chen, C.-T. J.; Vito, F.; Brandt, W. N.; Alexander, D. M.; Luo, B.; Sun, M. Y.; Xue, Y. Q.; Bauer, F. E.; Koekemoer, A. M.; Lehmer, B. D.; Liu, T.; et al. (The Astrophysical journal, 2017)
Keywords: Astrophysics; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; BLACK HOLES; COMPARATIVE EVALUATIONS; ENERGY SPECTRA; GALACTIC EVOLUTION; Galaxies; galaxies: active; galaxies: evolution; galaxies: nuclei; GALAXY NUCLEI; MASS; QUASARS; quasars: supermassive black holes; RED SHIFT; Space telescopes; Spectral energy distribution; Star & galaxy formation; Star formation; Star formation rate; STARS; Stars & galaxies; Stellar mass; Stellar mass accretion; Supermassive black holes; X-RAY GALAXIES; X-rays: galaxies