1 code implementation • 17 Dec 2015 • P. Ranalli, E. Koulouridis, I. Georgantopoulos, S. Fotopoulou, L. -T. Hsu, M. Salvato, A. Comastri, M. Pierre, N. Cappelluti, F. J. Carrera, L. Chiappetti, N. Clerc, R. Gilli, K. Iwasawa, F. Pacaud, S. Paltani, E. Plionis, C. Vignali
The binned luminosity function and its evolution is determined with a variant of the Page-Carrera method, improved to include corrections for absorption and to account for the full probability distribution of photometric redshifts.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
1 code implementation • 28 Nov 2003 • A. Marconi, G. Risaliti, R. Gilli, L. K. Hunt, R. Maiolino, M. Salvati
We quantify the importance of mass accretion during AGN phases in the growth of supermassive black holes (BH) by comparing the mass function of black holes in the local universe with that expected from AGN relics, which are black holes grown entirely with mass accretion during AGN phases.
astro-ph
