activity
20002010
most citedFormation of Supermassive Black Holes by Direct Collapse in Pregalactic Halos

857 citations · 3.8k across the 25 of their papers we have counts for

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Showing 2006Show all

8 papers · 1 filter

astro-ph200614 cited

Modeling active galactic nuclei: ongoing problems for the faint-end of the luminosity function

F. Marulli, E. Branchini, L. Moscardini +1

We consider simple semi-analytic models that relate the active galactic nuclei (AGN) evolution to the merging history of their host dark matter haloes and quantify their ability of…

astro-ph200691 cited

The importance of dry and wet merging on the formation and evolution of elliptical galaxies

L. Ciotti, B. Lanzoni, M. Volonteri

With the aid of a simple yet robust approach we investigate the influence of dissipationless and dissipative merging on galaxy structure, and the consequent effects on the scaling…

astro-ph200635 cited

Unresolved X-ray background: clues on galactic nuclear activity at z>6

R. Salvaterra, F. Haardt, M. Volonteri

We study, by means of dedicated simulations of massive black hole build-up, the possibility to constraint the existence and nature of the AGN population at z>6 with available and p…

astro-ph20061 cited

Supermassive black hole mergers and cosmological structure formation

Marta Volonteri

Massive black holes (MBHs), with masses in the range 10^3-10^8 Msolar, which merge with a companion black hole of similar mass are expected to be the most powerful source of gravit…

astro-ph2006205 cited

Quasars at z=6: the survival of the fittest

M. Volonteri, M. J. Rees

The Sloan Digital Sky survey detected luminous quasars at very high redshift, z>6. Follow-up observations indicated that at least some of these quasars are powered by supermassive…

astro-ph200646 cited

Constraints on the Accretion History of Massive Black Holes from Faint X-ray Counts

Marta Volonteri, Ruben Salvaterra, Francesco Haardt

We investigate how hierarchical models for the co-evolution of the massive black hole (MBH) and AGN population can reproduce the observed faint X-ray counts. We find that the main…