most citedA refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations

194 citations · 562 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2015110 cited

The cosmic growth of the active black hole population at 1<z<2 in zCOSMOS, VVDS and SDSS

A. Schulze, A. Bongiorno, I. Gavignaud +11

We present a census of the active black hole population at 1<z<2, by constructing the bivariate distribution function of black hole mass and Eddington ratio, employing a maximum li…

astro-ph.GA201426 cited

The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe

Matteo Fossati, David J. Wilman, Fabio Fontanot +6

A well calibrated method to describe the environment of galaxies at all redshifts is essential for the study of structure formation. Such a calibration should include well understo…

astro-ph.GA2014112 cited

The stellar accretion origin of stellar population gradients in massive galaxies at large radii

Michaela Hirschmann, Thorsten Naab, Jeremiah P. Ostriker +5

We investigate the evolution of stellar population gradients from to in massive galaxies at large radii () using ten cosmological zoom simulation…

astro-ph.GA2014194 cited

A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations

Lisa K. Steinborn, Klaus Dolag, Michaela Hirschmann +2

In large scale cosmological hydrodynamic simulations simplified sub-grid models for gas accretion onto black holes and AGN feedback are commonly used. Such models typically depend…

astro-ph.GA2014120 cited

The influence of the environmental history on quenching star formation in a CDM universe

Michaela Hirschmann, Gabriella De Lucia, Dave Wilman +5

We present a detailed analysis of the influence of the environment and of the environmental history on quenching star formation in central and satellite galaxies in the local Unive…