activity
20082026
most citedDensity profile of dark matter haloes and galaxies in the Horizon-AGN simulation: the impact of AGN feedback

145 citations · 195 across the 12 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2025

Beyond Extreme Burstiness: Evolving Star Formation Efficiency as the Key to Early Galaxy Abundance

Abhijnan Kar, Shadab Alam, Joseph Silk

JWST observations have revealed an overabundance of bright galaxies at , creating apparent tensions with theoretical predictions within standard CDM cosmology. We addr…

astro-ph.GA2024

Supermassive black hole growth in hierarchically merging nuclear star clusters

Konstantinos Kritos, Ricarda S. Beckmann, Joseph Silk +5

Supermassive black holes are prevalent at the centers of massive galaxies, and their masses scale with galaxy properties, increasing evidence suggesting that these trends continue…

astro-ph.GA2024★ 1 cited

TRINITY VI: Connection between Galaxy Star Formation Rates and Supermassive Black Hole Accretion Rates from z=0-10

Haowen Zhang, Peter Behroozi, Marta Volonteri +6

We infer supermassive black hole (SMBH) accretion rates and Eddington ratios as a function of SMBH/host galaxy mass and redshift with the empirical TRINITY model of dark matter hal…

astro-ph.GA2024

Which came first: supermassive black holes or galaxies? Insights from JWST

Joseph Silk, Mitchell Begelman, Colin Norman +2

Insights from JWST observations suggest that AGN feedback evolved from a short-lived, high redshift phase in which radiatively cooled turbulence and/or momentum-conserving outflows…

astro-ph.GA2016★ 145 cited

Density profile of dark matter haloes and galaxies in the Horizon-AGN simulation: the impact of AGN feedback

S. Peirani, Y. Dubois, M. Volonteri +7

Using a suite of three large cosmological hydrodynamical simulations, Horizon-AGN, Horizon-noAGN (no AGN feedback) and Horizon-DM (no baryons), we investigate how a typical sub-gri…