Antonio J. Porras-Valverde

activity

20192026

most citedWhy do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?

6 citations · 14 across the 8 of their papers we have counts for

collaborators

Showing 2024 · astro-ph.GAShow all

2 papers · 2 filters

astro-ph.GA2024★ 1 cited

On the signature of black holes on the quenched stellar mass function

Antonio J. Porras-Valverde, John C. Forbes

As star-forming galaxies approach or exceed a stellar mass around $1 0^{11} M_{⊙}$ , they are increasingly likely to be quenched in a process generically called mass quenching. Cen…

astro-ph.GA2024★ 1 cited

The redshift evolution of the $M_{BH} - M_{*}$ scaling relation: new insights from cosmological simulations and semi-analytic models

Shashank Dattathri, Priyamvada Natarajan, Antonio J. Porras-Valverde +4

We study the co-evolution of black holes (BHs) and their host galaxies in the ASTRID and Illustris-TNG300 cosmological simulations and the Dark Sage Semi-Analytic Model (SAM), focu…

On the signature of black holes on the quenched stellar mass function

The redshift evolution of the MBH​−M∗​ scaling relation: new insights from cosmological simulations and semi-analytic models

The redshift evolution of the $M_{BH} - M_{*}$ scaling relation: new insights from cosmological simulations and semi-analytic models