activity
20032026
most citedModelling the Galaxy Bimodality: Shutdown Above a Critical Halo Mass

444 citations · 2.6k across the 41 of their papers we have counts for

collaborators

43 papers

astro-ph.CO2026

Energy deposited by black holes in the hot X-ray gas of elliptical galaxies, groups and clusters

A. Cattaneo, S. Ettori

Galaxy groups show entropy excesses with respect to theoretical expectations from models and simulations with purely gravitational heating. We determine the heat $Q_{\rm heat}…

astro-ph.GA2025

A group of merging galaxies falling onto Abell 2142

Aashiya Anitha Shaji, Anaëlle Hallé, Damir Gasymov +3

Galaxy clusters produce a very hostile environment to galaxies, whose gas gets stripped by ram-pressure, suffer galaxy interactions and witness quenching of their star formation. C…

astro-ph.GA2022★ 8 cited

Probing the link between quenching and morphological evolution

Ioanna Koutsouridou, Andrea Cattaneo

We use a semianalytic model of galaxy formation to compare the predictions of two quenching scenarios: halo quenching and black-hole (BH) quenching. After calibrating both models s…

astro-ph.CO2022

Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl

Hao Fu, Francesco Shankar, Mohammadreza Ayromlou +19

The relative roles of mergers and star formation in regulating galaxy growth are still a matter of intense debate. We here present our DECODE, a new Discrete statistical sEmi-empir…

astro-ph.GA2022★ 4 cited

Cold-mode and hot-mode accretion in galaxy formation: an entropy approach

Édouard Tollet, Andrea Cattaneo, Andrea V. Macciò +1

We have analysed two cosmological zoom simulations with from the NIHAO series, both with and without feedback. We show that an entropy crite…

astro-ph.GA2022★ 49 cited

Coincidence between morphology and star-formation activity through cosmic time: the impact of the bulge growth

Paola Dimauro, Emanuele Daddi, Francesco Shankar +10

The origin of the quenching in galaxies is still highly debated. Different scenarios and processes are proposed. We use multi-band (400-1600 nm) bulge-disc decompositions of massiv…