collaborators

8 papers

astro-ph.GA2026

Circumgalactic medium depletion drives satellite quenching in IllustrisTNG

Natan de Isídio, Natan de Isídio, Paola Popesso +6

Satellite galaxies dominate the quenched population at low stellar masses (), yet identifying which processes shut down their star formation,…

astro-ph.GA2026

Fishing for Jellyfish Galaxies: Exploring ram-pressure stripping with crowd science

C. Bellhouse, Y. L. Jaffé, J. P. Crossett +13

Aims: We present the first results of Fishing for Jellyfish Galaxies, a pilot citizen-science project using Zooniverse to identify galaxies undergoing ram-pressure stripping (RPS).…

astro-ph.GA2026

Identifying and Distinguishing Quenching Galaxies with Spatially Resolved Star Formation in the Hubble Frontier Fields

Cameron Lawlor-Forsyth, Michael L. Balogh, Sean L. McGee +1

We investigate the nature and prevalence of different quenching signatures for 1437 galaxies with and $\text{SFR} \geqslant 10^{-3}~M_{\…

astro-ph.GA2026

Identifying and Distinguishing Quenching Galaxies with Spatially Resolved Star Formation in Mock CASTOR and NGRST Observations

Cameron Lawlor-Forsyth, Michael L. Balogh, Sean L. McGee +1

We present synthetic images of galaxies that are in the stages of star formation quenching for the Cosmological Advanced Survey Telescope for Optical and UV Research (CASTOR) and N…

astro-ph.GA2026

A hydrodynamical CLONE of the Virgo cluster: II. Confronting observed and synthetic galaxy population twins in a dense environment

Jenny G. Sorce, Sean L. McGee, Yohan Dubois +3

Galaxy clusters offer powerful laboratories for studying galaxy evolution in dense environments. In this context, the Constrained LOcal and Nesting Environment (CLONE) project prov…

astro-ph.GA2026

Cosmic web stripping and starvation of low-mass filament galaxies in TNG50

Daria Zakharova, Gabriella De Lucia, Benedetta Vulcani +3

Galaxy properties are known to correlate with their location within the cosmic web. However, the role of filaments remains poorly understood, particularly for low-mass galaxies, wh…