activity
20242026
collaborators

4 papers

astro-ph.GA2026

Identifying and distinguishing quenching galaxies with spatially resolved star formation in TNG50

Cameron Lawlor-Forsyth, Michael L. Balogh, Elizaveta Sazonova +3

Using the TNG50 simulation, we determine observationally motivated metrics that can distinguish quenching galaxies from star forming galaxies for $M_{*} \geqslant 10^{9.5}~M_{\odot…

astro-ph.GA2025

Deep galaxy stellar mass functions as a function of star formation rate in the Virgo cluster environment

Cameron R. Morgan, Elizaveta Sazonova, Ian D. Roberts +8

We analyze deep () galaxy stellar mass functions (SMFs) of the Virgo cluster using stellar masses derived as part of the Next Generation Virgo Survey (N…

astro-ph.GA2025

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XVIII. Reconstructing the star formation history of early-type galaxies through the combination of their UV and H emission

S. Martocchia, A. Boselli, C. Maraston +21

We reconstruct the SFHs of 7 massive () early-type galaxies (ETGs) in the Virgo cluster by analysing their spatially resolved stellar population…

astro-ph.GA2024

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE): XVI. The ubiquity of truncated star-forming disks across the Virgo cluster environment

C. R. Morgan, M. L. Balogh, A. Boselli +14

We examine the prevalence of truncated star-forming disks in the Virgo cluster down to . This work makes use of deep, high-resolution imaging in…