3 papers
astro-ph.GA2026
statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys
Elizaveta Sazonova, Cameron R. Morgan, Michael Balogh +16
Quantitative morphology provides a key probe of galaxy evolution across cosmic time and environments. However, these metrics can be biased by changes in imaging quality - resolutio…
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…