collaborators

10 papers

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

The Next Generation Virgo Cluster Survey (NGVS). II. A Catalog of Galaxies in the Virgo Cluster

Laura Ferrarese, Patrick Cote, Lauren A. MacArthur +51

The Next Generation Virgo Cluster Survey (NGVS) is a deep, high resolution imaging campaign that used the 1 deg MegaCam instrument on the Canada-France-Hawaii Telescope to carr…

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.EP2026

How Late Solid Enrichment Shapes Atmospheric Abundances in Giant Planets

Michael L. Balogh, Yuvan Sooryakumar, Sachen Gombu +4

Atmospheric abundance measurements of giant exoplanets are increasingly used to infer their formation histories, motivating upcoming population studies with facilities such as the…

astro-ph.GA2026

The Hubble sequence in JWST CEERS from unbiased galaxy morphologies

Elizaveta Sazonova, Cameron R. Morgan, Michael Balogh

Whether the "Hubble sequence" of galaxy morphologies exists up to z~4 is still disputed, and one of the challenges is characterizing galaxy structure consistently across a wide ran…

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…