collaborators

12 papers

astro-ph.GA2026

MAUVE-MUSE: When Metallicity Follows or Fights Star Formation -- A Mass-Dependent Inversion in Virgo Galaxies

Rongjun Huang, Luca Cortese, Barbara Catinella +11

Although globally-integrated studies often find that, at fixed stellar mass, high star formation rate (SFR) galaxies are relatively metal-poor while lower-SFR systems are more meta…

astro-ph.GA2026

A Comprehensive Analysis of WISE Mid-Infrared Colors for Obscured AGN Selection

Anika Goel, Samir Salim, Sara L. Ellison +4

In this paper, we investigate the robustness of WISE mid-IR color selection (W1-W2) for identifying obscured (Type 2) active galactic nuclei (AGNs) at low redshift (z<0.3), using a…

astro-ph.GA2026

EMBERS I: Low redshift post-starburst galaxies are frequently depleted in molecular gas relative to star forming progenitors

Ben F. Rasmussen, María Jesús Jiménez-Donaire, Sara L. Ellison +10

The cold gas content of post-starburst galaxies (PSBs) provides important insight into the mechanisms that drive rapid quenching, but a multiphase assessment of both the atomic and…

astro-ph.GA2025

SDSS-ALMA Legacy Value Archival Gas Exploration (SALVAGE) -- I: global star formation is governed by central (not global) molecular gas

Scott Wilkinson, Toby Brown, Chiara Circosta +3

Star-forming galaxies form tight relations between their stellar mass, star-formation rate, and molecular gas reservoir on global and resolved scales. On the path to quiescence, th…

astro-ph.GA2025

Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE)

Barbara Catinella, Luca Cortese, Jiayi Sun +26

The Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE) project is a multi-facility programme exploring how dense environments transform galaxies. Combining a VLT/MUSE…

astro-ph.GA2025

Star Formation Rates, Metallicities, and Stellar Masses on kpc-scales in TNG50

Jia Qi, Alex M. Garcia, Davis Robinson +7

Integral field units (IFU) have extended our knowledge of galactic properties to kpc (or, sometimes, even smaller) patches of galaxies. These scales are where the physics driving g…