papers

Publications (40)

astro-ph.GA2019

The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe

Viviana Casasola, Simone Bianchi, Pieter De Vis +18

The purpose of this work is the characterization of the main scaling relations between all the ISM components (dust, atomic/molecular/total gas), gas-phase metallicity, and other g…

astro-ph.GA2019

Revealing the dust attenuation properties on resolved scales in NGC628 with SWIFT UVOT data

Marjorie Decleir, Ilse De Looze, Médéric Boquien +8

Understanding how dust attenuation laws vary between and within galaxies is a key question if we want to reliably measure the physical properties of galaxies at both global and loc…

astro-ph.GA2025

Evolution and Mass Dependence of UV-to-near-IR Color Gradients up to z=2.5 from HST+JWST

Marco Martorano, Arjen van der Wel, Andrea Gebek +7

We present the redshift evolution of radial color gradients (in rest-frame and ) for galaxies in the range z $<2.5…

astro-ph.GA2024

The Size-Mass relation at Rest-Frame m from JWST/NIRCam in the COSMOS-WEB and PRIMER-COSMOS fields

Marco Martorano, Arjen van der Wel, Maarten Baes +4

We present the galaxy stellar mass - size relation in the rest-frame near-IR () and its evolution with redshift up to . Sérsic profiles are measured for $…

astro-ph.GA2023

A simple spectroscopic technique to identify rejuvenating galaxies

Junyu Zhang, Yijia Li, Joel Leja +4

Rejuvenating galaxies are unusual galaxies that fully quench and then subsequently experience a "rejuvenation" event to become star-forming once more. Rejuvenation rates vary subst…

astro-ph.GA2024

Age and metal gradients in massive quiescent galaxies at : implications for quenching and assembly histories

Chloe M. Cheng, Mariska Kriek, Aliza G. Beverage +12

We present spatially resolved, simple stellar population equivalent ages, stellar metallicities, and abundance ratios for 456 massive ($10.3\lesssim\log(\mathrm{M}_*/\mathrm{M}_\od…