activity
20052025
most citedStellar Masses and SFRs for 1M Galaxies from SDSS and WISE

258 citations · 2.3k across the 37 of their papers we have counts for

collaborators

36 papers

astro-ph.GA2025★ 1 cited

The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at

Angelos Nersesian, Yasha Kaushal, Marco Martorano +9

We analyzed the sizes and star-formation histories (SFHs) of 2908 galaxies with M at , drawn from the LEGA-C survey. The goal is to inves…

astro-ph.GA2025★ 2 cited

LEGA-C stellar populations scaling relations. I: Chemo-archaeological downsizing trends at z~0.7

Anna R. Gallazzi, Stefano Zibetti, Arjen van der Wel +11

We analyze stellar population properties of 552 galaxies at redshift 0.6<z<0.77 from the LEGA-C spectroscopic survey. This first paper in a series presents the catalog of revised a…

astro-ph.GA2025★ 5 cited

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.GA2025★ 2 cited

MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe

Adam Muzzin, Katherine A. Suess, Danilo Marchesini +81

We present an overview of the MINERVA survey, a 259.8 hour (prime) and 127 hour (parallel) Cycle 4 treasury program on the James Webb Space Telescope (JWST). MINERVA is obtaining 8…

astro-ph.GA2025★ 3 cited

Even redder than we knew: color and evolution up to from JWST/NIRCam photometry

A. van der Wel, M. Martorano, D. Marchesini +14

JWST/NIRCam provides rest-frame near-IR photometry of galaxies up to with exquisite depth and accuracy. This affords an unprecedented view of the evolution of the UV-optica…

astro-ph.GA2025★ 9 cited

A Cosmic Miracle: A Remarkably Luminous Galaxy at Confirmed with JWST

Rohan P. Naidu, Pascal A. Oesch, Gabriel Brammer +43

JWST has revealed a stunning population of bright galaxies at surprisingly early epochs, , where few such sources were expected. Here we present the most distant example of t…