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20042026
most citedCALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation

1.3k citations · 14.1k across the 171 of their papers we have counts for

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Showing 2025Show all

18 papers · 1 filter

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

Localized Deviations from the CO-PAH Relation in PHANGS-JWST Galaxies: Faint PAH Emission or Elevated CO Emissivity?

Jaeyeon Kim, Adam K. Leroy, Karin Sandstrom +25

Polycyclic aromatic hydrocarbon (PAH) emission is widely used to trace the distribution of molecular gas in the interstellar medium, exhibiting a tight correlation with CO(2-1) emi…

astro-ph.GA2025

PHANGS-JWST: the largest extragalactic molecular cloud catalog traced by polycyclic aromatic hydrocarbon emission

Z. Bazzi, D. Colombo, F. Bigiel +25

High-resolution JWST images of nearby spiral galaxies reveal polycyclic aromatic hydrocarbon (PAH) emission structures that trace molecular gas, including CO-dark regions. We ident…

astro-ph.GA2025★ 8 cited

The PHANGS-MUSE/HST-Halpha Nebulae Catalogue

A. T. Barnes, R. Chandar, K. Kreckel +38

We present the PHANGS-MUSE/HST-Halpha nebulae catalogue, comprising 5177 spatially resolved nebulae across 19 nearby star-forming galaxies (< 20 Mpc), based on high-resolution Halp…

astro-ph.GA2025

Masses, Star-Formation Efficiencies, and Dynamical Evolution of 18,000 HII Regions

Debosmita Pathak, Adam K. Leroy, Ashley. T. Barnes +36

We present measurements of the masses associated with HII regions across 19 nearby star-forming galaxies by combining data from JWST, HST, MUSE, ALMA, VLA, and MeerKAT…

astro-ph.GA2025★ 3 cited

Transforming galaxies with EASE: widespread structural changes enabled by short-lived spirals

Arjen van der Wel, Sharon E. Meidt

We propose that galaxy structural changes - and the rapid rise of a population of galaxies with early-type morphologies at cosmic noon () - can be explained with EASE: Early…