457 citations · 1.7k across the 27 of their papers we have counts for
27 papers
LEGA-C stellar populations scaling relations. II: Dissecting mass-complete archaeological trends and their evolution since z~0.7 with LEGA-C and SDSS
Anna R. Gallazzi, Stefano Zibetti, Arjen van der Wel +11
With a sample of 552 galaxies at z~0.7 from the LEGA-C survey, we investigate how current star formation influences light-weighted mean stellar ages and metallicities, and their me…
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…
Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions
Kosei Matsumoto, Laura Sommovigo, Andrea Gebek +8
We investigate the impacts of the evolution of dust mass and grain size distribution within a Milky Way-like (MW-like) galaxy simulation on global attenuation curves, focusing on t…
Unusually High Gas-to-Dust Ratios Observed in High-Redshift Quiescent Galaxies
Justin S. Spilker, Katherine E. Whitaker, Desika Narayanan +15
Tracking the cold molecular gas contents of galaxies is critical to understand the interplay between star formation and galaxy growth across cosmic time. Observations of the long-w…
Reconciling extragalactic star formation efficiencies with theory: insights from PHANGS
Sharon E. Meidt, Simon C. O. Glover, Ralf S. Klessen +22
New extragalactic measurements of the cloud population-averaged star formation (SF) efficiency per freefall time from PHANGS show little sign of theoretically predi…
Ages and metallicities of quiescent galaxies: confronting broadband () colours with stellar absorption lines
Chloe M. Cheng, Mariska Kriek, Aliza G. Beverage +9
For decades, studying quiescent galaxies beyond has been challenging due to the reliance on photometric spectral energy distributions, which are highly susceptible to dege…