most citedEarly results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field

11 citations · 16 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.IM2024

A forward-modelling approach to overcome PSF smearing and fit flexible models to the chemical structure of galaxies

Benjamin Metha, Simon Birrer, Tommaso Treu +3

Historically, metallicity profiles of galaxies have been modelled using a radially symmetric, two-parameter linear model, which reveals that most galaxies are more metal-rich in th…

astro-ph.GA2024

A geostatistical analysis of multiscale metallicity variations in galaxies -- III. Spatial resolution and data quality limits

Benjamin Metha, Michele Trenti, Andrew Battisti +1

Geostatistical methods are powerful tools for understanding the spatial structure of the metallicity distribution of galaxies, and enable construction of accurate predictive models…

astro-ph.GA202311 cited

Early results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field

Benedetta Vulcani, Tommaso Treu, Antonello Calabro +26

We combine JWST/NIRCam imaging and MUSE data to characterize the properties of galaxies in different environmental conditions in the cluster Abell2744 () and in its immed…

astro-ph.GA20235 cited

The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts

Benjamin Metha, Michele Trenti

Massive stars are thought to be progenitors of Long Gamma Ray Bursts (GRBs), most likely with a bias favouring low metallicity progenitors. Because galaxies do not have a constant…