activity
20242026
most citedInsights into environmental quenching at : an enhancement of faint, low-mass passive galaxies in clusters

4 citations · 5 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

MAGAZ3NE: Dust Deficiency in Ultramassive Quiescent Galaxies at with ALMA Observations

Wenjun Chang, Gillian Wilson, Ben Forrest +14

A major challenge in identifying massive quiescent galaxies at is distinguishing truly passive systems from dust-obscured star-forming galaxies, as both populations exhibit s…

astro-ph.GA2025

MAGAZ3NE: Far-IR and Radio Insights into the Nature and Properties of Ultramassive Galaxies at

Wenjun Chang, Gillian Wilson, Ben Forrest +12

Deep and wide-field near-infrared (NIR) surveys have recently discovered and confirmed ultramassive galaxies (UMGs; ) spectroscopically at high redsh…

astro-ph.GA2025

Excavating The Ruins: an Ancient Galaxy Which Formed in the First 500 Myr

Ian McConachie, Jacqueline Antwi-Danso, Wenjun Chang +14

We present the analysis of an ancient galaxy at which we dub ``Eridu.'' Simultaneously modeling the JWST/NIRSpec G140M and G235M spectra from the SMILES program and $0.4-…

astro-ph.GA2025

A massive and evolved slow-rotating galaxy in the early Universe

Ben Forrest, Adam Muzzin, Danilo Marchesini +15

In the contemporary Universe, most galaxies are supported by ordered rotation, yet a significant subset of the most massive and quiescent systems are dominated by random stellar mo…

astro-ph.GA20251 cited

CANUCS/Technicolor Data Release 1: Imaging, Photometry, Slit Spectroscopy, and Stellar Population Parameters

Ghassan T. E. Sarrouh, Yoshihisa Asada, Nicholas S. Martis +44

We present the first data release of the CAnadian NIRISS Unbiased Cluster Survey (CANUCS), a JWST Cycle 1 GTO program targeting 5 lensing clusters and flanking fields in parallel (…

astro-ph.GA2025

Distinct origins of environmentally quenched galaxies in the core and outer virialised regions of massive clusters at

Guillaume Hewitt, Florian Sarron, Michael L. Balogh +15

High-redshift () galaxy clusters are the domain where environmental quenching mechanisms are expected to emerge as important factors in the evolution of the quiescent galax…