activity
20212025
most citedMeasuring using X-ray and SZ effect observations of dynamically relaxed galaxy clusters

22 citations · 37 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

Dwarf Galaxies at Cosmic Noon: New JWST Constraints on Satellite Models and Subhalo Tidal Evolution

Jenny T. Wan, Philip Mansfield, Katherine A. Suess +4

The advent of JWST has revolutionized the study of faint satellite galaxies at , enabling statistical constraints on galaxy evolution and the galaxyhalo connection…

astro-ph.GA2025

Decoding the variability in the star-formation histories of z ~ 0.8 galaxies

Jenny T. Wan, Sandro Tacchella, Francesco D'Eugenio +2

The scatter of the star-forming main sequence (SFMS) holds a wealth of information about how galaxies evolve. The timescales encoded in this scatter can provide valuable insight in…

astro-ph.GA2024

Age-dating early quiescent galaxies: high star-formation efficiency, but consistent with direct, higher-redshift observations

Crispin Turner, Sandro Tacchella, Francesco D'Eugenio +9

We present a detailed analysis of JWST/NIRSpec and NIRCam observations of ZF-UDS-7329, a massive, quiescent galaxy at redshift , which has been put forward to challenge cosm…

astro-ph.GA2024

Stochastic prior for non-parametric star-formation histories

Jenny T. Wan, Sandro Tacchella, Benjamin D. Johnson +3

The amount of power contained in the variations in galaxy star-formation histories (SFHs) across a range of timescales encodes key information about the physical processes which mo…

astro-ph.CO2022★ 15 cited

The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 0.60 and M M

Jack Sayers, Adam B. Mantz, Elena Rasia +5

We have combined X-ray observations from Chandra with Sunyaev-Zel'dovich (SZ) effect data from Planck and Bolocam to measure intra-cluster medium pressure profiles from 0.03R$_{500…

astro-ph.CO2021★ 22 cited

Measuring using X-ray and SZ effect observations of dynamically relaxed galaxy clusters

Jenny T. Wan, Adam B. Mantz, Jack Sayers +3

We use a sample of 14 massive, dynamically relaxed galaxy clusters to constrain the Hubble Constant, , by combining X-ray and Sunyaev-Zel'dovich (SZ) effect signals measured w…