activity
20142019
most citedLoCuSS: Testing hydrostatic equilibrium in galaxy clusters

121 citations · 287 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2019★ 48 cited

Detection of anti-correlation of hot and cold baryons in galaxy clusters

Arya Farahi, Sarah L. Mulroy, August E. Evrard +10

The largest clusters of galaxies in the Universe contain vast amounts of dark matter, plus baryonic matter in two principal phases, a majority hot gas component and a minority cold…

astro-ph.CO2019★ 63 cited

LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content

Sarah L. Mulroy, Arya Farahi, August E. Evrard +13

We present a simultaneous analysis of galaxy cluster scaling relations between weak-lensing mass and multiple cluster observables, across a wide range of wavelengths, that probe bo…

astro-ph.CO2017★ 19 cited

Galaxy cluster luminosities and colours, and their dependence on cluster mass and merger state

Sarah L. Mulroy, Sean L. McGee, Steven Gillman +5

We study a sample of 19 galaxy clusters in the redshift range with highly complete spectroscopic membership catalogues (to ) from the Arizona…

astro-ph.GA2015★ 17 cited

The XXL Survey X: K-band luminosity - weak-lensing mass relation for groups and clusters of galaxies

F. Ziparo, G. P. Smith, S. L. Mulroy +15

We present the K-band luminosity-halo mass relation, , for a subsample of 20 of the 100 brightest clusters in the XXL Survey observed with WIRCam at the Canad…

astro-ph.CO2015★ 121 cited

LoCuSS: Testing hydrostatic equilibrium in galaxy clusters

G. P. Smith, P. Mazzotta, N. Okabe +17

We test the assumption of hydrostatic equilibrium in an X-ray luminosity selected sample of 50 galaxy clusters at from the Local Cluster Substructure Survey (LoCuSS).…

astro-ph.CO2014★ 19 cited

LoCuSS: The Near-Infrared Luminosity and Weak-Lensing Mass Scaling Relation of Galaxy Clusters

Sarah L. Mulroy, Graham P. Smith, Chris P. Haines +7

We present the first scaling relation between weak-lensing galaxy cluster mass, , and near-infrared luminosity, . Our results are based on 17 clusters observed with wi…