most citedThe XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters

96 citations · 96 across the 1 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2020

Environmental dependence of X-ray and optical properties of galaxy clusters

Maria Manolopoulou, Ben Hoyle, Robert G. Mann +2

Galaxy clusters are widely used to constrain cosmological parameters through their properties, such as masses, luminosity and temperature distributions. One should take into accoun…

astro-ph.GA2019

Bubble mapping with the Square Kilometer Array -- I. Detecting galaxies with Euclid, JWST, WFIRST and ELT within ionized bubbles in the intergalactic medium at z>6

Erik Zackrisson, Suman Majumdar, Rajesh Mondal +16

The Square Kilometer Array is expected to provide the first tomographic observations of the neutral intergalactic medium at redshifts z>6 and pinpoint the locations of individual i…

astro-ph.CO2019

Mass Variance from Archival X-ray Properties of Dark Energy Survey Year-1 Galaxy Clusters

A. Farahi, X. Chen, A. E. Evrard +76

Using archival X-ray observations and a log-normal population model, we estimate constraints on the intrinsic scatter in halo mass at fixed optical richness for a galaxy cluster sa…

astro-ph.CO20193 cited

Populations behind the source-subtracted cosmic infrared background anisotropies

A. Kashlinsky, R. G. Arendt, M. Ashby +27

While the upcoming telescopes will reveal correspondingly fainter, more distant galaxies, a question will persist: what more is there that these telescopes cannot see? One answer i…

astro-ph.CO2019

Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters

A. Palmese, J. Annis, J. Burgad +82

We introduce a galaxy cluster mass observable, , based on the stellar masses of cluster members, and we present results for the Dark Energy Survey (DES) Year 1 observation…

astro-ph.CO201985 cited

Dark Energy Survey Year 1 Results: Calibration of Cluster Mis-centering in the redMaPPer Catalogs

Y. Zhang, T. Jeltema, D. L. Hollowood +83

The center determination of a galaxy cluster from an optical cluster finding algorithm can be offset from theoretical prescriptions or -body definitions of its host halo center.…