activity
20152017
most citedDark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data

166 citations · 380 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.CO201740 cited

Galaxy Cluster Mass Reconstruction Project: III. The impact of dynamical substructure on cluster mass estimates

L. Old, R. Wojtak, F. R. Pearce +14

With the advent of wide-field cosmological surveys, we are approaching samples of hundreds of thousands of galaxy clusters. While such large numbers will help reduce statistical un…

astro-ph.CO20176 cited

Complex diffuse emission in the cluster PLCK~G004.5-19.5

J. G. Albert, C. Sifón, A. Stroe +4

We present radio observations of the galaxy cluster PLCK G004.5-19.5 () using the Giant Metrewave Radio Telescope at 150~MHz, 325~MHz, and 610~MHz. We find an unusual arran…

astro-ph.GA2017128 cited

The abundance of ultra-diffuse galaxies from groups to clusters: UDGs are relatively more common in more massive haloes

Remco F. J. van der Burg, Henk Hoekstra, Adam Muzzin +17

In recent years, multiple studies have reported substantial populations of large, low-surface-brightness galaxies in local galaxy clusters. Various theories that aim to explain the…

astro-ph.GA2016

The evolution in the stellar mass of Brightest Cluster Galaxies over the past 10 billion years

Sabine Bellstedt, Chris Lidman, Adam Muzzin +14

Using a sample of 98 galaxy clusters recently imaged in the near infra-red with the ESO NTT, WIYN and WHT telescopes, supplemented with 33 clusters from the ESO archive, we measure…

astro-ph.GA2015166 cited

Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data

M. Viola, M. Cacciato, M. Brouwer +24

The Kilo-Degree Survey (KiDS) is an optical wide-field survey designed to map the matter distribution in the Universe using weak gravitational lensing. In this paper, we use these…