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19992026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 29.8k across the 268 of their papers we have counts for

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astro-ph.CO2017★ 8 cited

ATCA observations of the MACS-Planck Radio Halo Cluster Project II. Radio observations of an intermediate redshift cluster sample

G. Martinez Aviles, M. Johnston-Hollitt, C. Ferrari +16

A fraction of galaxy clusters host diffuse radio sources whose origins are investigated through multi-wavelength studies of cluster samples. We investigate the presence of diffuse…

astro-ph.CO2017★ 23 cited

Sub-structure and merger detection in resolved NIKA Sunyaev-Zel'dovich images of distant clusters

R. Adam, O. Hahn, F. Ruppin +48

Sub-structures in the hot gas of galaxy clusters are related to their formation history and to the astrophysical processes at play in the intracluster medium (ICM). The thermal Sun…

astro-ph.CO2017★ 71 cited

First Sunyaev-Zel'dovich mapping with the NIKA2 camera: Implication of cluster substructures for the pressure profile and mass estimate

F. Ruppin, F. Mayet, G. W. Pratt +37

The complete characterization of the pressure profile of high-redshift galaxy clusters, from their core to their outskirts, is a major issue for the study of the formation of large…

astro-ph.IM2017★ 9 cited

French SKA White Book - The French Community towards the Square Kilometre Array

F. Acero, J. -T. Acquaviva, R. Adam +175

The "Square Kilometre Array" (SKA) is a large international radio telescope project characterised, as suggested by its name, by a total collecting area of approximately one square…

astro-ph.CO2017

NIKA2: a mm camera for cluster cosmology

J. F. Macias-Perez, R. Adam, P. Ade +37

Galaxy clusters constitute a major cosmological probe. However, Planck 2015 results have shown a weak tension between CMB-derived and cluster-derived cosmological parameters. This…

astro-ph.CO2017★ 16 cited

Internal dark matter structure of the most massive galaxy clusters

Amandine M. C. Le Brun, Monique Arnaud, Gabriel W. Pratt +1

We investigate the evolution of the dark matter density profiles of the most massive galaxy clusters in the Universe. Using a `zoom-in' procedure on a large suite of cosmological s…