156 citations · 2.9k across the 252 of their papers we have counts for
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AMICO galaxy clusters in KiDS-DR3: sample properties and selection function
Matteo Maturi, Fabio Bellagamba, Mario Radovich +5
We present the first catalogue of galaxy cluster candidates derived from the third data release of the Kilo Degree Survey (KiDS-DR3). The sample of clusters has been produced using…
The XXL Survey XXV. Cosmological analysis of the C1 cluster number counts
F. Pacaud, M. Pierre, J. -B. Melin +25
Context. We present an estimation of cosmological parameters with clusters of galaxies. Aims. We constrain the , , and parameters from a stand-alone sample of X-ray c…
AMICO galaxy clusters in KiDS-DR3: weak-lensing mass calibration
Fabio Bellagamba, Mauro Sereno, Mauro Roncarelli +8
We present the mass calibration for galaxy clusters detected with the AMICO code in KiDS DR3 data. The cluster sample comprises 7000 objects and covers the redshift range 0.…
Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters
Arpine Kozmanyan, Hervé Bourdin, Pasquale Mazzotta +2
The possibility of determining the value of the Hubble constant using observations of galaxy clusters in X-ray and microwave wavelengths through the Sunyaev Zeldovich (SZ) effect h…
The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
F. Marulli, A. Veropalumbo, M. Sereno +20
Galaxy clusters trace the highest density peaks in the large-scale structure of the Universe. Their clustering provides a powerful probe that can be exploited in combination with c…
Gravitational lensing detection of an extremely dense environment around a galaxy cluster
Mauro Sereno, Carlo Giocoli, Luca Izzo +8
Galaxy clusters form at the highest density nodes of the cosmic web. The clustering of massive halos is enhanced relative to the general mass distribution and matter beyond the vir…