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19952025
most citedredMaPPer I: Algorithm and SDSS DR8 Catalog

780 citations · 3.8k across the 63 of their papers we have counts for

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30 papers · 1 filter

astro-ph.CO2025

Euclid preparation. XCI. Validation method for the detections in the Euclid Catalogue of Galaxy Clusters using external data

Euclid Collaboration, J. -B. Melin, S. A. Stanford +315

We present our methodology for identifying known clusters as counterparts to objects in the Euclid Catalogue of Galaxy Clusters (ECGC). Euclid is expected to detect a large number…

astro-ph.CO2025

The XXL Survey LIV. X-ray Luminosity Function and Luminosity-Mass Relation of Optically Selected Galaxy Groups

C. Wood, B. J. Maughan, J. P. Crossett +10

The overlap between the GAMA spectroscopic survey and the XXL X-ray survey was used to study the X-ray properties of optically-selected groups of galaxies. Forced X-ray aperture ph…

astro-ph.CO2023

NIKA2 observations of 3 low-mass galaxy clusters at : pressure profile and - relation

R. Adam, M. Ricci, D. Eckert +64

Three galaxy clusters selected from the XXL X-ray survey at high redshift and low mass ( and M) were observed with NIKA2 to imag…

astro-ph.CO2020★ 8 cited

The XXL survey: XLII. Detection and characterization of the galaxy population of distant galaxy clusters in the XXL-N/VIDEO field: A tale of variety

A. Trudeau, C. Garrel, J. Willis +16

Context. Distant galaxy clusters provide an effective laboratory in which to study galaxy evolution in dense environments and at early cosmic times. Aims. We aim to identify distan…

astro-ph.CO2018★ 131 cited

The XXL Survey XX: The 365 cluster catalogue

C. Adami, P. Giles, E. Koulouridis +54

In the currently debated context of using clusters of galaxies as cosmological probes, the need for well-defined cluster samples is critical. The XXL Survey has been specifically d…

astro-ph.CO2018★ 79 cited

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…