activity
19942026
most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

1k citations · 5.6k across the 137 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

astro-ph.CO2019★ 4 cited

A rare case of FR I interaction with a hot X-ray bridge in the A2384 galaxy cluster

V. Parekh, T. F. Laganá, K. Thorat +3

Clusters of varying mass ratios can merge and the process significantly disturbs the cluster environments and alters their global properties. Active radio galaxies are another phen…

astro-ph.CO2019★ 26 cited

Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection

Euclid Collaboration, R. Adam, M. Vannier +56

Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test cosmological models. This method requires an efficient blind detection of clust…

astro-ph.GA2019★ 21 cited

The complex case of MACSJ0717.5+3745 and its extended filament: intra-cluster light, galaxy luminosity function, and galaxy orientations

A. Ellien, F. Durret, C. Adami +3

The properties of galaxies are known to be affected by their environment, but although galaxies in clusters and groups have been quite thoroughly investigated, little is known pres…

astro-ph.GA2019★ 5 cited

The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey II. X-ray and optical properties of the cluster sample

Ali Takey, Florence Durret, Isabel Márquez +3

We present X-ray and optical properties of the optically confirmed galaxy cluster sample from the 3XMM/SDSS Stripe 82 cluster survey. The sample includes 54 galaxy clusters in the…

astro-ph.GA2019★ 105 cited

Pre-processing of galaxies in cosmic filaments around AMASCFI clusters in the CFHTLS

Florian Sarron, Christophe Adami, Florence Durret +1

Galaxy clusters and groups are thought to accrete material along the preferred direction of cosmic filaments. Yet these structures have proven difficult to detect due to their low…

astro-ph.CO2019★ 31 cited

Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters

T. F. Laganá, F. Durret, P. A. A. Lopes

We analysed XMM-{\it Newton} EPIC data for 53 galaxy clusters. Through 2D spectral maps, we provide the most detailed and extended view of the spatial distribution of temperature (…