activity
19972021
most citedSpectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey

877 citations · 4.3k across the 87 of their papers we have counts for

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Showing 2018Show all

10 papers · 1 filter

astro-ph.GA2018★ 42 cited

The XXL Survey: XXVII. The 3XLSS point source catalogue

L. Chiappetti, S. Fotopoulou, C. Lidman +35

We present the version of the point source catalogue of the XXL Survey that was used, in part, in the first series of XXL papers. In this paper we release, in our database in Milan…

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.GA2018★ 9 cited

The XXL Survey : XXVI. Optical and near-infrared identifications of the ATCA 2.1 GHz radio sources in the XXL-S Field

Paolo Ciliegi, Nika Jurlin, Andrew Butler +7

In this paper we present the optical, near-infrared (NIR) and X-ray identifications of the 6287 radio sources detected in the 2.1 GHz deep radio survey down to a median rms of ~ 41…

astro-ph.IM2018★ 23 cited

The XXL Survey XXIV. The final detection pipeline

L. Faccioli, F. Pacaud, J. -L. Sauvageot +7

A well characterised detection pipeline is an important ingredient for X-ray cluster surveys. We present the final development of the XXL Survey pipeline. The pipeline optimally us…

astro-ph.GA2018★ 31 cited

The XXL survey XXXV. The role of cluster mass in AGN activity

E. Koulouridis, M. Ricci, P. Giles +15

We present the results of a study of the AGN density in a homogeneous and well-studied sample of 167 bona fide X-ray galaxy clusters () from the XXL Survey. The results…

astro-ph.GA2018★ 7 cited

The XXL Survey: XXXIII. Chandra Constraints on the AGN Contamination of z > 1 XXL Galaxy Clusters

C. H. A. Logan, B. J. Maughan, M. N. Bremer +11

Context. The XMM-XXL survey uses observations from XMM-Newton to detect clusters of galaxies over a wide range in mass and redshift. The moderate PSF of XMM-Newton means that point…