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The XXL Survey-I. Scientific motivations− XMM-Newton observing plan− Follow-up observations and simulation programme
Context. The quest for the cosmological parameters that describe our universe continues to
motivate the scientific community to undertake very large survey initiatives across the …
motivate the scientific community to undertake very large survey initiatives across the …
Cosmological constraints from galaxy clusters and groups in the eROSITA final equatorial depth survey
We present the first cosmological study of a sample of eROSITA clusters, which were
identified in the eROSITA Final Equatorial Depth Survey (eFEDS). In a joint selection on X …
identified in the eROSITA Final Equatorial Depth Survey (eFEDS). In a joint selection on X …
SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release
N Clerc, CC Kirkpatrick, A Finoguenov… - Monthly Notices of …, 2020 - academic.oup.com
ABSTRACT SPIDERS (The SPectroscopic IDentification of eROSITA Sources) is a large
spectroscopic programme for X-ray selected galaxy clusters as part of the Sloan Digital Sky …
spectroscopic programme for X-ray selected galaxy clusters as part of the Sloan Digital Sky …
SPIDERS: an overview of the largest catalogue of spectroscopically confirmed x-ray galaxy clusters
CC Kirkpatrick, N Clerc, A Finoguenov… - Monthly Notices of …, 2021 - academic.oup.com
ABSTRACT SPIDERS is the spectroscopic follow-up effort of the Sloan Digital Sky Survey IV
(SDSS-IV) project for the identification of X-ray selected galaxy clusters. We present our …
(SDSS-IV) project for the identification of X-ray selected galaxy clusters. We present our …
The XXL Survey-II. The bright cluster sample: catalogue and luminosity function
F Pacaud, N Clerc, PA Giles, C Adami… - Astronomy & …, 2016 - aanda.org
Context. The XXL Survey is the largest survey carried out by the XMM-Newton satellite and
covers a total area of 50 square degrees distributed over two fields. It primarily aims at …
covers a total area of 50 square degrees distributed over two fields. It primarily aims at …
Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
R Seppi, J Comparat, E Bulbul, K Nandra… - Astronomy & …, 2022 - aanda.org
Context. The extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on
board the Spectrum-Roentgen-Gamma (SRG) observatory is revolutionizing X-ray …
board the Spectrum-Roentgen-Gamma (SRG) observatory is revolutionizing X-ray …
X-ray scaling relations for a representative sample of Planck-selected clusters observed with XMM-Newton
We report the scaling relations derived by fitting the X-ray parameters determined from
analyzing the XMM-Newton observations of 120 galaxy clusters in the Planck Early Sunyaev …
analyzing the XMM-Newton observations of 120 galaxy clusters in the Planck Early Sunyaev …
The XMM-SERVS survey: new XMM–Newton point-source catalogue for the XMM-LSS field
We present an X-ray point-source catalogue from the XMM-Large Scale Structure (XMM-
LSS) survey region, one of the XMM-Spitzer Extragalactic Representative Volume Survey …
LSS) survey region, one of the XMM-Spitzer Extragalactic Representative Volume Survey …
HSC-XXL: Baryon budget of the 136 XXL groups and clusters
D Akino, D Eckert, N Okabe, M Sereno… - Publications of the …, 2022 - academic.oup.com
We present our determination of the baryon budget for an X-ray-selected XXL sample of 136
galaxy groups and clusters spanning nearly two orders of magnitude in mass (M 500∼ 1013 …
galaxy groups and clusters spanning nearly two orders of magnitude in mass (M 500∼ 1013 …
The XXL Survey-XIII. Baryon content of the bright cluster sample
Traditionally, galaxy clusters have been expected to retain all the material accreted since
their formation epoch. For this reason, their matter content should be representative of the …
their formation epoch. For this reason, their matter content should be representative of the …