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The XMM Cluster Survey: Exploring scaling relations and completeness of the Dark Energy Survey Year 3 redMaPPer cluster catalogue

Authors :
E W Upsdell
P A Giles
A K Romer
R Wilkinson
D J Turner
M Hilton
E Rykoff
A Farahi
S Bhargava
T Jeltema
M Klein
A Bermeo
C A Collins
L Ebrahimpour
D Hollowood
R G Mann
M Manolopoulou
C J Miller
P J Rooney
Martin Sahlén
J P Stott
P T P Viana
S Allam
O Alves
D Bacon
E Bertin
S Bocquet
D Brooks
D L Burke
M Carrasco Kind
J Carretero
M Costanzi
L N da Costa
M E S Pereira
J De Vicente
S Desai
H T Diehl
J P Dietrich
S Everett
I Ferrero
J Frieman
J García-Bellido
D W Gerdes
G Gutierrez
S R Hinton
K Honscheid
D J James
K Kuehn
N Kuropatkin
M Lima
J L Marshall
J Mena-Fernández
F Menanteau
R Miquel
J J Mohr
R L C Ogando
A Pieres
M Raveri
M Rodriguez-Monroy
E Sanchez
V Scarpine
I Sevilla-Noarbe
M Smith
E Suchyta
M E C Swanson
G Tarle
C To
N Weaverdyck
J Weller
P Wiseman
Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Institut d'Astrophysique de Paris (IAP)
Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
XMM
Source :
Mon.Not.Roy.Astron.Soc., Mon.Not.Roy.Astron.Soc., 2023, 522 (4), pp.5267-5290. ⟨10.1093/mnras/stad1220⟩
Publication Year :
2023
Publisher :
arXiv, 2023.

Abstract

We cross-match and compare characteristics of galaxy clusters identified in observations from two sky surveys using two completely different techniques. One sample is optically selected from the analysis of three years of Dark Energy Survey observations using the redMaPPer cluster detection algorithm. The second is X-ray selected from XMM observations analysed by the XMM Cluster Survey. The samples comprise a total area of 57.4 deg$^2$, bounded by the area of 4 contiguous XMM survey regions that overlap the DES footprint. We find that the X-ray selected sample is fully matched with entries in the redMaPPer catalogue, above $\lambda>$20 and within 0.1$< z<br />Comment: Accepted for publication to MNRAS

Details

Database :
OpenAIRE
Journal :
Mon.Not.Roy.Astron.Soc., Mon.Not.Roy.Astron.Soc., 2023, 522 (4), pp.5267-5290. ⟨10.1093/mnras/stad1220⟩
Accession number :
edsair.doi.dedup.....a0f0b4c1280bf034dd563700c37aa1d1
Full Text :
https://doi.org/10.48550/arxiv.2304.13570