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Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters

Research output: Working paperPreprint

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  • P. Kelly
  • J. Jobel
  • O. Eiger
  • A. Abd
  • T. E. Jeltema
  • P. Giles
  • D. L. Hollowood
  • R. D. Wilkinson
  • D. J. Turner
  • S. Bhargava
  • S. Everett
  • A. Farahi
  • A. K. Romer
  • E. S. Rykoff
  • F. Wang
  • S. Bocquet
  • D. Cross
  • R. Faridjoo
  • J. Franco
  • G. Gardner
  • M. Kwiecien
  • D. Laubner
  • A. McDaniel
  • J. H. O'Donnell
  • L. Sanchez
  • E. Schmidt
  • S. Sripada
  • A. Swart
  • E. Upsdell
  • A. Webber
  • M. Aguena
  • S. Allam
  • O. Alves
  • D. Bacon
  • D. Brooks
  • D. L. Burke
  • A. Carnero Rosell
  • J. Carretero
  • C. A. Collins
  • M. Costanzi
  • L. N. da Costa
  • M. E. S. Pereira
  • T. M. Davis
  • P. Doel
  • I. Ferrero
  • J. Frieman
  • J. García-Bellido
  • G. Giannini
  • D. Gruen
  • R. A. Gruendl
  • M. Hilton
  • S. R. Hinton
  • K. Honscheid
  • D. J. James
  • K. Kuehn
  • R. G. Mann
  • J. L. Marshall
  • J. Mena-Fernández
  • C. J. Miller
  • R. Miquel
  • J. Myles
  • A. Palmese
  • A. Pieres
  • A. A. Plazas Malagón
  • P. J. Rooney
  • M. Sahlen
  • E. Sanchez
  • D. Sanchez Cid
  • M. Schubnell
  • I. Sevilla-Noarbe
  • M. Smith
  • E. Suchyta
  • M. E. C. Swanson
  • G. Tarle
  • C. To
  • P. T. P. Viana
  • N. Weaverdyck
  • P. Wiseman
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Publication date24/07/2024
PublisherArxiv
<mark>Original language</mark>English

Abstract

We use Dark Energy Survey Year 3 (DES Y3) clusters with archival X-ray data from XMM-Newton and Chandra to assess the centering performance of the redMaPPer cluster finder and to measure key richness observable scaling relations. In terms of centering, we find that 10-20% of redMaPPer clusters are miscentered with no significant difference in bins of low versus high richness ($2040$) or redshift ($0.2