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Title: The XMM cluster survey: exploring scaling relations and completeness of the dark energy survey year 3 redMaPPer cluster catalogue

Journal Article · · Monthly Notices of the Royal Astronomical Society
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  1. Department of Physics and Astronomy, University of Sussex , Brighton BN1 9QH, UK
  2. Astrophysics Research Centre, University of KwaZulu-Natal , Westville Campus, Durban 4041, SA;School of Mathematics, Statistics, and Computer Science, University of KwaZulu-Natal , Westville Campus, Durban 4041, SA
  3. Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University , Stanford, CA 94305, USA
  4. Department of Statistics and Data Sciences, The University of Texas at Austin , Austin, TX 78712, USA
  5. AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot , Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France
  6. Santa Cruz Institute for Particle Physics, University of California , Santa Cruz, 1156 High St, Santa Cruz, CA 95064, USA
  7. Faculty of Physics, Ludwig-Maximilians-Universität , Scheinerstr. 1, D-81679, Munich, Germany
  8. Astrophysics Research Institute, Liverpool John Moores University , Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK
  9. Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP , Rua das Estrelas, P-4150-762 Porto, Portugal;Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto , Rua do Campo Alegre, 687, P-4169-007 Porto, Portugal
  10. Institute for Astronomy, University of Edinburgh, Royal Observatory , Blackford Hill, Edinburgh EH9 3HJ, UK
  11. Astronomy Department, University of Michigan , Ann Arbor, MI 48109, USA
  12. Department of Physics and Astronomy, Uppsala University , SE-751 20 Uppsala, Sweden
  13. Department of Physics, Lancaster University , Lancaster LA1 4YB, UK
  14. Fermi National Accelerator Laboratory , P. O. Box 500, Batavia, IL 60510, USA
  15. Department of Physics, University of Michigan , Ann Arbor, MI 48109, USA
  16. Institute of Cosmology and Gravitation, University of Portsmouth , Portsmouth, PO1 3FX, UK
  17. Sorbonne Universités , UPMC Univ Paris 06, UMR 7095, Institut d’Astrophysique de Paris, F-75014, Paris, France
  18. University Observatory, Faculty of Physics, Ludwig-Maximilians-Universität , Scheinerstr. 1, D-81679 Munich, Germany
  19. Department of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT, UK
  20. Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University , Stanford, CA 94305, USA;SLAC National Accelerator Laboratory , Menlo Park, CA 94025, USA
  21. Center for Astrophysical Surveys, National Center for Supercomputing Applications , 1205 West Clark St., Urbana, IL 61801, USA;Department of Astronomy, University of Illinois at Urbana-Champaign , 1002 W. Green Street, Urbana, IL 61801, USA
  22. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, E-08193 Bellaterra, Barcelona, Spain
  23. Astronomy Unit, Department of Physics, University of Trieste , via Tiepolo 11, I-34131 Trieste, Italy;INAF – Osservatorio Astronomico di Trieste , via G. B. Tiepolo 11, I-34143 Trieste, Italy;Institute for Fundamental Physics of the Universe , Via Beirut 2, I-34014 Trieste, Italy
  24. Laboratório Interinstitucional de e-Astronomia – LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
  25. Hamburger Sternwarte, Universität Hamburg , Gojenbergsweg 112, D-21029 Hamburg, Germany
  26. Centro de Investigaciones Energéticas , Medioambientales y Tecnológicas (CIEMAT), Madrid 28040, Spain
  27. Department of Physics, IIT Hyderabad , Kandi, Telangana 502285, India
  28. Jet Propulsion Laboratory, California Institute of Technology , 4800 Oak Grove Dr, Pasadena, CA 91109, USA
  29. Institute of Theoretical Astrophysics , University of Oslo. P.O. Box 1029 Blindern, NO-0315 Oslo, Norway
  30. Fermi National Accelerator Laboratory , P. O. Box 500, Batavia, IL 60510, USA;Kavli Institute for Cosmological Physics, University of Chicago , Chicago, IL 60637, USA
  31. Instituto de Fisica Teorica UAM/CSIC , Universidad Autonoma de Madrid, E-28049 Madrid, Spain
  32. Department of Astronomy, University of Michigan , Ann Arbor, MI 48109, USA
  33. School of Mathematics and Physics, University of Queensland , Brisbane, QLD 4072, Australia
  34. Center for Cosmology and Astro-Particle Physics, The Ohio State University , Columbus, OH 43210, USA;Department of Physics, The Ohio State University , Columbus, OH 43210, USA
  35. Center for Astrophysics | Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USA
  36. Australian Astronomical Optics, Macquarie University , North Ryde, NSW 2113, Australia;Lowell Observatory , 1400 Mars Hill Rd, Flagstaff, AZ 86001, USA
  37. Laboratório Interinstitucional de e-Astronomia – LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil;Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo , CP 66318, São Paulo, SP, 05314-970, Brazil
  38. George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University , College Station, TX 77843, USA
  39. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, E-08193 Bellaterra, Barcelona, Spain;Institució Catalana de Recerca i Estudis Avançats , E-08010 Barcelona, Spain
  40. University Observatory, Faculty of Physics, Ludwig-Maximilians-Universität , Scheinerstr. 1, D-81679 Munich, Germany;Max Planck Institute for Extraterrestrial Physics , Giessenbachstrasse, D-85748 Garching, Germany
  41. Observatório Nacional , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
  42. Laboratório Interinstitucional de e-Astronomia – LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil;Observatório Nacional , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
  43. Department of Physics, University of Genova and INFN , Via Dodecaneso 33, I-16146, Genova, Italy
  44. School of Physics and Astronomy, University of Southampton , Southampton, SO17 1BJ, UK
  45. Computer Science and Mathematics Division , Oak Ridge National Laboratory, Oak Ridge, TN 37831, United States
  46. Center for Cosmology and Astro-Particle Physics, The Ohio State University , Columbus, OH 43210, USA
  47. Department of Physics, University of Michigan , Ann Arbor, MI 48109, USA;Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA
  48. Max Planck Institute for Extraterrestrial Physics , Giessenbachstrasse, D-85748 Garching, Germany;Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München , Scheinerstr. 1, D-81679 München, Germany

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 3 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 deg2, bounded by the area of four contiguous XMM survey regions that overlap the DES footprint. Here we find that the X-ray-selected sample is fully matched with entries in the redMaPPer catalogue, above λ > 20 and within 0.1 <$$z$$ <0.9. Conversely, only 38 per cent of the redMaPPer catalogue is matched to an X-ray extended source. Next, using 120 optically clusters and 184 X-ray-selected clusters, we investigate the form of the X-ray luminosity–temperature (LX –TX ), luminosity–richness (LX –λ), and temperature–richness (TX –λ) scaling relations. We find that the fitted forms of the LX –TX relations are consistent between the two selection methods and also with other studies in the literature. However, we find tentative evidence for a steepening of the slope of the relation for low richness systems in the X-ray-selected sample. When considering the scaling of richness with X-ray properties, we again find consistency in the relations (i.e. LX –λ and TX –λ) between the optical and X-ray-selected samples. This is contrary to previous similar works that find a significant increase in the scatter of the luminosity scaling relation for X-ray-selected samples compared to optically selected samples.

Research Organization:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Argonne National Laboratory (ANL), Argonne, IL (United States)
Sponsoring Organization:
USDOE; USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
DES Collaboration
Grant/Contract Number:
AC05-00OR22725; AC02-07CH11359; AC02-05CH11231
OSTI ID:
1973876
Alternate ID(s):
OSTI ID: 1973460; OSTI ID: 1999035; OSTI ID: 2305493
Report Number(s):
DES-2022-0741; FERMILAB-PUB-23-020-PPD; arXiv:2304.13570; TRN: US2405426
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 522, Issue 4; ISSN 0035-8711
Publisher:
Oxford University PressCopyright Statement
Country of Publication:
United States
Language:
English

References (55)

CONSTRAINTS ON COSMOLOGY FROM THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM OF THE 2500 deg 2 SPT-SZ SURVEY journal January 2014
Collisional Plasma Models with APEC/APED: Emission-Line Diagnostics of Hydrogen-like and Helium-like Ions journal August 2001
A Wavelet‐Based Algorithm for the Spatial Analysis of Poisson Data journal January 2002
Dark Energy Surveyed Year 1 results: calibration of cluster mis-centring in the redMaPPer catalogues journal May 2019
Towards a realistic population of simulated galaxy groups and clusters journal May 2014
Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing journal August 2018
The eROSITA Final Equatorial-Depth Survey (eFEDS) journal May 2022
The eROSITA X-ray telescope on SRG journal February 2021
Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology journal May 2021
HI4PI: a full-sky H i survey based on EBHIS and GASS journal October 2016
The X-ray luminosity–temperature relation of a complete sample of low-mass galaxy clusters journal August 2016
The dark Energy Camera journal October 2015
The eROSITA Final Equatorial-Depth Survey (eFEDS) journal May 2022
Cluster Cosmology Constraints from the 2500 deg 2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope journal June 2019
Scaling Properties of Galaxy Groups journal May 2021
Galaxy cluster X-ray luminosity scaling relations from a representative local sample (REXCESS) journal March 2009
Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release: GAMA journal March 2011
Planck 2015 results : XXIV. Cosmology from Sunyaev-Zeldovich cluster counts journal September 2016
The XXL Survey: I. Scientific motivations − journal June 2016
Exploring the contamination of the DES-Y1 cluster sample with SPT-SZ selected clusters journal March 2021
Weighing the Giants – III. Methods and measurements of accurate galaxy cluster weak-lensing masses journal February 2014
Formation of Galaxy Clusters journal September 2012
The scatter and evolution of the global hot gas properties of simulated galaxy cluster populations journal December 2016
CHANDRA CLUSTER COSMOLOGY PROJECT III: COSMOLOGICAL PARAMETER CONSTRAINTS journal February 2009
Dark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing journal July 2020
The XXL Survey: XIII. Baryon content of the bright cluster sample⋆⋆⋆ journal June 2016
Localized massive halo properties in bahamas and MACSIS simulations: scalings, lognormality, and covariance journal May 2018
Scaling properties of a complete X-ray selected galaxy group sample journal January 2015
Stellar property statistics of massive haloes from cosmological hydrodynamics simulations: common kernel shapes journal April 2020
The Dark Energy Survey: more than dark energy – an overview journal March 2016
X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton journal April 2020
The amazing diversity in the hot gas content of an X-ray unbiased massive galaxy clusters sample journal January 2016
The XXL Survey. XLII. The LX − σv relation of galaxy groups and clusters detected in the XXL and GAMA surveys journal February 2022
Evolution and clustering of rich clusters journal September 1986
The eROSITA Final Equatorial-Depth Survey (eFEDS) journal January 2023
The environmental dependence of X-ray AGN activity at z ∼ 0.4 journal September 2020
Baryon acoustic oscillations from the SDSS DR10 galaxies angular correlation function journal January 2016
The Redmapper Galaxy Cluster Catalog from des Science Verification data journal May 2016
The eROSITA Final Equatorial Depth Survey (eFEDS) journal May 2022
A cluster finding algorithm based on the multiband identification of red sequence galaxies journal August 2014
Dark Energy Survey Year 1 results: weak lensing mass calibration of redMaPPer galaxy clusters journal October 2018
The XMM Cluster Survey analysis of the SDSS DR8 redMaPPer catalogue: implications for scatter, selection bias, and isotropy in cluster scaling relations journal August 2022
Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G3Cv1): GAMA: the GAMA galaxy group catalogue (G3Cv1) journal July 2011
A Serendipitous Galaxy Cluster Survey with XMM : Expected Catalog Properties and Scientific Applications journal February 2001
Testing the low-mass end of X-ray scaling relations with a sample of Chandra galaxy groups journal November 2011
CFHTLenS: weak lensing calibrated scaling relations for low-mass clusters of galaxies journal June 2015
The XMM Cluster Survey: X-ray analysis methodology: XCS: x-ray analysis methodology journal October 2011
Mass variance from archival X-ray properties of Dark Energy Survey Year-1 galaxy clusters journal September 2019
The Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Definition and Goals* journal July 2012
The structural and scaling properties of nearby galaxy clusters: II. The journal September 2005
Optical selection bias and projection effects in stacked galaxy cluster weak lensing journal July 2022
On the Absorption of X‐Rays in the Interstellar Medium journal October 2000
A multicomponent matched filter cluster confirmation tool for eROSITA: initial application to the RASS and DES-SV data sets journal November 2017
The eROSITA Final Equatorial-Depth Survey (eFEDS) journal May 2022
CHANDRA STUDIES OF THE X-RAY GAS PROPERTIES OF GALAXY GROUPS journal March 2009