The XMM cluster survey: exploring scaling relations and completeness of the dark energy survey year 3 redMaPPer cluster catalogue
- Department of Physics and Astronomy, University of Sussex , Brighton BN1 9QH, UK
- 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
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University , Stanford, CA 94305, USA
- Department of Statistics and Data Sciences, The University of Texas at Austin , Austin, TX 78712, USA
- AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot , Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France
- Santa Cruz Institute for Particle Physics, University of California , Santa Cruz, 1156 High St, Santa Cruz, CA 95064, USA
- Faculty of Physics, Ludwig-Maximilians-Universität , Scheinerstr. 1, D-81679, Munich, Germany
- Astrophysics Research Institute, Liverpool John Moores University , Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK
- 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
- Institute for Astronomy, University of Edinburgh, Royal Observatory , Blackford Hill, Edinburgh EH9 3HJ, UK
- Astronomy Department, University of Michigan , Ann Arbor, MI 48109, USA
- Department of Physics and Astronomy, Uppsala University , SE-751 20 Uppsala, Sweden
- Department of Physics, Lancaster University , Lancaster LA1 4YB, UK
- Fermi National Accelerator Laboratory , P. O. Box 500, Batavia, IL 60510, USA
- Department of Physics, University of Michigan , Ann Arbor, MI 48109, USA
- Institute of Cosmology and Gravitation, University of Portsmouth , Portsmouth, PO1 3FX, UK
- Sorbonne Universités , UPMC Univ Paris 06, UMR 7095, Institut d’Astrophysique de Paris, F-75014, Paris, France
- University Observatory, Faculty of Physics, Ludwig-Maximilians-Universität , Scheinerstr. 1, D-81679 Munich, Germany
- Department of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT, UK
- 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
- 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
- Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, E-08193 Bellaterra, Barcelona, Spain
- 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
- Laboratório Interinstitucional de e-Astronomia – LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
- Hamburger Sternwarte, Universität Hamburg , Gojenbergsweg 112, D-21029 Hamburg, Germany
- Centro de Investigaciones Energéticas , Medioambientales y Tecnológicas (CIEMAT), Madrid 28040, Spain
- Department of Physics, IIT Hyderabad , Kandi, Telangana 502285, India
- Jet Propulsion Laboratory, California Institute of Technology , 4800 Oak Grove Dr, Pasadena, CA 91109, USA
- Institute of Theoretical Astrophysics , University of Oslo. P.O. Box 1029 Blindern, NO-0315 Oslo, Norway
- Fermi National Accelerator Laboratory , P. O. Box 500, Batavia, IL 60510, USA;Kavli Institute for Cosmological Physics, University of Chicago , Chicago, IL 60637, USA
- Instituto de Fisica Teorica UAM/CSIC , Universidad Autonoma de Madrid, E-28049 Madrid, Spain
- Department of Astronomy, University of Michigan , Ann Arbor, MI 48109, USA
- School of Mathematics and Physics, University of Queensland , Brisbane, QLD 4072, Australia
- 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
- Center for Astrophysics | Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USA
- Australian Astronomical Optics, Macquarie University , North Ryde, NSW 2113, Australia;Lowell Observatory , 1400 Mars Hill Rd, Flagstaff, AZ 86001, USA
- 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
- 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
- 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
- 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
- Observatório Nacional , Rua Gal. José Cristino 77, Rio de Janeiro, RJ - 20921-400, Brazil
- 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
- Department of Physics, University of Genova and INFN , Via Dodecaneso 33, I-16146, Genova, Italy
- School of Physics and Astronomy, University of Southampton , Southampton, SO17 1BJ, UK
- Computer Science and Mathematics Division , Oak Ridge National Laboratory, Oak Ridge, TN 37831, United States
- Center for Cosmology and Astro-Particle Physics, The Ohio State University , Columbus, OH 43210, USA
- Department of Physics, University of Michigan , Ann Arbor, MI 48109, USA;Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA
- 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
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