Validation of selection function, sample contamination and mass calibration in galaxy cluster samples

Author:

Grandis S12,Klein M13,Mohr J J123,Bocquet S12,Paulus M13,Abbott T M C4,Aguena M56,Allam S7,Annis J7,Benson B A789,Bertin E1011,Bhargava S12,Brooks D13,Burke D L1415,Carnero Rosell A16,Carrasco Kind M1718,Carretero J19,Capasso R20,Costanzi M2122,da Costa L N623,De Vicente J16,Desai S24,Dietrich J P1,Doel P13,Eifler T F2526,Evrard A E2728,Flaugher B7,Fosalba P2930,Frieman J731,García-Bellido J32,Gaztanaga E2930,Gerdes D W2728,Gruen D331415,Gruendl R A1718,Gschwend J623,Gutierrez G7,Hartley W G1334,Hinton S R35,Hollowood D L36,Honscheid K3738,James D J39,Jeltema T36,Kuehn K4041,Kuropatkin N7,Lima M67,Maia M A G723,Marshall J L42,Melchior P43,Menanteau F1718,Miquel R4419,Ogando R L C623,Palmese A78,Paz-Chinchón F1718,Plazas A A43,Romer A K12,Roodman A1415,Sanchez E16,Saro A212245,Scarpine V7,Schubnell M28,Serrano S2930,Sheldon E46,Smith M47,Stark A A39,Suchyta E48,Swanson M E C18,Tarle G28,Thomas D49,Tucker D L7,Varga T N350,Weller J350,Wilkinson R12

Affiliation:

1. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany

2. Excellence Cluster Origins, Boltzmannstr. 2, D-85748 Garching, Germany

3. Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. D-85748, Garching, Germany

4. Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile

5. Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP-05314-970, Brazil

6. Laboratório Interinstitucional de e-Astronomia – LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ – 20921-400, Brazil

7. Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510, USA

8. Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA

9. Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA

10. CNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014 Paris, France

11. UPMC Univ Paris 06, UMR 7095, Institut d’Astrophysique de Paris, Sorbonne Universités, F-75014 Paris, France

12. Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, UK

13. Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK

14. Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, CA 94305, USA

15. SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA

16. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Av. Complutense, 40, 28040 Madrid, Spain

17. Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801, USA

18. National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA

19. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain

20. Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova University Centre, SE-106 91 Stockholm, Sweden

21. INAF – Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy

22. IFPU – Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy

23. Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ – 20921-400, Brazil

24. Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India

25. Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065, USA

26. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA

27. Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA

28. Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA

29. Institut d’Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain

30. Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain

31. Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA

32. Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain

33. Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA

34. Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland

35. School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia

36. Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA

37. Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA

38. Department of Physics, The Ohio State University, Columbus, OH 43210, USA

39. Center for Astrophysics, Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA

40. Australian Astronomical Optics, Macquarie University, North Ryde, NSW 2113, Australia

41. Lowell Observatory, 1400 Mars Hill Rd, Flagstaff, AZ 86001, USA

42. 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

43. Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA

44. Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain

45. Astronomy Unit, Department of Physics, University of Trieste, via Tiepolo 11, I-34131 Trieste, Italy

46. Brookhaven National Laboratory, Bldg 510, Upton, NY 11973, USA

47. School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK

48. Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA

49. Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, PO1 3FX, UK

50. Fakultät für Physik, Ludwig-Maximilians Universität München,Universitäts-Sternwarte, Scheinerstr. 1, D-81679 München, Germany

Abstract

ABSTRACT We construct and validate the selection function of the MARD-Y3 galaxy cluster sample. This sample was selected through optical follow-up of the 2nd ROSAT faint source catalogue with Dark Energy Survey year 3 data. The selection function is modelled by combining an empirically constructed X-ray selection function with an incompleteness model for the optical follow-up. We validate the joint selection function by testing the consistency of the constraints on the X-ray flux–mass and richness–mass scaling relation parameters derived from different sources of mass information: (1) cross-calibration using South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) clusters, (2) calibration using number counts in X-ray, in optical and in both X-ray and optical while marginalizing over cosmological parameters, and (3) other published analyses. We find that the constraints on the scaling relation from the number counts and SPT-SZ cross-calibration agree, indicating that our modelling of the selection function is adequate. Furthermore, we apply a largely cosmology independent method to validate selection functions via the computation of the probability of finding each cluster in the SPT-SZ sample in the MARD-Y3 sample and vice versa. This test reveals no clear evidence for MARD-Y3 contamination, SPT-SZ incompleteness or outlier fraction. Finally, we discuss the prospects of the techniques presented here to limit systematic selection effects in future cluster cosmological studies.

Funder

Max-Planck-Gesellschaft

Deutsche Forschungsgemeinschaft

Ludwig-Maximilians-Universität München

National Science Foundation

University of Chicago

Kavli Foundation

Gordon and Betty Moore Foundation

U.S. Department of Energy

Science and Technology Facilities Council

Higher Education Funding Council for England

University of Illinois at Urbana-Champaign

Ohio State University

Financiadora de Estudos e Projetos

Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Ministério da Ciência, Tecnologia e Inovação

Ministerio de Economía y Competitividad

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 15 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The SRG/eROSITA All-Sky Survey;Astronomy & Astrophysics;2024-07

2. The SRG/eROSITA All-Sky Survey;Astronomy & Astrophysics;2024-07

3. SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region;Monthly Notices of the Royal Astronomical Society;2024-06-13

4. Determining the baryon impact on the matter power spectrum with galaxy clusters;Monthly Notices of the Royal Astronomical Society;2024-01-27

5. X-ray Cluster Cosmology;Handbook of X-ray and Gamma-ray Astrophysics;2024

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3