SPIDERS: an overview of the largest catalogue of spectroscopically confirmed x-ray galaxy clusters

Author:

Kirkpatrick C C12ORCID,Clerc N3ORCID,Finoguenov A1ORCID,Damsted S1,Ider Chitham J4ORCID,Kukkola A E1,Gueguen A4,Furnell K5,Rykoff E67,Comparat J4,Saro A8910ORCID,Capasso R11ORCID,Padilla N12,Erfanianfar G4,Mamon G A13ORCID,Collins C5,Merloni A4,Brownstein J R14ORCID,Schneider D P1516

Affiliation:

1. Department of Physics, University of Helsinki, Gustaf Hällströmin katu 2, FI-00014 Helsinki, Finland

2. Helsinki Institute of Physics, Gustaf Hällströmin katu 2, FI-00014 Helsinki, Finland

3. IRAP, Université de Toulouse, CNRS, UPS, CNES, F-31028, Toulouse, France

4. Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, D-85748 Garching, Germany

5. Astrophyics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK

6. Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450, Stanford University, Stanford, CA 94305, USA

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

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

9. IFPU - Institute for Fundamental Physics of the Universe, via Beirut 2, I-34014 Trieste, Italy

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

11. The Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden

12. Instituto de Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuna Mackenna 4860, 782-0436 Macul, Santiago, Chile

13. Institut d’Astrophysique de Paris, (UMR 7095: CNRS & UPMC, Sorbonne Université), F-75014 Paris, France

14. Department of Physics and Astronomy, University of Utah, 115 S 1400 E, Salt Lake City, UT 84112, USA

15. Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA

16. Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA

Abstract

ABSTRACT SPIDERS is the spectroscopic follow-up effort of the Sloan Digital Sky Survey IV (SDSS-IV) project for the identification of X-ray selected galaxy clusters. We present our catalogue of 2740 visually inspected galaxy clusters as part of the SDSS Data Release 16 (DR16). Here we detail the target selection, our methods for validation of the candidate clusters, performance of the survey, the construction of the final sample, and a full description of what is found in the catalogue. Of the sample, the median number of members per cluster is approximately 10, with 818 having 15 or greater. We find that we are capable of validating over 99 per cent of clusters when five redshifts are obtained below z < 0.3 and when nine redshifts are obtained above z > 0.3. We discuss the improvements in this catalogue’s identification of cluster using 33 340 redshifts, with Δzphot/Δzspec ∼ 100, over other photometric and spectroscopic surveys, as well as presenting an update to previous (σ–LX) and (σ–λ) relations. Finally, we present our cosmological constraints derived using the velocity dispersion function.

Funder

Academy of Finland

European Research Council

Carnegie Mellon University

Johns Hopkins University

University of Tokyo

New Mexico State University

New York University

University of Notre Dame

Ohio State University

Pennsylvania State University

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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