The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release

Author:

Zhao Cheng1ORCID,Chuang Chia-Hsun2ORCID,Bautista Julian3ORCID,de Mattia Arnaud4,Raichoor Anand1,Ross Ashley J5ORCID,Hou Jiamin6,Neveux Richard4,Tao Charling7,Burtin Etienne4,Dawson Kyle S8,de la Torre Sylvain9,Gil-Marín Héctor1011ORCID,Kneib Jean-Paul19,Percival Will J121314,Rossi Graziano15,Tamone Amélie1,Tinker Jeremy L16ORCID,Zhao Gong-Bo1718,Alam Shadab19,Mueller Eva-Maria20

Affiliation:

1. Institute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland

2. Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA

3. Institute of Cosmology & Gravitation, Dennis Sciama Building, University of Portsmouth, Portsmouth PO1 3FX, UK

4. IRFU,CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France

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

6. Max-Planck-Institut für Extraterrestrische Physik, Postfach 1312, Giessenbachstr., 85748 Garching bei München, Germany

7. CPPM, Aix-Marseille Université, CNRS/IN2P3, CPPM UMR 7346, F13288 Marseille, France

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

9. Aix Marseille Univ, CNRS, CNES, LAM, F13388 Ma rseille, France

10. Institut de Ciències del Cosmos, Universitat de Barcelona, ICCUB, Martí i Franquès 1, E08028 Barcelona, Spain

11. Institut d’Estudis Espacials de Catalunya (IEEC), E08034 Barcelona, Spain

12. Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1, Canada

13. Department of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, Canada

14. Perimeter Institute for Theoretical Physics, 31 Caroline St. North, Waterloo, ON N2L 2Y5, Canada

15. Department of Physics and Astronomy, Sejong University, Seoul 143-747, Korea

16. Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, NY 10003, USA

17. National Astronomy Observatories, Chinese Academy of Science, Beijing 100101, P.R. China

18. School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, P.R.China

19. Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UK

20. Department of Astrophysics, Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK

Abstract

ABSTRACT We produce 1000 realizations of synthetic clustering catalogues for each type of the tracers used for the baryon acoustic oscillation and redshift space distortion analysis of the Sloan Digital Sky Surveys-iv extended Baryon Oscillation Spectroscopic Survey final data release (eBOSS DR16), covering the redshift range from 0.6 to 2.2, to provide reliable estimates of covariance matrices and test the robustness of the analysis pipeline with respect to observational systematics. By extending the Zel’dovich approximation density field with an effective tracer bias model calibrated with the clustering measurements from the observational data, we accurately reproduce the two- and three-point clustering statistics of the eBOSS DR16 tracers, including their cross-correlations in redshift space with very low computational costs. In addition, we include the gravitational evolution of structures and sample selection biases at different redshifts, as well as various photometric and spectroscopic systematic effects. The agreements on the auto-clustering statistics between the data and mocks are generally within $1\, \sigma$ variances inferred from the mocks, for scales down to a few $h^{-1}\, {\rm Mpc}$ in configuration space, and up to $0.3\, h\, {\rm Mpc}^{-1}$ in Fourier space. For the cross correlations between different tracers, the same level of consistency presents in configuration space, while there are only discrepancies in Fourier space for scales above $0.15\, h\, {\rm Mpc}^{-1}$. The accurate reproduction of the data clustering statistics permits reliable covariances for multi-tracer analysis.

Funder

Statens Naturvidenskabelige Forskningsrad

H2020 European Research Council

Agence Nationale de la Recherche

National Research Foundation of Korea

Ministry of Education, Science and Technology

Sejong University

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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