The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1,Monthly Notices of the Royal Astronomical Society

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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
Monthly Notices of the Royal Astronomical Society ( IF 4.7 ) Pub Date : 2020-12-17 , DOI: 10.1093/mnras/staa3891
Arnaud de Mattia ₁ , Vanina Ruhlmann-Kleider ₁ , Anand Raichoor ₂ , Ashley J Ross ₃ , Amélie Tamone ₂ , Cheng Zhao ₂ , Shadab Alam ₄ , Santiago Avila _{5,

6} , Etienne Burtin ₁ , Julian Bautista ₇ , Florian Beutler ₈ , Jonathan Brinkmann ₉ , Joel R Brownstein ₁₀ , Michael J Chapman _{11,

12} , Chia-Hsun Chuang ₁₃ , Johan Comparat ₁₄ , Hélion du Mas des Bourboux ₁₀ , Kyle S Dawson ₁₀ , Axel de la Macorra ₁₅ , Héctor Gil-Marín _{16,

17} , Violeta Gonzalez-Perez ₁₈ , Claudio Gorgoni ₂ , Jiamin Hou ₁₄ , Hui Kong ₃ , Sicheng Lin ₁₉ , Seshadri Nadathur ₇ , Jeffrey A Newman ₂₀ , Eva-Maria Mueller ₂₁ , Will J Percival _{11,

12,

22} , Mehdi Rezaie ₂₃ , Graziano Rossi ₂₄ , Donald P Schneider ₂₅ , Prabhakar Tiwari ₂₆ , M Vivek ₂₇ , Yuting Wang ₂₆ , Gong-Bo Zhao _{26,

28}

Affiliation

IRFU, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
Institute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, Ohio, USA
Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, EH9 3HJ, UK
Departamento de Física Teórica M8, Universidad Autónoma de Madrid, E-28049 Cantoblanco, Madrid, Spain
Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
Institute of Cosmology, and Gravitation, Dennis Sciama Building, University of Portsmouth, Portsmouth, PO1 3FX, UK
Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349, USA
Department Physics and Astronomy, University of Utah, 115 S 1400 E, Salt Lake City, UT 84112, USA
Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON N2L 3G1, Canada
Department of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, Canada
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA
Max-Planck-Institut für Extraterrestrische Physik, Postfach 1312, Giessenbachstr., 85748 Garching bei München, Germany
Instituto de Física, Universidad Nacional Autónoma de México, Apdo. Postal 20-364, Mexico
Institut de Ciències del Cosmos, Universitat de Barcelona, ICCUB, Martí i Franquès 1, E08028 Barcelona, Spain
Institut d’Estudis Espacials de Catalunya (IEEC), E08034 Barcelona, Spain
Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK
Center for Cosmology and Particle Physics, Department of Physics, New York University, 726 Broadway, New York, NY 10003, USA
PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA
Sub-department of Astrophysics, Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK
Perimeter Institute for Theoretical Physics, 31 Caroline St. North, Waterloo, ON N2L 2Y5, Canada
Department of Physics and Astronomy, Ohio University, 251B Clippinger Labs, Athens, OH 45701, USA
Department of Physics and Astronomy, Sejong University, Seoul 143-747, Korea
Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA
National Astronomy Observatories, Chinese Academy of Science, Beijing, 100101, P.R. China
Indian Institute of Astrophysics, Koramangala, Bangalore 560034, India
School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, P.R. China

We present the large-scale clustering of emission line galaxies (ELG) from the Data Release 16 of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey. The ELG sample contains 173,736 galaxies covering 1,170 square degrees in the redshift range $0.6

中文翻译：

已完成的 SDSS-IV 扩展重子振荡光谱调查：从红移 0.6 和 1.1 之间的各向异性功率谱测量 BAO 和发射线星系样本的结构生长速率

我们展示了来自斯隆数字巡天 IV 扩展重子振荡光谱调查的数据发布 16 的大规模发射线星系 (ELG) 聚类。ELG 样本包含 173,736 个星系，覆盖 1,170 平方度的红移范围 $0.6

更新日期：2020-12-17

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