@article{7ee792bc03c04e80b07b359d1e6a70c1,
title = "The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale structure catalogues and measurement of the isotropic BAO between redshift 0.6 and 1.1 for the Emission Line Galaxy Sample",
abstract = "We present the Emission Line Galaxy (ELG) sample of the extended Baryon Oscillation Spectroscopic Survey from the Sloan Digital Sky Survey IV Data Release 16. We describe the observations and redshift measurement for the 269 243 observed ELG spectra, and then present the large-scale structure catalogues, used for the cosmological analysis, and made of 173 736 reliable spectroscopic redshifts between 0.6 and 1.1. We perform a spherically averaged baryon acoustic oscillations (BAO) measurement in configuration space, with density field reconstruction: The data two-point correlation function shows a feature consistent with that of the BAO, the BAO model being only weakly preferred over a model without BAO (Δx2 < 1). Fitting a model constrained to have a BAO feature provides a 3.2 per cent measurement of the spherically averaged BAO distance DV(zeff)/rdrag = 18.23 ± 0.58 at the effective redshift zeff = 0.845.",
author = "Anand Raichoor and {De Mattia}, Arnaud and Ross, {Ashley J.} and Cheng Zhao and Shadab Alam and Santiago Avila and Julian Bautista and Jonathan Brinkmann and Brownstein, {Joel R.} and Etienne Burtin and Chapman, {Michael J.} and Chuang, {Chia Hsun} and Johan Comparat and Dawson, {Kyle S.} and Arjun Dey and {Du Mas des Bourboux}, Helion and Jack Elvin-Poole and Violeta Gonzalez-Perez and Claudio Gorgoni and Kneib, {Jean Paul} and Hui Kong and Dustin Lang and John Moustakas and Myers, {Adam D.} and Muller, {Eva Maria} and Seshadri Nadathur and Newman, {Jeffrey A.} and Percival, {Will J.} and Mehdi Rezaie and Graziano Rossi and Vanina Ruhlmann-Kleider and Schlegel, {David J.} and Schneider, {Donald P.} and Seo, {Hee Jong} and Amelie Tamone and Tinker, {Jeremy L.} and Rita Tojeiro and M. Vivek and Christophe Yeche and Zhao, {Gong Bo}",
note = "Funding Information: AR and JPK acknowledge support from the ERC advanced grant LIDA. AR, CZ, and AT acknowledge support from the SNF grant 200020 175751. AdM acknowledges support from the P2IO LabEx (ANR-10-LABX-0038) in the framework {\textquoteleft}Investissements d{\textquoteright}Avenir{\textquoteright} (ANR-11-IDEX-0003-01) managed by the Agence Nationale de la Recherche (ANR, France). AJR is grateful for support from the Ohio State University Center for Cosmology and Particle Physics. Authors acknowledge support from the ANR eBOSS project (ANR-16-CE31-0021) of the French National Research Agency. S. Alam is supported by the European Research Council through the COSFORM Research grant (#670193). S. Avila was supported by the MICUES project funded by the European Union{\textquoteright}s Horizon 2020 research programme under the Marie Sklodowska-Curie Grant Agreement No. 713366 (InterTalentum UAM). ADM was supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics, under Award number DE-SC0019022. VGP acknowledges support from the European Union{\textquoteright}s Horizon 2020 research and innovation programme (ERC grant #769130). JM gratefully acknowledges support from the U.S. Department of Energy, Office of Science, Office of High Energy Physics under award number DE-SC002008 and from the National Science Foundation under grant AST-1616414. EMM acknowledges support from the European Research Council (ERC) under the European Union{\textquoteright}s Horizon 2020 research and innovation programme (grant agreement no. 693024). GR acknowledges support from the National Research Foundation of Korea (NRF) through grants no. 2017R1E1A1A01077508 and no. 2020R1A2C1005655 funded by the Korean Ministry of Education, Science and Technology (MoEST), and from the faculty research fund of Sejong University. Funding Information: Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS website is www.sdss.org. Funding Information: DECaLS used data obtained with the Dark Energy Camera (DECam), which was constructed by the Dark Energy Survey (DES) collaboration. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago,Center for Cosmology and Astroparticle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundac¸{\~a}o Carlos Chagas Filho de Amparo, Fi-nanciadora de Estudos e Projetos, Fundac¸{\~a}o Carlos Chagas Filho de Amparo {\`a} Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cient{\'i}fico e Tecnol{\'o}gico and the Minist{\'e}rio da Ci{\^e}ncia, Tecnologia e Inovac{\~a}o, the Deutsche Forschungsgemein-schaft, and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones En{\'e}rgeticas, Medioambientales y Tec-nol{\'o}gicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgen{\"o}ssische Technische Hochschule (ETH) Z{\"u}rich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ci{\`e}ncies de l{\textquoteright}Espai (IEEC/CSIC), the Funding Information: This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under contract no. DE-AC02-05CH11231. Funding Information: This work used resources from the Sciama High Performance Computing cluster, which is supported by the Institute of Cosmology and Gravitation and the University of Portsmouth. Publisher Copyright: {\textcopyright} 2021 Oxford University Press. All rights reserved.",
year = "2021",
month = jan,
day = "1",
doi = "10.1093/mnras/staa3336",
language = "English (US)",
volume = "500",
pages = "3254--3274",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "3",
}