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

被引：91

作者：

Raichoor, Anand ^{[1
]}

de Mattia, Arnaud ^{[2
]}

Ross, Ashley J. ^{[3
]}

Zhao, Cheng ^{[1
]}

Alam, Shadab ^{[4
]}

Avila, Santiago ^{[5
,6
]}

Bautista, Julian ^{[7
]}

Brinkmann, Jonathan ^{[8
,9
]}

Brownstein, Joel R. ^{[10
]}

Burtin, Etienne ^{[2
]}

Chapman, Michael J. ^{[11
,12
]}

Chuang, Chia-Hsun ^{[13
]}

Comparat, Johan ^{[14
]}

Dawson, Kyle S. ^{[10
]}

Dey, Arjun ^{[15
]}

des Bourboux, Helion du Mas ^{[10
]}

Elvin-Poole, Jack ^{[3
]}

Gonzalez-Perez, Violeta ^{[7
,16
]}

Gorgoni, Claudio ^{[1
]}

Kneib, Jean-Paul ^{[1
,17
]}

Kong, Hui ^{[3
]}

Lang, Dustin ^{[12
,18
]}

Moustakas, John ^{[19
]}

Myers, Adam D. ^{[20
]}

Mueller, Eva-Maria ^{[21
]}

Nadathur, Seshadri ^{[7
]}

Newman, Jeffrey A. ^{[22
,23
]}

Percival, Will J. ^{[11
,12
,18
]}

Rezaie, Mehdi ^{[24
]}

Rossi, Graziano ^{[25
]}

Ruhlmann-Kleider, Vanina ^{[2
]}

Schlegel, David J. ^{[26
]}

Schneider, Donald P. ^{[27
,28
]}

Seo, Hee-Jong ^{[24
]}

Tamone, Amelie ^{[1
]}

Tinker, Jeremy L. ^{[29
]}

Tojeiro, Rita ^{[30
]}

Vivek, M. ^{[27
,31
]}

Yeche, Christophe ^{[2
,26
]}

Zhao, Gong-Bo ^{[7
,32
,33
]}

机构：

[1] Ecole Polytech Fed Lausanne EPFL, Observ Sauverny, Lab Astrophys, Inst Phys, CH-1290 Versoix, Switzerland

[2] Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France

[3] Ohio State Univ, Ctr Cosmol & AstroParticle Phys, Columbus, OH 43212 USA

[4] Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

[5] Univ Autonoma Madrid, E-28049 Madrid, Spain

[6] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain

[7] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg,Burnaby Rd, Portsmouth PO1 3FX, Hants, England

[8] Apache Point Observ, POB 59, Sunspot, NM 88349 USA

[9] New Mexico State Univ, POB 59, Sunspot, NM 88349 USA

[10] Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA

[11] Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L 3G1, Canada

[12] Univ Waterloo, Dept Phys & Astron, 200 Univ Ave W, Waterloo, ON N2L 3G1, Canada

[13] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA

[14] Max Planck Inst Extraterr Phys MPE, Giessenbachstr 1, D-85748 Garrhing, Germany

[15] NSFs Natl Opt Infrared Astron Res Lab, 950 N Cherry Ave, Tucson, AZ 85719 USA

[16] Liverpool John Moores Univ, Astrophys Res Inst, 146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England

[17] Aix Marseille Univ, LAM, CNES, CNRS, F-13388 Marseille, France

[18] Perimeter Inst, Waterloo, ON N2L 2Y5, Canada

[19] Siena Coll, Dept Phys & Astron, 515 Loudon Rd, Loudonville, NY 12211 USA

[20] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA

[21] Univ Oxford, Dept Phys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England

[22] Univ Pittsburgh, Pittsburgh, PA 15260 USA

[23] PITT PACC, Pittsburgh, PA 15260 USA

[24] Ohio Univ, Dept Phys & Astron, Clippinger Labs, Athens, OH 45701 USA

[25] Sejong Univ, Dept Phys & Astron, Seoul 143747, South Korea

[26] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[27] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[28] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA

[29] NYU, Ctr Cosmol & Particle Phys, Dept Phys, 726 Broadway,Room 1005, New York, NY 10003 USA

[30] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland

[31] Indian Inst Astrophys, Bangalore 560034, Karnataka, India

[32] Chinese Acad Sci, Natl Astron Observ China, 20A Datun Rd, Beijing 100012, Peoples R China

[33] Univ Chinese Acad Sci, Beijing 100049, Peoples R China

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2021年 / 500卷 / 03期

基金：

欧盟地平线“2020”; 欧洲研究理事会; 美国国家科学基金会; 美国安德鲁·梅隆基金会; 新加坡国家研究基金会; 英国科学技术设施理事会;

关键词：

galaxies: distances and redshifts; dark energy; distance scale; large-scale structure of Universe; cosmology: observations; DARK ENERGY SURVEY; LUMINOUS RED GALAXY; DIGITAL SKY SURVEY; ANISOTROPIC POWER SPECTRUM; STAR-FORMATION HISTORY; ACOUSTIC-OSCILLATIONS; DISTANCE MEASUREMENTS; QUASAR SAMPLE; GROWTH-RATE; RECONSTRUCTION;

D O I：

10.1093/mnras/staa3336

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 (Delta chi(2) < 1). Fitting a model constrained to have a BAO feature provides a 3.2 per cent measurement of the spherically averaged BAO distance D-V(z(eff))/r(drag) = 18.23 +/- 0.58 at the effective redshift z(eff) = 0.845.

引用

页码：3254 / 3274

页数：21

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