Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7594
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dc.contributor.authordu Mas des Bourboux, H-
dc.contributor.authorRich, J-
dc.contributor.authorFont-Ribera, A-
dc.contributor.authorde Sainte Agathe, V-
dc.contributor.authorFarr, J-
dc.contributor.authorEtourneau, T-
dc.contributor.authorLe Goff, J.-M-
dc.contributor.authorCuceu, Andrei-
dc.contributor.authorBalland, C-
dc.contributor.authorBautista, J. E-
dc.contributor.authorBlomqvist, M-
dc.contributor.authorBrinkmann, J-
dc.contributor.authorBrownstein, J. R-
dc.contributor.authorChabanier, S-
dc.contributor.authorChaussidon, E-
dc.contributor.authorDawson, K-
dc.contributor.authorGonzalez-Morales, A. X-
dc.contributor.authorGuy, J-
dc.contributor.authorLyke, B. W-
dc.contributor.authorde la Macorra, A-
dc.contributor.authorMueller, E.-M-
dc.contributor.authorMyers, A. D-
dc.contributor.authorNitschelm, C-
dc.contributor.authorGutierrez, A. M-
dc.contributor.authorPalanque-Delabrouille, N-
dc.contributor.authorParker, J-
dc.contributor.authorPercival, W. J-
dc.contributor.authorPerez-Rafols, I-
dc.contributor.authorPetitjean, P-
dc.contributor.authorPieri, M. M-
dc.contributor.authorRavoux, R-
dc.contributor.authorRossi, R-
dc.contributor.authorSchneider, D. P-
dc.contributor.authorSeo, H.-J-
dc.contributor.authorSlosar, A-
dc.contributor.authorStermer, J-
dc.contributor.authorVivek, M-
dc.contributor.authorYeche, C-
dc.contributor.authorYoules, S-
dc.date.accessioned2021-02-07T04:46:48Z-
dc.date.available2021-02-07T04:46:48Z-
dc.date.issued2020-10-01-
dc.identifier.citationThe Astrophysical Journal, Vol. 901, No. 2, 153en_US
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/7594-
dc.descriptionRestricted Access © The American Astronomical Society https://doi.org/10.3847/1538-4357/abb085en_US
dc.description.abstractWe present a measurement of baryonic acoustic oscillations (BAOs) from Lyα absorption and quasars at an effective redshift z = 2.33 using the complete extended Baryonic Oscillation Spectroscopic Survey (eBOSS). The 16th and final eBOSS data release (SDSS DR16) contains all data from eBOSS and its predecessor, the Baryonic Oscillation Spectroscopic Survey (BOSS), providing 210,005 quasars with zq > 2.10 that are used to measure Lyα absorption. We measure the BAO scale both in the autocorrelation of Lyα absorption and in its cross-correlation with 341,468 quasars with redshift zq > 1.77. Apart from the statistical gain from new quasars and deeper observations, the main improvements over previous work come from more accurate modeling of physical and instrumental correlations and the use of new sets of mock data. Combining the BAO measurement from the auto- and cross-correlation yields the constraints of the two ratios DH (z = 2.33 8.99 0.19 ) rd =  and DM d ( ) z r = = 2.33 37.5 1.1, where the error bars are statistical. These results are within 1.5σ of the prediction of the flat-ΛCDM cosmology of Planck (2016). The analysis code, picca, the catalog of the flux transmission field measurements, and the Δχ2 surfaces are publicly available.en_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.subjectDark energyen_US
dc.subjectCosmologyen_US
dc.subjectLarge-scale structure of the universeen_US
dc.subjectBaryon acoustic oscillationsen_US
dc.subjectLyman alpha foresten_US
dc.titleThe Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations with Lyα Forestsen_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications



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