The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function

Ashley J. Ross, Florian Beutler, Chia Hsun Chuang, Marcos Pellejero-Ibanez, Hee Jong Seo, Mariana Vargas-Magaña, Antonio J. Cuesta, Will J. Percival, Angela Burden, Ariel G. Sánchez, Jan Niklas Grieb, Beth Reid, Joel R. Brownstein, Kyle S. Dawson, Daniel J. Eisenstein, Shirley Ho, Francisco Shu Kitaura, Robert C. Nichol, Matthew D. Olmstead, Francisco PradaSergio A. Rodríguez-Torres, Shun Saito, Salvador Salazar-Albornoz, Donald P. Schneider, Daniel Thomas, Jeremy Tinker, Rita Tojeiro, Yuting Wang, Martin White, Gong Bo Zhao

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Abstract

We present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1.2 million massive galaxies with redshifts 0.2 < z < 0.75 distributed over 9300 deg2, as quantified by their redshift-space correlation function. In order to facilitate these measurements, we define, describe, and motivate the selection function for galaxies in the final data release (DR12) of the SDSS III Baryon Oscillation Spectroscopic Survey (BOSS). This includes the observational footprint, masks for image quality and Galactic extinction, and weights to account for density relationships intrinsic to the imaging and spectroscopic portions of the survey. We simulate the observed systematic trends in mock galaxy samples and demonstrate that they impart no bias on BAO scale measurements and have a minor impact on the recovered statistical uncertainty. We measure transverse and radial BAO distance measurements in 0.2 < z < 0.5, 0.5 < z < 0.75, and (overlapping) 0.4 < z < 0.6 redshift bins. In each redshift bin, we obtain a precision that is 2.7 per cent or better on the radial distance and 1.6 per cent or better on the transverse distance. The combination of the redshift bins represents 1.8 per cent precision on the radial distance and 1.1 per cent precision on the transverse distance. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. The measurements and likelihoods presented here are combined with others in Alam et al. to produce the final cosmological constraints from BOSS.

Original languageEnglish (US)
Pages (from-to)1168-1191
Number of pages24
JournalMonthly Notices of the Royal Astronomical Society
Volume464
Issue number1
DOIs
StatePublished - Jan 1 2017

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baryons
acoustics
oscillation
galaxies
oscillations
footprints
footprint
extinction
masks
trends

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Ross, Ashley J. ; Beutler, Florian ; Chuang, Chia Hsun ; Pellejero-Ibanez, Marcos ; Seo, Hee Jong ; Vargas-Magaña, Mariana ; Cuesta, Antonio J. ; Percival, Will J. ; Burden, Angela ; Sánchez, Ariel G. ; Grieb, Jan Niklas ; Reid, Beth ; Brownstein, Joel R. ; Dawson, Kyle S. ; Eisenstein, Daniel J. ; Ho, Shirley ; Kitaura, Francisco Shu ; Nichol, Robert C. ; Olmstead, Matthew D. ; Prada, Francisco ; Rodríguez-Torres, Sergio A. ; Saito, Shun ; Salazar-Albornoz, Salvador ; Schneider, Donald P. ; Thomas, Daniel ; Tinker, Jeremy ; Tojeiro, Rita ; Wang, Yuting ; White, Martin ; Zhao, Gong Bo. / The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : Observational systematics and baryon acoustic oscillations in the correlation function. In: Monthly Notices of the Royal Astronomical Society. 2017 ; Vol. 464, No. 1. pp. 1168-1191.
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abstract = "We present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1.2 million massive galaxies with redshifts 0.2 < z < 0.75 distributed over 9300 deg2, as quantified by their redshift-space correlation function. In order to facilitate these measurements, we define, describe, and motivate the selection function for galaxies in the final data release (DR12) of the SDSS III Baryon Oscillation Spectroscopic Survey (BOSS). This includes the observational footprint, masks for image quality and Galactic extinction, and weights to account for density relationships intrinsic to the imaging and spectroscopic portions of the survey. We simulate the observed systematic trends in mock galaxy samples and demonstrate that they impart no bias on BAO scale measurements and have a minor impact on the recovered statistical uncertainty. We measure transverse and radial BAO distance measurements in 0.2 < z < 0.5, 0.5 < z < 0.75, and (overlapping) 0.4 < z < 0.6 redshift bins. In each redshift bin, we obtain a precision that is 2.7 per cent or better on the radial distance and 1.6 per cent or better on the transverse distance. The combination of the redshift bins represents 1.8 per cent precision on the radial distance and 1.1 per cent precision on the transverse distance. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. The measurements and likelihoods presented here are combined with others in Alam et al. to produce the final cosmological constraints from BOSS.",
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Ross, AJ, Beutler, F, Chuang, CH, Pellejero-Ibanez, M, Seo, HJ, Vargas-Magaña, M, Cuesta, AJ, Percival, WJ, Burden, A, Sánchez, AG, Grieb, JN, Reid, B, Brownstein, JR, Dawson, KS, Eisenstein, DJ, Ho, S, Kitaura, FS, Nichol, RC, Olmstead, MD, Prada, F, Rodríguez-Torres, SA, Saito, S, Salazar-Albornoz, S, Schneider, DP, Thomas, D, Tinker, J, Tojeiro, R, Wang, Y, White, M & Zhao, GB 2017, 'The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function', Monthly Notices of the Royal Astronomical Society, vol. 464, no. 1, pp. 1168-1191. https://doi.org/10.1093/mnras/stw2372

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : Observational systematics and baryon acoustic oscillations in the correlation function. / Ross, Ashley J.; Beutler, Florian; Chuang, Chia Hsun; Pellejero-Ibanez, Marcos; Seo, Hee Jong; Vargas-Magaña, Mariana; Cuesta, Antonio J.; Percival, Will J.; Burden, Angela; Sánchez, Ariel G.; Grieb, Jan Niklas; Reid, Beth; Brownstein, Joel R.; Dawson, Kyle S.; Eisenstein, Daniel J.; Ho, Shirley; Kitaura, Francisco Shu; Nichol, Robert C.; Olmstead, Matthew D.; Prada, Francisco; Rodríguez-Torres, Sergio A.; Saito, Shun; Salazar-Albornoz, Salvador; Schneider, Donald P.; Thomas, Daniel; Tinker, Jeremy; Tojeiro, Rita; Wang, Yuting; White, Martin; Zhao, Gong Bo.

In: Monthly Notices of the Royal Astronomical Society, Vol. 464, No. 1, 01.01.2017, p. 1168-1191.

Research output: Contribution to journalArticle

TY - JOUR

T1 - The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey

T2 - Observational systematics and baryon acoustic oscillations in the correlation function

AU - Ross, Ashley J.

AU - Beutler, Florian

AU - Chuang, Chia Hsun

AU - Pellejero-Ibanez, Marcos

AU - Seo, Hee Jong

AU - Vargas-Magaña, Mariana

AU - Cuesta, Antonio J.

AU - Percival, Will J.

AU - Burden, Angela

AU - Sánchez, Ariel G.

AU - Grieb, Jan Niklas

AU - Reid, Beth

AU - Brownstein, Joel R.

AU - Dawson, Kyle S.

AU - Eisenstein, Daniel J.

AU - Ho, Shirley

AU - Kitaura, Francisco Shu

AU - Nichol, Robert C.

AU - Olmstead, Matthew D.

AU - Prada, Francisco

AU - Rodríguez-Torres, Sergio A.

AU - Saito, Shun

AU - Salazar-Albornoz, Salvador

AU - Schneider, Donald P.

AU - Thomas, Daniel

AU - Tinker, Jeremy

AU - Tojeiro, Rita

AU - Wang, Yuting

AU - White, Martin

AU - Zhao, Gong Bo

PY - 2017/1/1

Y1 - 2017/1/1

N2 - We present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1.2 million massive galaxies with redshifts 0.2 < z < 0.75 distributed over 9300 deg2, as quantified by their redshift-space correlation function. In order to facilitate these measurements, we define, describe, and motivate the selection function for galaxies in the final data release (DR12) of the SDSS III Baryon Oscillation Spectroscopic Survey (BOSS). This includes the observational footprint, masks for image quality and Galactic extinction, and weights to account for density relationships intrinsic to the imaging and spectroscopic portions of the survey. We simulate the observed systematic trends in mock galaxy samples and demonstrate that they impart no bias on BAO scale measurements and have a minor impact on the recovered statistical uncertainty. We measure transverse and radial BAO distance measurements in 0.2 < z < 0.5, 0.5 < z < 0.75, and (overlapping) 0.4 < z < 0.6 redshift bins. In each redshift bin, we obtain a precision that is 2.7 per cent or better on the radial distance and 1.6 per cent or better on the transverse distance. The combination of the redshift bins represents 1.8 per cent precision on the radial distance and 1.1 per cent precision on the transverse distance. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. The measurements and likelihoods presented here are combined with others in Alam et al. to produce the final cosmological constraints from BOSS.

AB - We present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1.2 million massive galaxies with redshifts 0.2 < z < 0.75 distributed over 9300 deg2, as quantified by their redshift-space correlation function. In order to facilitate these measurements, we define, describe, and motivate the selection function for galaxies in the final data release (DR12) of the SDSS III Baryon Oscillation Spectroscopic Survey (BOSS). This includes the observational footprint, masks for image quality and Galactic extinction, and weights to account for density relationships intrinsic to the imaging and spectroscopic portions of the survey. We simulate the observed systematic trends in mock galaxy samples and demonstrate that they impart no bias on BAO scale measurements and have a minor impact on the recovered statistical uncertainty. We measure transverse and radial BAO distance measurements in 0.2 < z < 0.5, 0.5 < z < 0.75, and (overlapping) 0.4 < z < 0.6 redshift bins. In each redshift bin, we obtain a precision that is 2.7 per cent or better on the radial distance and 1.6 per cent or better on the transverse distance. The combination of the redshift bins represents 1.8 per cent precision on the radial distance and 1.1 per cent precision on the transverse distance. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. The measurements and likelihoods presented here are combined with others in Alam et al. to produce the final cosmological constraints from BOSS.

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