TY - JOUR
T1 - The large-scale 3-point correlation function of the SDSS BOSS DR12 CMASS galaxies
AU - Slepian, Zachary
AU - Eisenstein, Daniel J.
AU - Beutler, Florian
AU - Chuang, Chia-Hsun
AU - Cuesta, Antonio J.
AU - Ge, Jian
AU - Gil Marin, Hector
AU - Ho, Shirley
AU - Kitaura, Francisco-Shu
AU - McBride, Cameron K.
AU - Nichol, Bob
AU - Percival, Will
AU - Rodríguez-Torres, Sergio
AU - Ross, Ashley Jacob
AU - Scoccimarro, Roman
AU - Seo, Hee-Jong
AU - Tinker, Jeremy L.
AU - Tojeiro, Rita
AU - Vargas Magana, Mariana
PY - 2017/6/11
Y1 - 2017/6/11
N2 - We report a measurement of the large-scale three-point correlation function of galaxies using the largest data set for this purpose to date, 777 202 luminous red galaxies in the Sloan Digital Sky Survey Baryon Acoustic Oscillation Spectroscopic Survey (SDSS BOSS) DR12 CMASS sample. This work exploits the novel algorithm of Slepian & Eisenstein to compute the multipole moments of the 3PCF in O(N 2) time, with N the number of galaxies. Leading-order perturbation theory models the data well in a compressed basis where one triangle side is integrated out. We also present an accurate and computationally efficient means of estimating the covariance matrix. With these techniques, the redshift-space linear and non-linear bias are measured, with 2.6 per cent precision on the former if σ8 is fixed. The data also indicate a 2.8σ preference for the BAO, confirming the presence of BAO in the three-point function.
AB - We report a measurement of the large-scale three-point correlation function of galaxies using the largest data set for this purpose to date, 777 202 luminous red galaxies in the Sloan Digital Sky Survey Baryon Acoustic Oscillation Spectroscopic Survey (SDSS BOSS) DR12 CMASS sample. This work exploits the novel algorithm of Slepian & Eisenstein to compute the multipole moments of the 3PCF in O(N 2) time, with N the number of galaxies. Leading-order perturbation theory models the data well in a compressed basis where one triangle side is integrated out. We also present an accurate and computationally efficient means of estimating the covariance matrix. With these techniques, the redshift-space linear and non-linear bias are measured, with 2.6 per cent precision on the former if σ8 is fixed. The data also indicate a 2.8σ preference for the BAO, confirming the presence of BAO in the three-point function.
U2 - 10.1093/mnras/stw3234
DO - 10.1093/mnras/stw3234
M3 - Article
SN - 0035-8711
VL - 468
SP - 1070
EP - 1083
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 1
ER -