The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample�…
JE Bautista, R Paviot, M Vargas Maga�a…�- Monthly Notices of�…, 2021 - academic.oup.com
We present the cosmological analysis of the configuration-space anisotropic clustering in
the completed Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic
Survey (eBOSS) Data Release 16 galaxy sample. This sample consists of luminous red
galaxies (LRGs) spanning the redshift range 0.6<< 1, at an effective redshift of eff= 0.698. It
combines 174 816 eBOSS and 202 642 BOSS LRGs. We extract and model the baryon
acoustic oscillation (BAO) and redshift-space distortion (RSD) features from the galaxy two�…
the completed Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic
Survey (eBOSS) Data Release 16 galaxy sample. This sample consists of luminous red
galaxies (LRGs) spanning the redshift range 0.6<< 1, at an effective redshift of eff= 0.698. It
combines 174 816 eBOSS and 202 642 BOSS LRGs. We extract and model the baryon
acoustic oscillation (BAO) and redshift-space distortion (RSD) features from the galaxy two�…
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the quasar sample�…
J Hou, AG S�nchez, AJ Ross, A Smith…�- Monthly Notices of�…, 2021 - academic.oup.com
We measure the anisotropic clustering of the quasar sample from Data Release 16 (DR16)
of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey
(eBOSS). A sample of 343 708 spectroscopically confirmed quasars between redshift 0.8<
z< 2.2 are used as tracers of the underlying dark matter field. In comparison with DR14
sample, the final sample doubles the number of objects as well as the survey area. In this
paper, we present the analysis in configuration space by measuring the two-point correlation�…
of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey
(eBOSS). A sample of 343 708 spectroscopically confirmed quasars between redshift 0.8<
z< 2.2 are used as tracers of the underlying dark matter field. In comparison with DR14
sample, the final sample doubles the number of objects as well as the survey area. In this
paper, we present the analysis in configuration space by measuring the two-point correlation�…