The authors fit the galaxy power spectrum of BOSS (0.3<z<0.65) and eBOSS (0.6<z<1.0) samples to obtain BAO dilation-scale parameters α, finding BOSS more precise than eBOSS and 1σ agreement with DESI III.
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples
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Baryon Acoustic Oscillations from galaxy surveys
The authors fit the galaxy power spectrum of BOSS (0.3<z<0.65) and eBOSS (0.6<z<1.0) samples to obtain BAO dilation-scale parameters α, finding BOSS more precise than eBOSS and 1σ agreement with DESI III.