Table 5.
BAO data used in this analysis.
| Survey set I | z | 𝒟V(z) | σ𝒟 |
 |
|---|---|---|---|---|
| 6dFGS | 0.106 | 457 | 27 | 153.55 |
| SDSS-LRG | 0.35 | 1356 | 25 | 152.76 |
| SDSS-MGS | 0.15 | 664 | 25 | 148.69 |
| BOSS-DR12 | 0.38 | 1477 | 16 | 147.78 |
| BOSS-DR12 | 0.51 | 1877 | 19 | 147.78 |
| BOSS-DR12 | 0.61 | 2140 | 22 | 147.78 |
| Survey set II | z | 𝒟V(z) | σ𝒟 |
 |
| WiggleZ | 0.44 | 1716 | – | 148.6 |
| WiggleZ | 0.60 | 2221 | – | 148.6 |
| WiggleZ | 0.73 | 2516 | – | 148.6 |
Notes. The data come from seven different surveys: the 6dF Galaxy Survey (6dFGS) (Beutler et al. 2011), the Sloan Digital Sky Survey luminous red galaxy (SDSS-LRG) (Padmanabhan et al. 2012), SDSS data release 7 main galaxy sample (SDSS-MGS) (Ross et al. 2015), the Baryon Oscillation Spectroscopic Survey data release 12 (BOSS-DR12) (Alam et al. 2017) and from the WiggleZ Dark Energy Survey (Kazin et al. 2014). 𝒟V(z), σ𝒟 and 
are given in Mpc. The σ𝒟 are not shown here because the three WiggleZ measurements are correlated and we take the full covariance matrix in the analysis.
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