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Fig. 18

image

One- and two-standard deviation constraints on the oΛCDM parameters MΛ) using BAO measurements of DM(z) /rd and DH(z) /rd without CMB measurements, i.e. without imposing the CMB value of rd. The red contours use the work presented here (line 1 of Table 6), the z< 0.8 galaxy data (Alam et al. 2016; Beutler et al. 2011; Ross et al. 2015) and the quasar-forest cross-correlation (Font-Ribera et al. 2014). The gray contours exclude the quasar-forest cross-correlation. The blue contours use only the z< 0.8 galaxy data and the green contours show the constraints derived from the SNIa Hubble diagram (Betoule et al. 2014). The black dot is the position of the flat-ΛCDM model that describes CMB data (Planck Collaboration XIII 2016).

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