Fig. 15

68% and 95% confidence contours (including systematic uncertainty) for the Ωm and ΩΛ cosmological parameters for the o-ΛCDM model. Labels for the various datasets correspond to the present SN Ia compilation (JLA), the Conley et al. (2011) SN Ia compilation (C11), the combination of Planck temperature and WMAP polarization measurements of the CMB fluctuation (Planck+WP), and a combination of measurements of the BAO scale (BAO). See Sect. 7.1 for details. The black dashed line corresponds to a flat universe.
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