Constraints on the matter and dark-energy density parameters (Ω_M,Ω_Λ) assuming a dark-energy pressure-density ratio w = −1. The blue regions are the one and two standard deviation constraints derived from our contours in Fig. 16 (method 2, broadband 24) combined with a measurement of H₀ (Riess et al. 2011). Also shown are one and two standard deviation contours from lower redshift measurements of D_V/r_s (also combined with H₀) at z = 0.11 (6dF: Beutler et al. 2011), z = 0.35 (LRG: Percival et al. 2010) and z = 0.57 (CMASS: Anderson et al. 2012). All constraints use a WMAP7 (Komatsu et al. 2011) prior on the baryon-to-photon ratio η but do not otherwise incorporate CMB results.