Fig. 6.

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Confidence contours (68 and 95%) and posterior distributions for the dark energy EoS parameter w and mass calibration parameter (1 − b) when combining CMB (with or without BAO) and SZ cluster data for three different cases of allowing extensions to ΛCDM (detailed in the legends), in comparison with confidence contours from the effect of a strong prior on (1 − b) centred around the Planck calibration value of 0.8.
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