Constraints on ∑ mν from a joint analysis of the cluster counts and primary CMB. The solid and dashed, red and black lines reproduce the marginalized posterior distributions from Fig. 11. The solid blue line is the posterior from a similar analysis, but marginalized over the additional parameter AL (see text). If applied to the present Planck cluster cosmology sample, a future mass calibration of 1−b = 0.78 ± 0.01 would result in the bold, dotted green posterior curve.
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