Fig. 12

Upper left: Planck
measurements of the lensing power spectrum compared to the ΛCDM mean prediction and 68%
confidence interval (dashed lines) for models fit to
Planck+WP+highL (see text). The eight bandpowers are those used
in the Planck lensing likelihood; they are renormalized, along
with their errors, to account for the small differences between the lensed
in the best-fit model and the
fiducial model used throughout this paper. The error bars are the ± 1σ errors from
the diagonal of the covariance matrix. The colour coding shows how
varies with the optical depth
τ
across samples from the ΛCDM posterior distribution. Upper right: as
upper-left but using only the temperature power spectrum from
Planck. Lower left: as upper-left panel but in
models with spatial curvature. The colour coding is for ΩK.
Lower right: as upper-left but in models with three massive
neutrinos (of equal mass). The colour coding is for the summed neutrino mass
∑
mν.
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