Compilation of recent CMB angular power spectrum measurements from which most cosmological inferences are drawn. Upper panel: power spectra of the temperature and E-mode and B-mode polarization signals, the next panel the cross-correlation spectrum between T and E, while lower panel: lensing deflection power spectrum. Different colours correspond to different experiments, each retaining its original binning. For Planck, ACTPol, and SPTpol, the EE points with large error bars are not plotted (to avoid clutter). The dashed line shows the best-fit ΛCDM model to the Planck temperature, polarization, and lensing data. See text for details and references.
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