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Fig. 12


Comparison of various estimations of cosmological parameters, together with their 68% CL, in the ΛCDM(3ν), νΛCDM(3ν) and ΛCDM(1ν) models, from the combination of: the high-Planck (hlpALL, hlpALLps or PlikALL separated by the vertical dashed lines); the lowTEB likelihood or a τreio auxiliary constraint; Commander; the CMB lensing from Planck; BAO; and SNIa. Those results, derived from profile likelihood analyses, are compared (last point in black) to the Planck 2015 results with a similar data combination (last column of Table 4, in Planck Collaboration XIII 2016).

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