![]() Results are only weakly dependent on the cosmological model and remain stable, Parameters and $95\,\%$ on upper limits). Spectral index $n_s = 0.965\pm 0.004$, and optical depth $\tau = 0.054\pmĠ.007$ (in this abstract we quote $68\,\%$ confidence regions on measured A combined analysis gives dark matter density $\Omega_c h^2 =Ġ.120\pm 0.001$, baryon density $\Omega_b h^2 = 0.0224\pm 0.0001$, scalar Paper), from polarization, temperature, and lensing, separately and inĬombination. Spectrum of adiabatic scalar perturbations (denoted "base $\Lambda$CDM" in this Standard spatially-flat 6-parameter $\Lambda$CDM cosmology having a power-law ![]() Aghanim and 180 other authors Download PDF Abstract: We present cosmological parameter results from the final full-mission Planck ![]() ![]() Cosmological parameters, by Planck Collaboration: N. (82 additional authors not shown) You must enable JavaScript to view entire author list.ĭownload a PDF of the paper titled Planck 2018 results. ![]()
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