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Feb 15, 2024 · Large-scale polarized power spectra. The foregrounds are stronger in polarization relative to the CMB than in temperature and cleaning the Planck frequencies ...
Feb 3, 2024 · Planck 2015 results-XI. CMB power spectra, likelihoods, and robustness of parameters. N Aghanim, M Arnaud, M Ashdown, J Aumont, C Baccigalupi, AJ Banday ...
Jun 24, 2024 · Planck 2015 results — XI. CMB power spectra, likelihoods, and robustness of parameters. A&A 594, A11 (2016). Planck 2018 results — VI. Cosmological parameters
Jun 11, 2024 · (Planck), Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters, Astron. Astrophys. 594, A11 (2016), · arXiv:1507.02704 [astro ...
Jul 30, 2024 · CMB power spectra, likelihoods, and robustness of parameters, Astron. Astrophys. 594, A11 (2016). N. Aghanim et al. (Planck Collaboration), Planck 2018 results.
Jul 18, 2024 · [102] Planck Collaboration, N. Aghanim et al., “Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters,” Astron. Astrophys ...
Feb 6, 2024 · This section describes the High-` Likelihood on Polarized. Power spectra (HiLLiPoP), including the models used for the foreground residuals and the instrumental ...
Jun 15, 2024 · Aghanim, et al. Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters. Astron. Astrophys., 594 (2016), p. A11, 10.1051/0004 ...
Oct 14, 2024 · This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlation functions of CMB temperature and polarization. They use the ...
Dec 10, 2023 · September 2016 • Planck Collaboration • Ade, P. A. R. • Aghanim, N. • et al. Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of ...