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Paolo Natoli

Researcher at University of Ferrara

Publications -  332
Citations -  98751

Paolo Natoli is an academic researcher from University of Ferrara. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 122, co-authored 326 publications receiving 86885 citations. Previous affiliations of Paolo Natoli include Istituto Nazionale di Fisica Nucleare & Agenzia Spaziale Italiana.

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Planck 2013 results. XV. CMB power spectra and likelihood

Peter A. R. Ade, +258 more
TL;DR: In this article, the Planck likelihood is used to derive the CMB power spectrum over three decades in l, covering 2 = 50, and employ a correlated Gaussian likelihood approximation based on angular cross-spectra derived from the 100, 143 and 217 GHz channels.
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Planck 2018 results: V. CMB power spectra and likelihoods

Nabila Aghanim, +216 more
TL;DR: In this article, the legacy Planck cosmic microwave background (CMB) likelihoods derived from the 2018 data release are described, with a hybrid method using different approximations at low (l ǫ ≥ 30) multipoles, implementing several methodological and data-analysis refinements compared to previous releases.
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Planck 2015 results - X. Diffuse component separation: Foreground maps

R. Adam, +284 more
TL;DR: In this paper, the authors consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to derive an internally consistent set of full-sky astrophysical components maps.
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Planck 2015 results - XV. Gravitational lensing

Peter A. R. Ade, +292 more
TL;DR: The most significant measurement of the cosmic microwave background (CMB) lensing potential at a level of 40σ using temperature and polarization data from the Planck 2015 full-mission release was presented in this article.
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Planck 2013 results. XV. CMB power spectra and likelihood

Peter A. R. Ade, +328 more
TL;DR: The Planck 2013 likelihood as mentioned in this paper is a complete statistical description of the two-point correlation function of the CMB temperature fluctuations that accounts for all known relevant uncertainties, both instrumental and astrophysical in nature.