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Nicola Bartolo

Researcher at University of Padua

Publications -  203
Citations -  36803

Nicola Bartolo is an academic researcher from University of Padua. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 83, co-authored 203 publications receiving 30579 citations. Previous affiliations of Nicola Bartolo include Istituto Nazionale di Fisica Nucleare & International Centre for Theoretical Physics.

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Planck 2018 results. VII. Isotropy and Statistics of the CMB

Yashar Akrami, +148 more
TL;DR: In this article, a comprehensive analysis of the statistics of the polarization signal over all angular scales, using either maps of the Stokes parameters, $Q$ and $U$, or the $E$-mode signal derived from these using a new methodology is presented.
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Planck 2013 results. XXIV. Constraints on primordial non-Gaussianity

Peter A. R. Ade, +302 more
TL;DR: The Planck nominal mission cosmic microwave background (CMB) maps yield unprecedented constraints on primordial non-Gaussianity (NG) using three optimal bispectrum estimators, separable template-fitting (KSW), binned, and modal as discussed by the authors.
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Planck 2018 results. VIII. Gravitational lensing

Nabila Aghanim, +205 more
TL;DR: In this article, the authors presented an extensive set of tests of the robustness of the lensing-potential power spectrum, and constructed a minimum-variance estimator likelihood over lensing multipoles 8.
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Planck 2018 results. IX. Constraints on primordial non-Gaussianity

Yashar Akrami, +190 more
TL;DR: In this paper, the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps were used to obtain constraints on primordial non-Gaussianity.
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Planck intermediate results - XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

R. Adam, +301 more
TL;DR: In this article, the authors exploit the uniqueness of the Planck HFI polarization data from 100 to 353 GHz to measure the polarized dust angular power spectra C_l^(EE) and C_ l^(BB) over the multipole range 40