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Paolo Serra

Researcher at California Institute of Technology

Publications -  127
Citations -  30024

Paolo Serra is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Cosmic microwave background. The author has an hindex of 40, co-authored 111 publications receiving 28512 citations. Previous affiliations of Paolo Serra include University of Paris-Sud & Université Paris-Saclay.

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Planck 2015 results - XIII. Cosmological parameters

Peter A. R. Ade, +337 more
TL;DR: In this article, the authors present a cosmological analysis based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation.
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Planck 2015 results. XIII. Cosmological parameters

Peter A. R. Ade, +260 more
TL;DR: In this paper, the authors present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB, which are consistent with the six-parameter inflationary LCDM cosmology.
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Planck 2013 results. I. Overview of products and scientific results

Peter A. R. Ade, +472 more
TL;DR: The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009 as discussed by the authors.
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Planck 2015 results. I. Overview of products and scientific results

R. Adam, +353 more
TL;DR: The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submillimetre sky continuously between 12~August 2009 and 23~October 2013 as discussed by the authors.
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Planck 2015 results - XI. CMB power spectra, likelihoods, and robustness of parameters

Nabila Aghanim, +294 more
TL;DR: In this article, the authors present the Planck 2015 likelihoods, statistical descriptions of the 2-point correlation functions of the cosmic microwave background (CMB) temperature and polarization fluctuations that account for relevant uncertainties.