dc.contributor | Universidade de São Paulo (USP) | |
dc.contributor | Aalto Univ | |
dc.contributor | Dept Radio Sci & Engn | |
dc.contributor | Acad Sci Tatarstan | |
dc.contributor | African Inst Math Sci | |
dc.contributor | Agenzia Spaziale Italiana Sci Data Ctr | |
dc.contributor | Aix Marseille Univ | |
dc.contributor | Univ Cam bridge | |
dc.contributor | Univ KwaZulu Natal | |
dc.contributor | ALMA Santiago Cent Off | |
dc.contributor | CGEE | |
dc.contributor | Univ Toronto | |
dc.contributor | IRAP | |
dc.contributor | Trinity Coll Dublin | |
dc.contributor | CALTECH | |
dc.contributor | Univ Cambridge | |
dc.contributor | CEFCA | |
dc.contributor | Lawrence Berkeley Natl Lab | |
dc.contributor | CSIC | |
dc.contributor | CEA Saclay | |
dc.contributor | Tech Univ Denmark | |
dc.contributor | Univ Geneva | |
dc.contributor | Univ Copenhagen | |
dc.contributor | Univ La Laguna ULL | |
dc.contributor | Univ Oviedo | |
dc.contributor | Univ Cantabria | |
dc.contributor | Kazan Fed Univ | |
dc.contributor | Radboud Univ Nijmegen | |
dc.contributor | Univ British Columbia | |
dc.contributor | Univ Southern Calif | |
dc.contributor | Johns Hopkins Univ | |
dc.contributor | UCL | |
dc.contributor | Univ Sussex | |
dc.contributor | Florida State Univ | |
dc.contributor | Univ Helsinki | |
dc.contributor | Princeton Univ | |
dc.contributor | Univ Alberta | |
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dc.contributor | Univ Calif Santa Barbara | |
dc.contributor | Univ Illinois | |
dc.contributor | Univ Padua | |
dc.contributor | Univ Bologna | |
dc.contributor | Univ Ferrara | |
dc.contributor | Univ Roma La Sapienza | |
dc.contributor | Univ Milan | |
dc.contributor | Univ Trieste | |
dc.contributor | Univ Roma Tor Vergata | |
dc.contributor | Niels Bohr Inst | |
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dc.contributor | ESAC | |
dc.contributor | ESTEC | |
dc.contributor | Univ Turku | |
dc.contributor | Observ Paris | |
dc.contributor | INFN | |
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dc.contributor | Heidelberg Univ | |
dc.contributor | Haverford Coll | |
dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.contributor | INAF | |
dc.contributor | IASF Bologna | |
dc.contributor | IASF Milano | |
dc.contributor | Univ Roma Sapienza | |
dc.contributor | Natl Inst Nucl Phys | |
dc.contributor | Univ Grenoble Alpes | |
dc.contributor | CNRS | |
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dc.contributor | Imperial Coll London | |
dc.contributor | Univ Joseph Fourier Grenoble I | |
dc.contributor | Inst Univ France | |
dc.contributor | Univ Paris Saclay | |
dc.contributor | Inst Astrophys Paris | |
dc.contributor | Rhein Westfal TH Aachen | |
dc.contributor | Inst Space Sci | |
dc.contributor | Univ Oslo | |
dc.contributor | INAOE | |
dc.contributor | Inst Astrofis Canarias | |
dc.contributor | Ist Nazl Astrofis | |
dc.contributor | Ist Nazl Fis Nucl | |
dc.contributor | Univ Manchester | |
dc.contributor | Univ Chicago | |
dc.contributor | Kavli Inst Cosmol Cambridge | |
dc.contributor | Univ Paris 11 | |
dc.contributor | Telecom ParisTech | |
dc.contributor | Univ Paris Sud 11 | |
dc.contributor | Russian Acad Sci | |
dc.contributor | Natl Taiwan Univ | |
dc.contributor | Max Planck Inst Astrophys | |
dc.contributor | Max Planck Inst Extraterr Phys | |
dc.contributor | McGill Univ | |
dc.contributor | Moscow Inst Phys & Technol | |
dc.contributor | Univ Coll London | |
dc.contributor | Natl Univ Ireland | |
dc.contributor | Nicolaus Copernicus Astron Ctr | |
dc.contributor | Nordita Nord Inst Theoret Phys | |
dc.contributor | Perimeter Inst Theoret Phys | |
dc.contributor | Shahid Beheshti Univ | |
dc.contributor | SISSA | |
dc.contributor | Univ E Campus | |
dc.contributor | Cardiff Univ | |
dc.contributor | Univ Nottingham | |
dc.contributor | Simon Fraser Univ | |
dc.contributor | UPMC | |
dc.contributor | Stanford Univ | |
dc.contributor | Sterrewacht Leiden | |
dc.contributor | Univ Oxford | |
dc.contributor | Univ Sydney | |
dc.contributor | TUBITAK Natl Observ | |
dc.contributor | Stockholm Univ | |
dc.contributor | CERN | |
dc.contributor | UPMC Univ Paris 06 | |
dc.contributor | Univ Toulouse | |
dc.contributor | Stratospher Observ Infrared Astron | |
dc.contributor | Ludwig Maximilian Univ Munich | |
dc.contributor | Univ Granada | |
dc.contributor | Univ Warsaw Observ | |
dc.date.accessioned | 2018-11-26T17:06:58Z | |
dc.date.available | 2018-11-26T17:06:58Z | |
dc.date.created | 2018-11-26T17:06:58Z | |
dc.date.issued | 2016-10-01 | |
dc.identifier | Astronomy & Astrophysics. Les Ulis Cedex A: Edp Sciences S A, v. 594, 38 p., 2016. | |
dc.identifier | 1432-0746 | |
dc.identifier | http://hdl.handle.net/11449/162079 | |
dc.identifier | 10.1051/0004-6361/201527101 | |
dc.identifier | WOS:000385832200030 | |
dc.identifier | WOS000385832200030.pdf | |
dc.description.abstract | The European Space Agency's Planck satellite, which is dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013. In February 2015, ESA and the Planck Collaboration released the second set of cosmology products based on data from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the main characteristics of the data and the data products in the release, as well as the associated cosmological and astrophysical science results and papers. The data products include maps of the cosmic microwave background (CMB), the thermal Sunyaev-Zeldovich effect, diffuse foregrounds in temperature and polarization, catalogues of compact Galactic and extragalactic sources (including separate catalogues of Sunyaev-Zeldovich clusters and Galactic cold clumps), and extensive simulations of signals and noise used in assessing uncertainties and the performance of the analysis methods. The likelihood code used to assess cosmological models against the Planck data is described, along with a CMB lensing likelihood. Scientific results include cosmological parameters derived from CMB power spectra, gravitational lensing, and cluster counts, as well as constraints on inflation, non-Gaussianity, primordial magnetic fields, dark energy, and modified gravity, and new results on low-frequency Galactic foregrounds. | |
dc.language | eng | |
dc.publisher | Edp Sciences S A | |
dc.relation | Astronomy & Astrophysics | |
dc.rights | Acesso aberto | |
dc.source | Web of Science | |
dc.subject | cosmology: observations | |
dc.subject | cosmic background radiation | |
dc.subject | surveys | |
dc.subject | space vehicles: instruments | |
dc.subject | instrumentation: detectors | |
dc.title | Planck 2015 results I. Overview of products and scientific results | |
dc.type | Artículos de revistas | |