dc.contributor | Universidade de São Paulo (USP) | |
dc.contributor | Aalto Univ | |
dc.contributor | African Inst Math Sci | |
dc.contributor | Agenzia Spaziale Italiana | |
dc.contributor | Aix Marseille Univ | |
dc.contributor | Univ Cambridge | |
dc.contributor | Univ KwaZulu Natal | |
dc.contributor | ALMA Santiago Cent Off | |
dc.contributor | Univ Toronto | |
dc.contributor | IRAP | |
dc.contributor | Trinity Coll Dublin | |
dc.contributor | CALTECH | |
dc.contributor | CEFCA | |
dc.contributor | Lawrence Berkeley Natl Lab | |
dc.contributor | CEA Saclay | |
dc.contributor | Tech Univ Denmark | |
dc.contributor | Univ Geneva | |
dc.contributor | Univ Oviedo | |
dc.contributor | Radboud Univ Nijmegen | |
dc.contributor | Univ British Columbia | |
dc.contributor | Univ Southern Calif | |
dc.contributor | UCL | |
dc.contributor | Florida State Univ | |
dc.contributor | Univ Helsinki | |
dc.contributor | Princeton Univ | |
dc.contributor | Univ Calif Santa Barbara | |
dc.contributor | Univ Illinois | |
dc.contributor | Univ Padua | |
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 | |
dc.contributor | Univ La Laguna | |
dc.contributor | ESO Vitacura | |
dc.contributor | European Space Agcy | |
dc.contributor | Univ E Campus | |
dc.contributor | Ist Nazl Fis Nucl | |
dc.contributor | HGSFP | |
dc.contributor | Heidelberg Univ | |
dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.contributor | INAF Osservatorio Astron Padova | |
dc.contributor | INAF Osservatorio Astron Roma | |
dc.contributor | INAF Osservatorio Astron Trieste | |
dc.contributor | INAF IASF Bologna | |
dc.contributor | INAF IASF Milano | |
dc.contributor | Univ Roma Sapienza | |
dc.contributor | Univ Grenoble Alpes | |
dc.contributor | Imperial Coll London | |
dc.contributor | Univ Joseph Fourier Grenoble I | |
dc.contributor | Inst Univ France | |
dc.contributor | Univ Paris Sud 11 | |
dc.contributor | Inst Astrophys Paris | |
dc.contributor | Univ Oslo | |
dc.contributor | Inst Astrofis Canarias | |
dc.contributor | CSIC Univ Cantabria | |
dc.contributor | Univ Manchester | |
dc.contributor | Kavli Inst Cosmol Cambridge | |
dc.contributor | Univ Paris 11 | |
dc.contributor | Univ Savoie | |
dc.contributor | Observ Paris | |
dc.contributor | CNRS | |
dc.contributor | Telecom ParisTech | |
dc.contributor | Russian Acad Sci | |
dc.contributor | Max Planck Inst Astrophys | |
dc.contributor | Natl Univ Ireland | |
dc.contributor | Ecole Polytech Fed Lausanne | |
dc.contributor | SISSA | |
dc.contributor | Cardiff Univ | |
dc.contributor | UPMC | |
dc.contributor | Univ Calif Berkeley | |
dc.contributor | Univ Oxford | |
dc.contributor | CERN | |
dc.contributor | UPMC Univ Paris 06 | |
dc.contributor | Univ Toulouse | |
dc.contributor | Ludwig Maximilian Univ Munich | |
dc.contributor | Univ Granada | |
dc.contributor | Univ Warsaw Observ | |
dc.date.accessioned | 2018-11-26T17:06:47Z | |
dc.date.available | 2018-11-26T17:06:47Z | |
dc.date.created | 2018-11-26T17:06:47Z | |
dc.date.issued | 2016-10-01 | |
dc.identifier | Astronomy & Astrophysics. Les Ulis Cedex A: Edp Sciences S A, v. 594, 24 p., 2016. | |
dc.identifier | 1432-0746 | |
dc.identifier | http://hdl.handle.net/11449/162077 | |
dc.identifier | 10.1051/0004-6361/201525826 | |
dc.identifier | WOS:000385832200011 | |
dc.identifier | WOS000385832200011.pdf | |
dc.description.abstract | We have constructed all-sky Compton parameters maps, y-maps, of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 30 to 857 GHz frequency channel maps from the Planck satellite. These reconstructed y-maps are delivered as part of the Planck 2015 release. The y-maps are characterized in terms of noise properties and residual foreground contamination, mainly thermal dust emission at large angular scales, and cosmic infrared background and extragalactic point sources at small angular scales. Specific masks are defined to minimize foreground residuals and systematics. Using these masks, we compute the y-map angular power spectrum and higher order statistics. From these we conclude that the y-map is dominated by tSZ signal in the multipole range, 20 < l < 600. We compare the measured tSZ power spectrum and higher order statistics to various physically motivated models and discuss the implications of our results in terms of cluster physics and cosmology. | |
dc.language | eng | |
dc.publisher | Edp Sciences S A | |
dc.relation | Astronomy & Astrophysics | |
dc.rights | Acesso aberto | |
dc.source | Web of Science | |
dc.subject | large-scale structure of Universe | |
dc.subject | cosmology: observations | |
dc.title | Planck 2015 results XXII. A map of the thermal Sunyaev-Zeldovich effect | |
dc.type | Artículos de revistas | |