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http://hdl.handle.net/10261/110557
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dc.contributor.author | Bouchet, F. R. | - |
dc.contributor.author | Barreiro, R. Belén | - |
dc.contributor.author | Bonavera, Laura | - |
dc.contributor.author | Curto, Andrés | - |
dc.contributor.author | Diego, José María | - |
dc.contributor.author | González-Nuevo, J. | - |
dc.contributor.author | Herranz, D. | - |
dc.contributor.author | López-Caniego, M. | - |
dc.contributor.author | Martínez-González, Enrique | - |
dc.contributor.author | Rebolo López, Rafael | - |
dc.contributor.author | Vielva, Patricio | - |
dc.contributor.author | Planck Collaboration | - |
dc.date.accessioned | 2015-02-12T11:48:18Z | - |
dc.date.available | 2015-02-12T11:48:18Z | - |
dc.date.issued | 2014 | - |
dc.identifier | doi: 10.1051/0004-6361/201321570 | - |
dc.identifier | e-issn: 1432-0746 | - |
dc.identifier | issn: 0004-6361 | - |
dc.identifier.citation | Astronomy and Astrophysics 571: A6 (2014) | - |
dc.identifier.uri | http://hdl.handle.net/10261/110557 | - |
dc.description.abstract | We describe the processing of the 531 billion raw data samples from the High Frequency Instrument (HFI), which we performed to produce six temperature maps from the first 473 days of Planck-HFI survey data. These maps provide an accurate rendition of the sky emission at 100, 143, 217, 353, 545, and 857 GHz with an angular resolution ranging from 9.I 7 to 4.I 6. The detector noise per (effective) beam solid angle is respectively, 10, 6, 12, and 39 μK in the four lowest HFI frequency channels (100-353 GHz) and 13 and 14 kJy sr-1 in the 545 and 857 GHz channels. Relative to the 143 GHz channel, these two high frequency channels are calibrated to within 5% and the 353 GHz channel to the percent level. The 100 and 217 GHz channels, which together with the 143 GHz channel determine the high-multipole part of the CMB power spectrum (50., 2500), are calibrated relative to 143 GHz to better than 0.2%. | - |
dc.description.sponsorship | The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). | - |
dc.publisher | EDP Sciences | - |
dc.relation.isversionof | Publisher's version | - |
dc.rights | openAccess | - |
dc.subject | Surveys | - |
dc.subject | Cosmology: observations | - |
dc.subject | Cosmic background radiation | - |
dc.subject | Methods: data analysis | - |
dc.title | Planck 2013 results. VI. High frequency instrument data processing | - |
dc.type | artículo | - |
dc.identifier.doi | 10.1051/0004-6361/201321570 | - |
dc.relation.publisherversion | http://dx.doi.org/10.1051/0004-6361/201321570 | - |
dc.date.updated | 2015-02-12T11:48:18Z | - |
dc.description.version | Peer Reviewed | - |
dc.language.rfc3066 | eng | - |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.openairetype | artículo | - |
item.grantfulltext | open | - |
Aparece en las colecciones: | (IFCA) Artículos |
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Fichero | Descripción | Tamaño | Formato | |
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VI. High Frequency.pdf | 33,47 MB | Adobe PDF | Visualizar/Abrir |
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