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dc.contributor.authorAkrami, Y.
dc.contributor.authorBarreiro Vilas, Rita Belén 
dc.contributor.authorDiego Rodríguez, José María 
dc.contributor.authorHerranz Muñoz, Diego 
dc.contributor.authorMartínez González, Enrique
dc.contributor.authorVielva Martínez, Patricio 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2022-05-16T15:58:16Z
dc.date.available2022-05-16T15:58:16Z
dc.date.issued2020
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttp://hdl.handle.net/10902/24847
dc.description.abstractWe present a final description of the data-processing pipeline for the Planck Low Frequency Instrument (LFI), implemented for the 2018 data release. Several improvements have been made with respect to the previous release, especially in the calibration process and in the correction of instrumental features such as the effects of nonlinearity in the response of the analogue-to-digital converters. We provide a brief pedagogical introduction to the complete pipeline, as well as a detailed description of the important changes implemented. Self-consistency of the pipeline is demonstrated using dedicated simulations and null tests. We present the final version of the LFI full sky maps at 30, 44, and 70 GHz, both in temperature and polarization, together with a refined estimate of the solar dipole and a final assessment of the main LFI instrumental parameters.es_ES
dc.description.sponsorshipAcknowledgements. The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (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 ERC and PRACE (EU). A description of the Planck Collaboration and a list of its members, indicating which technical or scientific activities they have been involved in, can be found at http://www.cosmos.esa.int/web/planck/. The simulations for systematics assessment used the Extreme Science and Engineering Discovery Environment (XSEDE, Towns et al. 2014), supported by National Science Foundation grant number ACI-1548562, in particular the Comet Supercomputer at the San Diego Supercomputer Center through allocation AST160021: “Monte Carlo simulations for calibration uncertainty of the Planck mission”, PI A. Zonca, CoPI P. Meinhold.es_ES
dc.format.extent33 p.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rights© ESOes_ES
dc.sourceAstronomy & Astrophysics. Vol 641, Sep. 2020. A2es_ES
dc.subject.otherSpace vehicles: instrumentses_ES
dc.subject.otherMethods: data analysises_ES
dc.subject.otherCosmic background radiationes_ES
dc.titlePlanck 2018 results: II. Low Frequency Instrument data processinges_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1051/0004-6361/201833293es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOIhttps://doi.org/10.1051/0004-6361/201833293
dc.type.versionpublishedVersiones_ES


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