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dc.contributor.authorAkrami, Yashar
dc.contributor.authorArgüeso, Francisco
dc.contributor.authorAshdown, Mark A.J.
dc.date.accessioned2020-11-06T10:57:33Z
dc.date.available2020-11-06T10:57:33Z
dc.date.issued2020
dc.identifier.citationAkrami, Y. et al. (2020). Planck 2018 results: II. low frequency Instrument data processing.Astronomy and Astrophysics.461,A2. Doi: https://doi.org/10.1051/0004-6361/201833293en_US
dc.identifier.issn1432-0746
dc.identifier.urihttp://hdl.handle.net/10566/5375
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 parametersen_US
dc.language.isoenen_US
dc.publisherEDP Sciencesen_US
dc.subjectSpace vehiclesen_US
dc.subjectInstrumentsen_US
dc.subjectMethodsen_US
dc.subjectCosmic microwave backgrounden_US
dc.subjectData analysisen_US
dc.titlePlanck 2018 results: II. low frequency Instrument data processingen_US
dc.typeArticleen_US


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