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@article{Akrami:2020:0004-6361/201833293,
author = {Akrami, Y and Argueso, F and Ashdown, M and Aumont, J and Baccigalupi, C and Ballardini, M and Banday, AJ and Barreiro, RB and Bartolo, N and Basak, S and Benabed, K and Bernard, J-P and Bersanelli, M and Bielewicz, P and Bonavera, L and Bond, JR and Borrill, J and Bouchet, FR and Boulanger, F and Bucher, M and Burigana, C and Butler, RC and Calabrese, E and Cardoso, J-F and Colombo, LPL and Crill, BP and Cuttaia, F and de, Bernardis P and de, Rosa A and de, Zotti G and Delabrouille, J and Di, Valentino E and Dickinson, C and Diego, JM and Donzelli, S and Ducout, A and Dupac, X and Efstathiou, G and Elsner, F and Ensslin, TA and Eriksen, HK and Fantaye, Y and Finelli, F and Frailis, M and Franceschi, E and Frolov, A and Galeotta, S and Galli, S and Ganga, K and Genova-Santos, RT and Gerbino, M and Ghosh, T and Gonzalez-Nuevo, J and Gorski, KM and Gratton, S and Gruppuso, A and Gudmundsson, JE and Handley, W and Hansen, FK and Herranz, D and Hivon, E and Huang, Z and Jaffe, AH and Jones},
doi = {0004-6361/201833293},
journal = {Astronomy and Astrophysics: a European journal},
title = {Planck 2018 results: II. Low Frequency Instrument data processing},
url = {http://dx.doi.org/10.1051/0004-6361/201833293},
volume = {641},
year = {2020}
}

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TY  - JOUR
AB  - We 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.
AU  - Akrami,Y
AU  - Argueso,F
AU  - Ashdown,M
AU  - Aumont,J
AU  - Baccigalupi,C
AU  - Ballardini,M
AU  - Banday,AJ
AU  - Barreiro,RB
AU  - Bartolo,N
AU  - Basak,S
AU  - Benabed,K
AU  - Bernard,J-P
AU  - Bersanelli,M
AU  - Bielewicz,P
AU  - Bonavera,L
AU  - Bond,JR
AU  - Borrill,J
AU  - Bouchet,FR
AU  - Boulanger,F
AU  - Bucher,M
AU  - Burigana,C
AU  - Butler,RC
AU  - Calabrese,E
AU  - Cardoso,J-F
AU  - Colombo,LPL
AU  - Crill,BP
AU  - Cuttaia,F
AU  - de,Bernardis P
AU  - de,Rosa A
AU  - de,Zotti G
AU  - Delabrouille,J
AU  - Di,Valentino E
AU  - Dickinson,C
AU  - Diego,JM
AU  - Donzelli,S
AU  - Ducout,A
AU  - Dupac,X
AU  - Efstathiou,G
AU  - Elsner,F
AU  - Ensslin,TA
AU  - Eriksen,HK
AU  - Fantaye,Y
AU  - Finelli,F
AU  - Frailis,M
AU  - Franceschi,E
AU  - Frolov,A
AU  - Galeotta,S
AU  - Galli,S
AU  - Ganga,K
AU  - Genova-Santos,RT
AU  - Gerbino,M
AU  - Ghosh,T
AU  - Gonzalez-Nuevo,J
AU  - Gorski,KM
AU  - Gratton,S
AU  - Gruppuso,A
AU  - Gudmundsson,JE
AU  - Handley,W
AU  - Hansen,FK
AU  - Herranz,D
AU  - Hivon,E
AU  - Huang,Z
AU  - Jaffe,AH
AU  - Jones,WC
AU  - Karakci,A
AU  - Keihanen,E
AU  - Keskitalo,R
AU  - Kiiveri,K
AU  - Kim,J
AU  - Kisner,TS
AU  - Krachmalnicoff,N
AU  - Kunz,M
AU  - Kurki-Suonio,H
AU  - Lamarre,J-M
AU  - Lasenby,A
AU  - Lattanzi,M
AU  - Lawrence,CR
AU  - Leahy,JP
AU  - Levrier,F
AU  - Liguori,M
AU  - Lilje,PB
AU  - Lindholm,V
AU  - Lopez-Caniego,M
AU  - Ma,Y-Z
AU  - Macias-Perez,JF
AU  - Maggio,G
AU  - Maino,D
AU  - Mandolesi,N
AU  - Mangilli,A
AU  - Maris,M
AU  - Martin,PG
AU  - Martinez-Gonzalez,E
AU  - Matarrese,S
AU  - Mauri,N
AU  - McEwen,JD
AU  - Meinhold,PR
AU  - Melchiorri,A
AU  - Mennella,A
AU  - Migliaccio,M
AU  - Molinari,D
AU  - Montier,L
AU  - Morgante,G
AU  - Moss,A
AU  - Natoli,P
AU  - Pagano,L
AU  - Paoletti,D
AU  - Partridge,B
AU  - Patanchon,G
AU  - Patrizii,L
AU  - Peel,M
AU  - Perrotta,F
AU  - Pettorino,V
AU  - Piacentini,F
AU  - Polenta,G
AU  - Puget,J-L
AU  - Rachen,JP
AU  - Racine,B
AU  - Reinecke,M
AU  - Remazeilles,M
AU  - Renzi,A
AU  - Rocha,G
AU  - Roudier,G
AU  - Rubino-Martin,JA
AU  - Salvati,L
AU  - Sandri,M
AU  - Savelainen,M
AU  - Scott,D
AU  - Seljebotn,DS
AU  - Sirignano,C
AU  - Sirri,G
AU  - Spencer,LD
AU  - Suur-Uski,A-S
AU  - Tauber,JA
AU  - Tavagnacco,D
AU  - Tenti,M
AU  - Terenzi,L
AU  - Toffolatti,L
AU  - Tomasi,M
AU  - Trombetti,T
AU  - Valiviita,J
AU  - Vansyngel,F
AU  - Van,Tent B
AU  - Vielva,P
AU  - Villa,F
AU  - Vittorio,N
AU  - Wandelt,BD
AU  - Watson,R
AU  - Wehus,IK
AU  - Zacchei,A
AU  - Zonca,A
DO  - 0004-6361/201833293
PY  - 2020///
SN  - 0004-6361
TI  - Planck 2018 results: II. Low Frequency Instrument data processing
T2  - Astronomy and Astrophysics: a European journal
UR  - http://dx.doi.org/10.1051/0004-6361/201833293
UR  - https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000571763700002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=a2bf6146997ec60c407a63945d4e92bb
UR  - https://www.aanda.org/articles/aa/full_html/2020/09/aa33293-18/aa33293-18.html
UR  - http://hdl.handle.net/10044/1/107606
VL  - 641
ER  -

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Professor Andrew H Jaffe

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