Abstract
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.
| Original language | English (US) |
|---|---|
| Article number | A2 |
| Journal | Astronomy and Astrophysics |
| Volume | 641 |
| DOIs | |
| State | Published - Sep 1 2020 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Cosmic background radiation
- Methods: data analysis
- Space vehicles: instruments
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Planck 2018 results : II. Low Frequency Instrument data processing. / Akrami, Y.; Argüeso, F.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Ballardini, M.; Banday, A. J.; Barreiro, R. B.; Bartolo, N.; Basak, S.; Benabed, K.; Bernard, J. P.; Bersanelli, M.; Bielewicz, P.; Bonavera, L.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bucher, M.; Burigana, C.; Butler, R. C.; Calabrese, E.; Cardoso, J. F.; Colombo, L. P.L.; Crill, B. P.; Cuttaia, F.; De Bernardis, P.; De Rosa, A.; De Zotti, G.; Delabrouille, J.; Di Valentino, E.; Dickinson, C.; Diego, J. M.; Donzelli, S.; Ducout, A.; Dupac, X.; Efstathiou, G.; Elsner, F.; Enßlin, T. A.; Eriksen, H. K.; Fantaye, Y.; Finelli, F.; Frailis, M.; Franceschi, E.; Frolov, A.; Galeotta, S.; Galli, S.; Ganga, K.; Génova-Santos, R. T.; Gerbino, M.; Ghosh, T.; González-Nuevo, J.; Górski, K. M.; Gratton, S.; Gruppuso, A.; Gudmundsson, J. E.; Handley, W.; Hansen, F. K.; Herranz, D.; Hivon, E.; Huang, Z.; Jaffe, A. H.; Jones, W. C.; Karakci, A.; Keihänen, E.; Keskitalo, R.; Kiiveri, K.; Kim, J.; Kisner, T. S.; Krachmalnicoff, N.; Kunz, M.; Kurki-Suonio, H.; Lamarre, J. M.; Lasenby, A.; Lattanzi, M.; Lawrence, C. R.; Leahy, J. P.; Levrier, F.; Liguori, M.; Lilje, P. B.; Lindholm, V.; López-Caniego, M.; Ma, Y. Z.; Maciás-Pérez, J. F.; Maggio, G.; Maino, D.; Mandolesi, N.; Mangilli, A.; Maris, M.; Martin, P. G.; Martínez-González, E.; Matarrese, S.; Mauri, N.; McEwen, J. D.; Meinhold, P. R.; Melchiorri, A.; Mennella, A.; Migliaccio, M.; Molinari, D.; Montier, L.; Morgante, G.; Moss, A.; Natoli, P.; Pagano, L.; Paoletti, D.; Partridge, B.; Patanchon, G.; Patrizii, L.; Peel, M.; Perrotta, F.; Pettorino, V.; Piacentini, F.; Polenta, G.; Puget, J. L.; Rachen, J. P.; Racine, B.; Reinecke, M.; Remazeilles, M.; Renzi, A.; Rocha, G.; Roudier, G.; Rubiño-Martín, J. A.; Salvati, L.; Sandri, M.; Savelainen, M.; Scott, D.; Seljebotn, D. S.; Sirignano, C.; Sirri, G.; Spencer, L. D.; Suur-Uski, A. S.; Tauber, J. A.; Tavagnacco, D.; Tenti, M.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Trombetti, T.; Valiviita, J.; Vansyngel, F.; Van Tent, B.; Vielva, P.; Villa, F.; Vittorio, N.; Wandelt, B. D.; Watson, R.; Wehus, I. K.; Zacchei, A.; Zonca, A.
In: Astronomy and Astrophysics, Vol. 641, A2, 01.09.2020.Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - Planck 2018 results
T2 - II. Low Frequency Instrument data processing
AU - Akrami, Y.
AU - Argüeso, F.
AU - Ashdown, M.
AU - Aumont, J.
AU - Baccigalupi, C.
AU - Ballardini, M.
AU - Banday, A. J.
AU - Barreiro, R. B.
AU - Bartolo, N.
AU - Basak, S.
AU - Benabed, K.
AU - Bernard, J. P.
AU - Bersanelli, M.
AU - Bielewicz, P.
AU - Bonavera, L.
AU - Bond, J. R.
AU - Borrill, J.
AU - Bouchet, F. R.
AU - Boulanger, F.
AU - Bucher, M.
AU - Burigana, C.
AU - Butler, R. C.
AU - Calabrese, E.
AU - Cardoso, J. F.
AU - Colombo, L. P.L.
AU - Crill, B. P.
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, J. M.
AU - Donzelli, S.
AU - Ducout, A.
AU - Dupac, X.
AU - Efstathiou, G.
AU - Elsner, F.
AU - Enßlin, T. A.
AU - Eriksen, H. K.
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 - Génova-Santos, R. T.
AU - Gerbino, M.
AU - Ghosh, T.
AU - González-Nuevo, J.
AU - Górski, K. M.
AU - Gratton, S.
AU - Gruppuso, A.
AU - Gudmundsson, J. E.
AU - Handley, W.
AU - Hansen, F. K.
AU - Herranz, D.
AU - Hivon, E.
AU - Huang, Z.
AU - Jaffe, A. H.
AU - Jones, W. C.
AU - Karakci, A.
AU - Keihänen, E.
AU - Keskitalo, R.
AU - Kiiveri, K.
AU - Kim, J.
AU - Kisner, T. S.
AU - Krachmalnicoff, N.
AU - Kunz, M.
AU - Kurki-Suonio, H.
AU - Lamarre, J. M.
AU - Lasenby, A.
AU - Lattanzi, M.
AU - Lawrence, C. R.
AU - Leahy, J. P.
AU - Levrier, F.
AU - Liguori, M.
AU - Lilje, P. B.
AU - Lindholm, V.
AU - López-Caniego, M.
AU - Ma, Y. Z.
AU - Maciás-Pérez, J. F.
AU - Maggio, G.
AU - Maino, D.
AU - Mandolesi, N.
AU - Mangilli, A.
AU - Maris, M.
AU - Martin, P. G.
AU - Martínez-González, E.
AU - Matarrese, S.
AU - Mauri, N.
AU - McEwen, J. D.
AU - Meinhold, P. R.
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, J. P.
AU - Racine, B.
AU - Reinecke, M.
AU - Remazeilles, M.
AU - Renzi, A.
AU - Rocha, G.
AU - Roudier, G.
AU - Rubiño-Martín, J. A.
AU - Salvati, L.
AU - Sandri, M.
AU - Savelainen, M.
AU - Scott, D.
AU - Seljebotn, D. S.
AU - Sirignano, C.
AU - Sirri, G.
AU - Spencer, L. D.
AU - Suur-Uski, A. S.
AU - Tauber, J. A.
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, B. D.
AU - Watson, R.
AU - Wehus, I. K.
AU - Zacchei, A.
AU - Zonca, A.
N1 - Funding Information: Acknowledgements. 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. Funding Information: ★ Corresponding author: D. Maino, e-mail: davide.maino@mi.infn.it 1 Planck (http://www.esa.int/Planck) is a project of the European Space Agency (ESA) with instruments provided by two scientific consortia funded by ESA member states and let by Principal Investigators from France and Italy, telescope reflectors provided through a collaboration between ESA and a scientific consortium led and funded by Denmark, and additional contributions from NASA (USA). Publisher Copyright: © ESO 2020.
PY - 2020/9/1
Y1 - 2020/9/1
N2 - 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.
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.
KW - Cosmic background radiation
KW - Methods: data analysis
KW - Space vehicles: instruments
UR - http://www.scopus.com/inward/record.url?scp=85091910244&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85091910244&partnerID=8YFLogxK
U2 - 10.1051/0004-6361/201833293
DO - 10.1051/0004-6361/201833293
M3 - Article
AN - SCOPUS:85091910244
VL - 641
JO - Astronomy and Astrophysics
JF - Astronomy and Astrophysics
SN - 0004-6361
M1 - A2
ER -