Planck 2018 results: II. Low Frequency Instrument data processing

Y. Akrami; F. Argüeso; M. Ashdown; J. Aumont; C. Baccigalupi; M. Ballardini; A. J. Banday; R. B. Barreiro; N. Bartolo; S. Basak; K. Benabed; J. P. Bernard; M. Bersanelli; P. Bielewicz; L. Bonavera; J. R. Bond; J. Borrill; F. R. Bouchet; F. Boulanger; M. Bucher; C. Burigana; R. C. Butler; E. Calabrese; J. F. Cardoso; L. P.L. Colombo; B. P. Crill; F. Cuttaia; P. De Bernardis; A. De Rosa; G. De Zotti; J. Delabrouille; E. Di Valentino; C. Dickinson; J. M. Diego; S. Donzelli; A. Ducout; X. Dupac; G. Efstathiou; F. Elsner; T. A. Enßlin; H. K. Eriksen; Y. Fantaye; F. Finelli; M. Frailis; E. Franceschi; A. Frolov; S. Galeotta; S. Galli; K. Ganga; R. T. Génova-Santos; M. Gerbino; T. Ghosh; J. González-Nuevo; K. M. Górski; S. Gratton; A. Gruppuso; J. E. Gudmundsson; W. Handley; F. K. Hansen; D. Herranz; E. Hivon; Z. Huang; A. H. Jaffe; W. C. Jones; A. Karakci; E. Keihänen; R. Keskitalo; K. Kiiveri; J. Kim; T. S. Kisner; N. Krachmalnicoff; M. Kunz; H. Kurki-Suonio; J. M. Lamarre; A. Lasenby; M. Lattanzi; C. R. Lawrence; J. P. Leahy; F. Levrier; M. Liguori; P. B. Lilje; V. Lindholm; M. López-Caniego; Y. Z. Ma; J. F. Maciás-Pérez; G. Maggio; D. Maino; N. Mandolesi; A. Mangilli; M. Maris; P. G. Martin; E. Martínez-González; S. Matarrese; N. Mauri; J. D. McEwen; P. R. Meinhold; A. Melchiorri; A. Mennella; M. Migliaccio; D. Molinari; L. Montier; G. Morgante; A. Moss; P. Natoli; L. Pagano; D. Paoletti; B. Partridge; G. Patanchon; L. Patrizii; M. Peel; F. Perrotta; V. Pettorino; F. Piacentini; G. Polenta; J. L. Puget; J. P. Rachen; B. Racine; M. Reinecke; M. Remazeilles; A. Renzi; G. Rocha; G. Roudier; J. A. Rubiño-Martín; L. Salvati; M. Sandri; M. Savelainen; D. Scott; D. S. Seljebotn; C. Sirignano; G. Sirri; L. D. Spencer; A. S. Suur-Uski; J. A. Tauber; D. Tavagnacco; M. Tenti; L. Terenzi; L. Toffolatti; M. Tomasi; T. Trombetti; J. Valiviita; F. Vansyngel; B. Van Tent; P. Vielva; F. Villa; N. Vittorio; B. D. Wandelt; R. Watson; I. K. Wehus; A. Zacchei; A. Zonca

doi:10.1051/0004-6361/201833293

Planck 2018 results: II. Low Frequency Instrument data processing

Y. Akrami, F. Argüeso, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, R. B. Barreiro, N. Bartolo, S. Basak, K. Benabed, J. P. Bernard, M. Bersanelli, P. Bielewicz, L. Bonavera, J. R. Bond, J. Borrill, F. R. Bouchet, F. Boulanger, M. BucherC. Burigana, R. C. Butler, E. Calabrese, J. F. Cardoso, L. P.L. Colombo, B. P. Crill, F. Cuttaia, P. De Bernardis, A. De Rosa, G. De Zotti, J. Delabrouille, E. Di Valentino, C. Dickinson, J. M. Diego, S. Donzelli, A. Ducout, X. Dupac, G. Efstathiou, F. Elsner, T. A. Enßlin, H. K. Eriksen, Y. Fantaye, F. Finelli, M. Frailis, E. Franceschi, A. Frolov, S. Galeotta, S. Galli, K. Ganga, R. T. Génova-Santos, M. Gerbino, T. Ghosh, J. González-Nuevo, K. M. Górski, S. Gratton, A. Gruppuso, J. E. Gudmundsson, W. Handley, F. K. Hansen, D. Herranz, E. Hivon, Z. Huang, A. H. Jaffe, W. C. Jones, A. Karakci, E. Keihänen, R. Keskitalo, K. Kiiveri, J. Kim, T. S. Kisner, N. Krachmalnicoff, M. Kunz, H. Kurki-Suonio, J. M. Lamarre, A. Lasenby, M. Lattanzi, C. R. Lawrence, J. P. Leahy, F. Levrier, M. Liguori, P. B. Lilje, V. Lindholm, M. López-Caniego, Y. Z. Ma, J. F. Maciás-Pérez, G. Maggio, D. Maino, N. Mandolesi, A. Mangilli, M. Maris, P. G. Martin, E. Martínez-González, S. Matarrese, N. Mauri, J. D. McEwen, P. R. Meinhold, A. Melchiorri, A. Mennella, M. Migliaccio, D. Molinari, L. Montier, G. Morgante, A. Moss, P. Natoli, L. Pagano, D. Paoletti, B. Partridge, G. Patanchon, L. Patrizii, M. Peel, F. Perrotta, V. Pettorino, F. Piacentini, G. Polenta, J. L. Puget, J. P. Rachen, B. Racine, M. Reinecke, M. Remazeilles, A. Renzi, G. Rocha, G. Roudier, J. A. Rubiño-Martín, L. Salvati, M. Sandri, M. Savelainen, D. Scott, D. S. Seljebotn, C. Sirignano, G. Sirri, L. D. Spencer, A. S. Suur-Uski, J. A. Tauber, D. Tavagnacco, M. Tenti, L. Terenzi, L. Toffolatti, M. Tomasi, T. Trombetti, J. Valiviita, F. Vansyngel, B. Van Tent, P. Vielva, F. Villa, N. Vittorio, B. D. Wandelt, R. Watson, I. K. Wehus, A. Zacchei, A. Zonca

Physics

Research output: Contribution to journal › Article › peer-review

21 Scopus citations

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	https://doi.org/10.1051/0004-6361/201833293
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

Access to Document

10.1051/0004-6361/201833293

Cite this

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., ... Zonca, A. (2020). Planck 2018 results: II. Low Frequency Instrument data processing. Astronomy and Astrophysics, 641, Article A2. https://doi.org/10.1051/0004-6361/201833293

@article{437ab31ba76040129e256d314f70fcd8,

title = "Planck 2018 results: II. Low Frequency Instrument data processing",

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.",

keywords = "Cosmic background radiation, Methods: data analysis, Space vehicles: instruments",

author = "Y. Akrami and F. Arg{\"u}eso and M. Ashdown and J. Aumont and C. Baccigalupi and M. Ballardini and Banday, {A. J.} and Barreiro, {R. B.} and N. Bartolo and S. Basak and K. Benabed and Bernard, {J. P.} and M. Bersanelli and P. Bielewicz and L. Bonavera and Bond, {J. R.} and J. Borrill and Bouchet, {F. R.} and F. Boulanger and M. Bucher and C. Burigana and Butler, {R. C.} and E. Calabrese and Cardoso, {J. F.} and Colombo, {L. P.L.} and Crill, {B. P.} and F. Cuttaia and {De Bernardis}, P. and {De Rosa}, A. and {De Zotti}, G. and J. Delabrouille and {Di Valentino}, E. and C. Dickinson and Diego, {J. M.} and S. Donzelli and A. Ducout and X. Dupac and G. Efstathiou and F. Elsner and En{\ss}lin, {T. A.} and Eriksen, {H. K.} and Y. Fantaye and F. Finelli and M. Frailis and E. Franceschi and A. Frolov and S. Galeotta and S. Galli and K. Ganga and G{\'e}nova-Santos, {R. T.} and M. Gerbino and T. Ghosh and J. Gonz{\'a}lez-Nuevo and G{\'o}rski, {K. M.} and S. Gratton and A. Gruppuso and Gudmundsson, {J. E.} and W. Handley and Hansen, {F. K.} and D. Herranz and E. Hivon and Z. Huang and Jaffe, {A. H.} and Jones, {W. C.} and A. Karakci and E. Keih{\"a}nen and R. Keskitalo and K. Kiiveri and J. Kim and Kisner, {T. S.} and N. Krachmalnicoff and M. Kunz and H. Kurki-Suonio and Lamarre, {J. M.} and A. Lasenby and M. Lattanzi and Lawrence, {C. R.} and Leahy, {J. P.} and F. Levrier and M. Liguori and Lilje, {P. B.} and V. Lindholm and M. L{\'o}pez-Caniego and Ma, {Y. Z.} and Maci{\'a}s-P{\'e}rez, {J. F.} and G. Maggio and D. Maino and N. Mandolesi and A. Mangilli and M. Maris and Martin, {P. G.} and E. Mart{\'i}nez-Gonz{\'a}lez and S. Matarrese and N. Mauri and McEwen, {J. D.} and Meinhold, {P. R.} and A. Melchiorri and A. Mennella and M. Migliaccio and D. Molinari and L. Montier and G. Morgante and A. Moss and P. Natoli and L. Pagano and D. Paoletti and B. Partridge and G. Patanchon and L. Patrizii and M. Peel and F. Perrotta and V. Pettorino and F. Piacentini and G. Polenta and Puget, {J. L.} and Rachen, {J. P.} and B. Racine and M. Reinecke and M. Remazeilles and A. Renzi and G. Rocha and G. Roudier and Rubi{\~n}o-Mart{\'i}n, {J. A.} and L. Salvati and M. Sandri and M. Savelainen and D. Scott and Seljebotn, {D. S.} and C. Sirignano and G. Sirri and Spencer, {L. D.} and Suur-Uski, {A. S.} and Tauber, {J. A.} and D. Tavagnacco and M. Tenti and L. Terenzi and L. Toffolatti and M. Tomasi and T. Trombetti and J. Valiviita and F. Vansyngel and {Van Tent}, B. and P. Vielva and F. Villa and N. Vittorio and Wandelt, {B. D.} and R. Watson and Wehus, {I. K.} and A. Zacchei and A. Zonca",

note = "Publisher Copyright: {\textcopyright} ESO 2020.",

year = "2020",

month = sep,

day = "1",

doi = "10.1051/0004-6361/201833293",

language = "English (US)",

volume = "641",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

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Akrami, Y, Argüeso, F, Ashdown, M, Aumont, J, Baccigalupi, C, Ballardini, M, Banday, AJ, Barreiro, RB, Bartolo, N, Basak, S, Benabed, K, Bernard, JP, Bersanelli, M, Bielewicz, P, Bonavera, L, Bond, JR, Borrill, J, Bouchet, FR, Boulanger, F, Bucher, M, Burigana, C, Butler, RC, Calabrese, E, Cardoso, JF, Colombo, LPL, Crill, BP, Cuttaia, F, De Bernardis, P, De Rosa, A, De Zotti, G, Delabrouille, J, Di Valentino, E, Dickinson, C, Diego, JM, Donzelli, S, Ducout, A, Dupac, X, Efstathiou, G, Elsner, F, Enßlin, TA, Eriksen, HK, Fantaye, Y, Finelli, F, Frailis, M, Franceschi, E, Frolov, A, Galeotta, S, Galli, S, Ganga, K, Génova-Santos, RT, Gerbino, M, Ghosh, T, González-Nuevo, J, Górski, KM, Gratton, S, Gruppuso, A, Gudmundsson, JE, Handley, W, Hansen, FK, Herranz, D, Hivon, E, Huang, Z, Jaffe, AH, Jones, WC, Karakci, A, Keihänen, E, Keskitalo, R, Kiiveri, K, Kim, J, Kisner, TS, Krachmalnicoff, N, Kunz, M, Kurki-Suonio, H, Lamarre, JM, Lasenby, A, Lattanzi, M, Lawrence, CR, Leahy, JP, Levrier, F, Liguori, M, Lilje, PB, Lindholm, V, López-Caniego, M, Ma, YZ, Maciás-Pérez, JF, Maggio, G, Maino, D, Mandolesi, N, Mangilli, A, Maris, M, Martin, PG, Martínez-González, E, Matarrese, S, Mauri, N, McEwen, JD, Meinhold, PR, 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, JL, Rachen, JP, Racine, B, Reinecke, M, Remazeilles, M, Renzi, A, Rocha, G, Roudier, G, Rubiño-Martín, JA, Salvati, L, Sandri, M, Savelainen, M, Scott, D, Seljebotn, DS, Sirignano, C, Sirri, G, Spencer, LD, Suur-Uski, AS, Tauber, JA, 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, BD, Watson, R, Wehus, IK, Zacchei, A & Zonca, A 2020, 'Planck 2018 results: II. Low Frequency Instrument data processing', Astronomy and Astrophysics, vol. 641, A2. https://doi.org/10.1051/0004-6361/201833293

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.

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

SN - 0004-6361

VL - 641

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A2

ER -

Planck 2018 results: II. Low Frequency Instrument data processing

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