We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our results and methods have remained unchanged since the 2013 paper and we highlight the changes made for the 2015 release, describing the products (especially timelines) and the ways in which they were obtained. We demonstrate that the pipeline is self-consistent (principally based on simulations) and report all null tests. For the first time, we present LFI maps in Stokes Q and U polarization. We refer to other related papers where more detailed descriptions of the LFI data processing pipeline may be found if needed.
Planck 2015 results. II. Low Frequency Instrument data processing / R.B. Barreiro, N. Bartolo, S. Basak, P. Battaglia, E. Battaner, K. Benabed, A. Benôıt, A. Benoit-L´evy, J.P. Bernard, M. Bersanelli, P. Bielewicz, J.J. Bock, A. Bonaldi, L. Bonavera, J.R. Bond, J. Borrill, F.R. Bouchet, M. Bucher, C. Burigana, R.C. Butler, E. Calabrese, J.F. Cardoso, G. Castex, A. Catalano, A. Chamballu, P.R. Christensen, S. Colombi, L.P.L. Colombo, B.P. Crill, A. Curto, F. Cuttaia, L. Danese, R.D. Davies, R.J. Davis, P. de Bernardis, A. de Rosa, G. de Zotti, J. Delabrouille, C. Dickinson, J.M. Diego, H. Dole, S. Donzelli, O. Dor´e, M. Douspis, A. Ducout, X. Dupac, G. Efstathiou, F. Elsner, T.A. Enßlin, H.K. Eriksen, J. Fergusson, F. Finelli, O. Forni, M. Frailis, C. Franceschet, E. Franceschi, A. Frejsel, S. Galeotta, S. Galli, K. Ganga, M. Giard, Y. Giraud-Héraud, E. Gjerløw, J. González-Nuevo, K.M. Górski, S. Gratton, A. Gregorio, A. Gruppuso, F.K. Hansen, D. Hanson, D.L. Harrison, S. Henrot-Versill´e, D. Herranz, S.R. Hildebrandt, E. Hivon, M. Hobson, W.A. Holmes, A. Hornstrup, W. Hovest, K.M. Huffenberger, G. Hurier, A.H. Jaffe, T.R. Jaffe, M. Juvela, E. Keihänen, R. Keskitalo, K. Kiiveri, T.S. Kisner, J. Knoche, N. Krachmalnico, M. Kunz, H. Kurki-Suonio, G. Lagache, A. Lähteenmäki, J.M. Lamarre, A. Lasenby, M. Lattanzi, C.R. Lawrence, J.P. Leahy, R. Leonardi, J. Lesgourgues, F. Levrier, M. Liguori, P.B. Lilje, M. Linden-Vørnle, V. Lindholm, M. Lopez-Caniego, P.M. Lubin, J.F. Macías-Pérez, G. Maggio, D. Maino, N. Mandolesi, A. Mangilli, M. Maris, P.G. Martin, E. Martínez-González, S. Masi, S. Matarrese, P. Mazzotta, P. McGehee, P.R. Meinhold, A. Melchiorri, L. Mendes, A. Mennella, M. Migliaccio, S. Mitra, L. Montier, G. Morgante, N. Morisset, D. Mortlock, A. Moss, D. Munshi, J.A. Murphy, P. Naselsky, F. Nati, P. Natoli, C.B. Netterfield, H.U. Nørgaard-Nielsen, D. Novikov, I. Novikov, N. Oppermann, F. Paci, L. Pagano, D. Paoletti, B. Partridge, F. Pasian, G. Patanchon, T.J. Pearson, M. Peel, O. Perdereau, L. Perotto, F. Perrotta, V. Pettorino, F. Piacentini, E. Pierpaoli, D. Pietrobon, E. Pointecouteau, G. Polenta, G.W. Pratt, G. Préezeau, S. Prunet, J.L. Puget, J.P. Rachen, R. Rebolo, M. Reinecke, M. Remazeilles, A. Renzi, G. Rocha, E. Romelli, C. Rosset, M. Rossetti, G. Roudier, J.A. Rubiño-Martín, B. Rusholme, M. Sandri, D. Santos, M. Savelainen, D. Scott, M.D. Seiffert, E.P.S. Shellard, L.D. Spencer, V. Stolyarov, D. Sutton, A.S. Suur-Uski, J.F. Sygnet, J.A. Tauber, D. Tavagnacco, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tristram, M. Tucci, J. Tuovinen, M. Tűrler, G. Umana, L. Valenziano, J. Valiviita, B. Van Tent, T. Vassallo, P. Vielva, F. Villa, L.A. Wade, B.D. Wandelt, R. Watson, I.K. Wehus, A. Wilkinson, D. Yvon, A. Zacchei, A. Zonca. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 1432-0746. - 594(2016 Oct).
Planck 2015 results. II. Low Frequency Instrument data processing
M. BersanelliPrimo
;L.P.L. Colombo;C. Franceschet;D. MainoSecondo
;A. MennellaPenultimo
;M. TomasiUltimo
;
2016
Abstract
We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our results and methods have remained unchanged since the 2013 paper and we highlight the changes made for the 2015 release, describing the products (especially timelines) and the ways in which they were obtained. We demonstrate that the pipeline is self-consistent (principally based on simulations) and report all null tests. For the first time, we present LFI maps in Stokes Q and U polarization. We refer to other related papers where more detailed descriptions of the LFI data processing pipeline may be found if needed.
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