Planck 2015 results. VII. High Frequency Instrument data processing: Time-ordered information and beams
Journal
Date Issued
2016
Author(s)
Planck Collaboration
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Adam, R.
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Ade, P. A. R.
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Aghanim, N.
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Arnaud, M.
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Ashdown, M.
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Aumont, J.
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Baccigalupi, C.
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Banday, A. J.
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Barreiro, R. B.
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Bartolo, N.
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Battaner, E.
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Benabed, K.
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Benoît, A.
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Benoit-Lévy, A.
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Bernard, J. -P.
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Bersanelli, M.
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Bertincourt, B.
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Bielewicz, P.
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Bock, J. J.
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Bonavera, L.
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Bond, J. R.
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Borrill, J.
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Bouchet, F. R.
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Boulanger, F.
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Bucher, M.
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Calabrese, E.
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Cardoso, J. -F.
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Catalano, A.
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Challinor, A.
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Chamballu, A.
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Chary, R. -R.
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Chiang, H. C.
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Christensen, P. R.
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Clements, D. L.
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Colombi, S.
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Colombo, L. P. L.
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Combet, C.
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Couchot, F.
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Coulais, A.
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Crill, B. P.
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Curto, A.
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Danese, L.
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Davies, R. D.
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Davis, R. J.
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de Bernardis, P.
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de Zotti, G.
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Delabrouille, J.
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Delouis, J. -M.
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Désert, F. -X.
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Diego, J. M.
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Dole, H.
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Donzelli, S.
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Doré, O.
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Douspis, M.
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Ducout, A.
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Dupac, X.
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Efstathiou, G.
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Elsner, F.
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Enßlin, T. A.
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Eriksen, H. K.
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Falgarone, E.
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Fergusson, J.
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Forni, O.
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Fraisse, A. A.
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Frejsel, A.
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Galli, S.
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Ganga, K.
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Ghosh, T.
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Giard, M.
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Giraud-Héraud, Y.
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Gjerløw, E.
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González-Nuevo, J.
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Górski, K. M.
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Gratton, S.
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Gudmundsson, J. E.
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Hansen, F. K.
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Hanson, D.
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Harrison, D. L.
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Henrot-Versillé, S.
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Herranz, D.
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Hildebrandt, S. R.
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Hivon, E.
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Hobson, M.
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Holmes, W. A.
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Hornstrup, A.
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Hovest, W.
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Huffenberger, K. M.
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Hurier, G.
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Jaffe, A. H.
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Jaffe, T. R.
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Jones, W. C.
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Juvela, M.
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Keihänen, E.
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Keskitalo, R.
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Kisner, T. S.
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Kneissl, R.
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Knoche, J.
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Kunz, M.
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Kurki-Suonio, H.
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Lagache, G.
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Lamarre, J. -M.
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Lasenby, A.
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Lattanzi, M.
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Lawrence, C. R.
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Le Jeune, M.
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Leahy, J. P.
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Lellouch, E.
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Leonardi, R.
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Lesgourgues, J.
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Levrier, F.
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Liguori, M.
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Lilje, P. B.
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Linden-Vørnle, M.
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López-Caniego, M.
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Lubin, P. M.
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Macías-Pérez, J. F.
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Maino, D.
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Mandolesi, N.
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Mangilli, A.
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Martin, P. G.
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Martínez-González, E.
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Masi, S.
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Matarrese, S.
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McGehee, P.
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Melchiorri, A.
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Mendes, L.
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Mennella, A.
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Migliaccio, M.
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Mitra, S.
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Miville-Deschênes, M. -A.
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Moneti, A.
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Montier, L.
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Moreno, R.
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Mortlock, D.
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Moss, A.
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Mottet, S.
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Munshi, D.
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Murphy, J. A.
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Naselsky, P.
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Nati, F.
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Natoli, P.
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Netterfield, C. B.
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Nørgaard-Nielsen, H. U.
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Noviello, F.
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Novikov, D.
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Novikov, I.
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Oxborrow, C. A.
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Paci, F.
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Pagano, L.
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Pajot, F.
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Pasian, F.
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Patanchon, G.
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Pearson, T. J.
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Perdereau, O.
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Perotto, L.
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Perrotta, F.
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Pettorino, V.
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Piacentini, F.
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Piat, M.
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Pierpaoli, E.
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Pietrobon, D.
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Plaszczynski, S.
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Pointecouteau, E.
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Polenta, G.
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Pratt, G. W.
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Prézeau, G.
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Prunet, S.
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Puget, J. -L.
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Rachen, J. P.
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Reinecke, M.
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Remazeilles, M.
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Renault, C.
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Renzi, A.
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Ristorcelli, I.
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Rocha, G.
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Rosset, C.
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Roudier, G.
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Rowan-Robinson, M.
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Rusholme, B.
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Santos, D.
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Sauvé, A.
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Savelainen, M.
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Savini, G.
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Scott, D.
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Seiffert, M. D.
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Shellard, E. P. S.
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Spencer, L. D.
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Stolyarov, V.
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Stompor, R.
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Sudiwala, R.
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Sutton, D.
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Suur-Uski, A. -S.
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Sygnet, J. -F.
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Tauber, J. A.
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Toffolatti, L.
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Tomasi, M.
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Tristram, M.
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Tucci, M.
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Tuovinen, J.
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Valiviita, J.
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Van Tent, B.
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Vibert, L.
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Vielva, P.
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Wade, L. A.
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Wandelt, B. D.
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Watson, R.
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Wehus, I. K.
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Yvon, D.
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Zonca, A.
Abstract
The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polarization (100, 143, 217, and 353 GHz). In order to obtain sky maps, the time-ordered information (TOI) containing the detector and pointing samples must be processed and the angular response must be assessed. The full mission TOI is included in the Planck 2015 release. This paper describes the HFI TOI and beam processing for the 2015 release. HFI calibration and map making are described in a companion paper. The main pipeline has been modified since the last release (2013 nominal mission in intensity only), by including a correction for the nonlinearity of the warm readout and by improving the model of the bolometer time response. The beam processing is an essential tool that derives the angular response used in all the Planck science papers and we report an improvement in the effective beam window function uncertainty of more than a factor of 10 relative to the2013 release. Noise correlations introduced by pipeline filtering function are assessed using dedicated simulations. Angular cross-power spectra using data sets that are decorrelated in time are immune to the main systematic effects.
Volume
594
Start page
A7
Issn Identifier
0004-6361
Ads BibCode
2016A&A...594A...7P
Rights
open.access
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