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CERN Accelerating science

Article
Report number arXiv:1502.01586
Title Planck 2015 results. VII. HFI TOI and beam processing
Author(s)

Adam, R. (LPSC, Grenoble) ; Ade, P.A.R. (Cardiff U.) ; Aghanim, N. (Orsay, IAS) ; Arnaud, M. (AIM, Saclay) ; Ashdown, M. (Cambridge U., KICC ; Cambridge U.) ; Aumont, J. (Orsay, IAS) ; Baccigalupi, C. (INFN, Trieste ; SISSA, Trieste) ; Banday, A.J. (IRAP, Toulouse) ; Barreiro, R.B. (Cantabria U., Santander) ; Bartolo, N. (Padua U. ; INFN, Padua) ; Battaner, E. (Granada U., Theor. Phys. Astrophys.) ; Benabed, K. (Paris, Inst. Astrophys.) ; Benoît, A. (Neel Lab, Grenoble) ; Benoit-Lévy, A. (University Coll. London ; Paris, Inst. Astrophys.) ; Bernard, J.-P. (IRAP, Toulouse) ; Bersanelli, M. (Milan U. ; IASF, Milan) ; Bertincourt, B. (Orsay, IAS) ; Bielewicz, P. (Warsaw, Copernicus Astron. Ctr. ; IRAP, Toulouse ; INFN, Trieste ; SISSA, Trieste) ; Bock, J.J. (Caltech, JPL ; Caltech) ; Bonavera, L. (Cantabria U., Santander) ; Bond, J.R. (Canadian Inst. Theor. Astrophys.) ; Borrill, J. (LBL, Berkeley ; UC, Berkeley, Space Sci. Dept.) ; Bouchet, F.R. (Paris, Inst. Astrophys.) ; Boulanger, F. (Orsay, IAS) ; Bucher, M. (APC, Paris) ; Burigana, C. (IASF, Bologna ; Ferrara U. ; INFN, Bologna) ; Calabrese, E. (Oxford U.) ; Cardoso, J.-F. (APC, Paris ; Paris, Inst. Astrophys.) ; Catalano, A. (LPSC, Grenoble ; Paris Observ.) ; Challinor, A. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC ; Cambridge U., DAMTP) ; Chamballu, A. (AIM, Saclay ; IRFU, SPP, Saclay ; Orsay, IAS) ; Chary, R.-R. (Caltech, IPAC) ; Chiang, H.C. (Princeton U. ; KwaZulu Natal U.) ; Christensen, P.R. (Bohr Inst.) ; Clements, D.L. (Imperial Coll., London) ; Colombi, S. (Paris, Inst. Astrophys.) ; Colombo, L.P.L. (Southern California U. ; Caltech, JPL) ; Combet, C. (LPSC, Grenoble) ; Couchot, F. (Orsay, LAL) ; Coulais, A. (Paris Observ.) ; Crill, B.P. (Caltech, JPL ; Caltech) ; Curto, A. (Cantabria U., Santander ; Cambridge U. ; Cambridge U., KICC) ; Cuttaia, F. (IASF, Bologna) ; Danese, L. (INFN, Trieste ; SISSA, Trieste) ; Davies, R.D. (Jodrell Bank) ; Davis, R.J. (Jodrell Bank) ; de Bernardis, P. (Rome U.) ; de Rosa, A. (IASF, Bologna) ; de Zotti, G. (Padua Observ. ; INFN, Trieste ; SISSA, Trieste) ; Delabrouille, J. (APC, Paris) ; Delouis, J.-M. (Paris, Inst. Astrophys.) ; Désert, F.-X. (IPAG) ; Diego, J.M. (Cantabria U., Santander) ; Dole, H. (Orsay, IAS ; IUF, Paris) ; Donzelli, S. (IASF, Milan) ; Doré, O. (Caltech, JPL ; Caltech) ; Douspis, M. (Orsay, IAS) ; Ducout, A. (Paris, Inst. Astrophys. ; Imperial Coll., London) ; Dupac, X. (ESA, Madrid) ; Efstathiou, G. (Cambridge U., Inst. of Astron.) ; Elsner, F. (University Coll. London ; Paris, Inst. Astrophys.) ; Enßlin, T.A. (Garching, Max Planck Inst., MPE) ; Eriksen, H.K. (Inst. Theor. Astrophys., Oslo) ; Falgarone, E. (Paris Observ.) ; Fergusson, J. (Cambridge U., DAMTP) ; Finelli, F. (IASF, Bologna ; INFN, Bologna) ; Forni, O. (IRAP, Toulouse) ; Frailis, M. (Trieste Observ.) ; Fraisse, A.A. (Princeton U.) ; Franceschi, E. (IASF, Bologna) ; Frejsel, A. (Bohr Inst.) ; Galeotta, S. (Trieste Observ.) ; Galli, S. (Chicago U., KICP) ; Ganga, K. (APC, Paris) ; Ghosh, T. (Orsay, IAS) ; Giard, M. (IRAP, Toulouse) ; Giraud-Héraud, Y. (APC, Paris) ; Gjerløw, E. (Inst. Theor. Astrophys., Oslo) ; González-Nuevo, J. (Oviedo U. ; Cantabria U., Santander) ; Górski, K.M. (Caltech, JPL ; Warsaw U. Observ.) ; Gratton, S. (Cambridge U., KICC ; Cambridge U., Inst. of Astron.) ; Gruppuso, A. (IASF, Bologna) ; Gudmundsson, J.E. (Princeton U.) ; Hansen, F.K. (Inst. Theor. Astrophys., Oslo) ; Hanson, D. (McGill U. ; Caltech, JPL ; Canadian Inst. Theor. Astrophys.) ; Harrison, D.L. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Henrot-Versillé, S. (Orsay, LAL) ; Herranz, D. (Cantabria U., Santander) ; Hildebrandt, S.R. (Caltech, JPL ; Caltech) ; Hivon, E. (Paris, Inst. Astrophys.) ; Hobson, M. (Cambridge U.) ; Holmes, W.A. (Caltech, JPL) ; Hornstrup, A. (Denmark, Tech. U.) ; Hovest, W. (Garching, Max Planck Inst., MPE) ; Huffenberger, K.M. (Florida State U.) ; Hurier, G. (Orsay, IAS) ; Jaffe, A.H. (Imperial Coll., London) ; Jaffe, T.R. (IRAP, Toulouse) ; Jones, W.C. (Princeton U.) ; Juvela, M. (Helsinki Inst. of Phys. ; Helsinki U.) ; Keihänen, E. (Helsinki Inst. of Phys. ; Helsinki U.) ; Keskitalo, R. (LBL, Berkeley) ; Kisner, T.S. (LBL, Berkeley) ; Kneissl, R. (European Southern Obs., Chile) ; Knoche, J. (Garching, Max Planck Inst., MPE) ; Kunz, M. (Geneva U., Dept. Theor. Phys. ; Orsay, IAS ; African Inst. Math. Sci., Cape Town) ; Kurki-Suonio, H. (Helsinki Inst. of Phys. ; Helsinki U.) ; Lagache, G. (Marseille, Lab. Astrophys. ; Orsay, IAS) ; Lamarre, J.-M. (Paris Observ.) ; Lasenby, A. (Cambridge U. ; Cambridge U., KICC) ; Lattanzi, M. (Ferrara U.) ; Lawrence, C.R. (Caltech, JPL) ; Le Jeune, M. (APC, Paris) ; Leahy, J.P. (Jodrell Bank) ; Lellouch, E. (Meudon Observ.) ; Leonardi, R. (ESA, Madrid) ; Lesgourgues, J. (Aachen, Tech. Hochsch. ; CERN) ; Levrier, F. (Paris Observ.) ; Liguori, M. (Padua U. ; INFN, Padua) ; Lilje, P.B. (Inst. Theor. Astrophys., Oslo) ; Linden-Vørnle, M. (Denmark, Tech. U.) ; López-Caniego, M. (ESA, Madrid ; Cantabria U., Santander) ; Lubin, P.M. (UC, Santa Barbara) ; Macías-Pérez, J.F. (LPSC, Grenoble) ; Maggio, G. (Trieste Observ.) ; Maino, D. (Milan U. ; IASF, Milan) ; Mandolesi, N. (IASF, Bologna ; Ferrara U.) ; Mangilli, A. (Orsay, IAS ; Orsay, LAL) ; Maris, M. (Trieste Observ.) ; Martin, P.G. (Canadian Inst. Theor. Astrophys.) ; Martínez-González, E. (Cantabria U., Santander) ; Masi, S. (Rome U.) ; Matarrese, S. (Padua U. ; INFN, Padua ; GSSI, Aquila) ; McGehee, P. (Caltech, IPAC) ; Melchiorri, A. (Rome U. ; INFN, Rome) ; Mendes, L. (ESA, Madrid) ; Mennella, A. (Milan U. ; IASF, Milan) ; Migliaccio, M. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Mitra, S. (IUCAA, Pune ; Caltech, JPL) ; Miville-Deschênes, M.-A. (Orsay, IAS ; Canadian Inst. Theor. Astrophys.) ; Moneti, A. (Paris, Inst. Astrophys.) ; Montier, L. (IRAP, Toulouse) ; Moreno, R. (Meudon Observ.) ; Morgante, G. (IASF, Bologna) ; Mortlock, D. (Imperial Coll., London) ; Moss, A. (Nottingham U.) ; Mottet, S. (Paris, Inst. Astrophys.) ; Munshi, D. (Cardiff U.) ; Murphy, J.A. (NUIM, Maynooth) ; Naselsky, P. (Bohr Inst.) ; Nati, F. (Princeton U.) ; Natoli, P. (Ferrara U. ; ASI, Rome ; IASF, Bologna) ; Netterfield, C.B. (Toronto U., Astron. Dept.) ; Nørgaard-Nielsen, H.U. (Denmark, Tech. U.) ; Noviello, F. (Jodrell Bank) ; Novikov, D. (Lebedev Inst.) ; Novikov, I. (Bohr Inst. ; Lebedev Inst.) ; Oxborrow, C.A. (Denmark, Tech. U.) ; Paci, F. (INFN, Trieste ; SISSA, Trieste) ; Pagano, L. (Rome U. ; INFN, Rome) ; Pajot, F. (Orsay, IAS) ; Paoletti, D. (IASF, Bologna ; INFN, Bologna) ; Pasian, F. (Trieste Observ.) ; Patanchon, G. (APC, Paris) ; Pearson, T.J. (Caltech ; Caltech, IPAC) ; Perdereau, O. (Orsay, LAL) ; Perotto, L. (LPSC, Grenoble) ; Perrotta, F. (INFN, Trieste ; SISSA, Trieste) ; Pettorino, V. (U. Heidelberg, ITP) ; Piacentini, F. (Rome U.) ; Piat, M. (APC, Paris) ; Pierpaoli, E. (Southern California U.) ; Pietrobon, D. (Caltech, JPL) ; Plaszczynski, S. (Orsay, LAL) ; Pointecouteau, E. (IRAP, Toulouse) ; Polenta, G. (ASI, Rome ; Rome Observ.) ; Pratt, G.W. (AIM, Saclay) ; Prézeau, G. (Caltech ; Caltech, JPL) ; Prunet, S. (Paris, Inst. Astrophys.) ; Puget, J.-L. (Orsay, IAS) ; Rachen, J.P. (Nijmegen U., IMAPP ; Garching, Max Planck Inst., MPE) ; Reinecke, M. (Garching, Max Planck Inst., MPE) ; Remazeilles, M. (Jodrell Bank ; Orsay, IAS ; APC, Paris) ; Renault, C. (LPSC, Grenoble) ; Renzi, A. (Rome U., Tor Vergata ; INFN, Rome2) ; Ristorcelli, I. (IRAP, Toulouse) ; Rocha, G. (Caltech, JPL ; Caltech) ; Rosset, C. (APC, Paris) ; Rossetti, M. (Milan U. ; IASF, Milan) ; Roudier, G. (APC, Paris ; Paris Observ. ; Caltech, JPL) ; Rowan-Robinson, M. (Imperial Coll., London) ; Rusholme, B. (Caltech, IPAC) ; Sandri, M. (IASF, Bologna) ; Santos, D. (LPSC, Grenoble) ; Sauvé, A. (IRAP, Toulouse) ; Savelainen, M. (Helsinki Inst. of Phys. ; Helsinki U.) ; Savini, G. (University Coll. London) ; Scott, D. (British Columbia U.) ; Seiffert, M.D. (Caltech, JPL ; Caltech) ; Shellard, E.P.S. (Cambridge U., DAMTP) ; Spencer, L.D. (Cardiff U.) ; Stolyarov, V. (Cambridge U. ; Cambridge U., KICC ; Stavropol, Astrophys. Observ.) ; Stompor, R. (APC, Paris) ; Sudiwala, R. (Cardiff U.) ; Sutton, D. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Suur-Uski, A.-S. (Helsinki Inst. of Phys. ; Helsinki U.) ; Sygnet, J.-F. (Paris, Inst. Astrophys.) ; Tauber, J.A. (ESTEC, Noordwijk) ; Terenzi, L. (Rome U. ; IASF, Bologna) ; Toffolatti, L. (Oviedo U. ; Cantabria U., Santander ; IASF, Bologna) ; Tomasi, M. (Milan U. ; IASF, Milan) ; Tristram, M. (Orsay, LAL) ; Tucci, M. (Geneva U., Dept. Theor. Phys.) ; Tuovinen, J. (Trinity Coll., Dublin) ; Valenziano, L. (IASF, Bologna) ; Valiviita, J. (Helsinki Inst. of Phys. ; Helsinki U.) ; Van Tent, B. (Orsay, LPT) ; Vibert, L. (Orsay, IAS) ; Vielva, P. (Cantabria U., Santander) ; Villa, F. (IASF, Bologna) ; Wade, L.A. (Caltech, JPL) ; Wandelt, B.D. (Paris, Inst. Astrophys. ; Illinois U., Urbana) ; Watson, R. (Jodrell Bank) ; Wehus, I.K. (Caltech, JPL) ; Yvon, D. (IRFU, SPP, Saclay) ; Zacchei, A. (Trieste Observ.)

Publication 2016-09-20
Imprint 05 Feb 2015
Number of pages 30
In: Astron. Astrophys. 594 (2016) A7
DOI 10.1051/0004-6361/201525844
Subject category Astrophysics and Astronomy
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 non-linearity 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 10 relative to the 2013 release. Noise correlations introduced by pipeline filtering function are assessed using dedicated simulations. Angular cross-power spectra using datasets which are decorrelated in time are immune to the main systematic effects.
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 Zapis kreiran 2015-02-06, zadnja izmjena 2024-05-03


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