Planck 2015 results. VII. HFI TOI and beam processing

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 dete...

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Detalles Bibliográficos
Autores principales: Adam, R., Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Bartolo, N., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J.-P., Bersanelli, M., Bertincourt, B., Bielewicz, P., Bock, J.J., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Bucher, M., Burigana, C., Calabrese, E., Cardoso, J.-F., Catalano, A., Challinor, A., Chamballu, A., Chary, R.-R., Chiang, H.C., Christensen, P.R., Clements, D.L., Colombi, S., Colombo, L.P.L., Combet, C., Couchot, F., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Delouis, J.-M., Désert, F.-X., Diego, J.M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T.A., Eriksen, H.K., Falgarone, E., Fergusson, J., Finelli, F., Forni, O., Frailis, M., Fraisse, A.A., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Ghosh, T., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K.M., Gratton, S., Gruppuso, A., Gudmundsson, J.E., Hansen, F.K., Hanson, D., Harrison, D.L., Henrot-Versillé, S., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Jones, W.C., Juvela, M., Keihänen, E., Keskitalo, R., Kisner, T.S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J.-M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Le Jeune, M., Leahy, J.P., Lellouch, E., Leonardi, R., Lesgourgues, J., Levrier, F., Liguori, M., Lilje, P.B., Linden-Vørnle, M., López-Caniego, M., Lubin, P.M., Macías-Pérez, J.F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P.G., Martínez-González, E., Masi, S., Matarrese, S., McGehee, P., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Miville-Deschênes, M.-A., Moneti, A., Montier, L., Moreno, R., Morgante, G., Mortlock, D., Moss, A., Mottet, S., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Nørgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., Oxborrow, C.A., Paci, F., Pagano, L., Pajot, F., Paoletti, D., Pasian, F., Patanchon, G., Pearson, T.J., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Pratt, G.W., Prézeau, G., Prunet, S., Puget, J.-L., Rachen, J.P., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rowan-Robinson, M., Rusholme, B., Sandri, M., Santos, D., Sauvé, A., Savelainen, M., Savini, G., Scott, D., Seiffert, M.D., Shellard, E.P.S., Spencer, L.D., Stolyarov, V., Stompor, R., Sudiwala, R., Sutton, D., Suur-Uski, A.-S., Sygnet, J.-F., Tauber, J.A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Valenziano, L., Valiviita, J., Van Tent, B., Vibert, L., Vielva, P., Villa, F., Wade, L.A., Wandelt, B.D., Watson, R., Wehus, I.K., Yvon, D., Zacchei, A.
Lenguaje:eng
Publicado: 2015
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1051/0004-6361/201525844
http://cds.cern.ch/record/1987163
_version_ 1780945480663957504
author Adam, R.
Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoît, A.
Benoit-Lévy, A.
Bernard, J.-P.
Bersanelli, M.
Bertincourt, B.
Bielewicz, P.
Bock, J.J.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Boulanger, F.
Bucher, M.
Burigana, C.
Calabrese, E.
Cardoso, J.-F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R.-R.
Chiang, H.C.
Christensen, P.R.
Clements, D.L.
Colombi, S.
Colombo, L.P.L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Delouis, J.-M.
Désert, F.-X.
Diego, J.M.
Dole, H.
Donzelli, S.
Doré, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Enßlin, T.A.
Eriksen, H.K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A.A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Héraud, Y.
Gjerløw, E.
González-Nuevo, J.
Górski, K.M.
Gratton, S.
Gruppuso, A.
Gudmundsson, J.E.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
Henrot-Versillé, S.
Herranz, D.
Hildebrandt, S.R.
Hivon, E.
Hobson, M.
Holmes, W.A.
Hornstrup, A.
Hovest, W.
Huffenberger, K.M.
Hurier, G.
Jaffe, A.H.
Jaffe, T.R.
Jones, W.C.
Juvela, M.
Keihänen, E.
Keskitalo, R.
Kisner, T.S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J.-M.
Lasenby, A.
Lattanzi, M.
Lawrence, C.R.
Le Jeune, M.
Leahy, J.P.
Lellouch, E.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P.B.
Linden-Vørnle, M.
López-Caniego, M.
Lubin, P.M.
Macías-Pérez, J.F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P.G.
Martínez-González, E.
Masi, S.
Matarrese, S.
McGehee, P.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschênes, M.-A.
Moneti, A.
Montier, L.
Moreno, R.
Morgante, G.
Mortlock, D.
Moss, A.
Mottet, S.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C.B.
Nørgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T.J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G.W.
Prézeau, G.
Prunet, S.
Puget, J.-L.
Rachen, J.P.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rusholme, B.
Sandri, M.
Santos, D.
Sauvé, A.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M.D.
Shellard, E.P.S.
Spencer, L.D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sutton, D.
Suur-Uski, A.-S.
Sygnet, J.-F.
Tauber, J.A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vibert, L.
Vielva, P.
Villa, F.
Wade, L.A.
Wandelt, B.D.
Watson, R.
Wehus, I.K.
Yvon, D.
Zacchei, A.
author_facet Adam, R.
Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoît, A.
Benoit-Lévy, A.
Bernard, J.-P.
Bersanelli, M.
Bertincourt, B.
Bielewicz, P.
Bock, J.J.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Boulanger, F.
Bucher, M.
Burigana, C.
Calabrese, E.
Cardoso, J.-F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R.-R.
Chiang, H.C.
Christensen, P.R.
Clements, D.L.
Colombi, S.
Colombo, L.P.L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Delouis, J.-M.
Désert, F.-X.
Diego, J.M.
Dole, H.
Donzelli, S.
Doré, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Enßlin, T.A.
Eriksen, H.K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A.A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Héraud, Y.
Gjerløw, E.
González-Nuevo, J.
Górski, K.M.
Gratton, S.
Gruppuso, A.
Gudmundsson, J.E.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
Henrot-Versillé, S.
Herranz, D.
Hildebrandt, S.R.
Hivon, E.
Hobson, M.
Holmes, W.A.
Hornstrup, A.
Hovest, W.
Huffenberger, K.M.
Hurier, G.
Jaffe, A.H.
Jaffe, T.R.
Jones, W.C.
Juvela, M.
Keihänen, E.
Keskitalo, R.
Kisner, T.S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J.-M.
Lasenby, A.
Lattanzi, M.
Lawrence, C.R.
Le Jeune, M.
Leahy, J.P.
Lellouch, E.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P.B.
Linden-Vørnle, M.
López-Caniego, M.
Lubin, P.M.
Macías-Pérez, J.F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P.G.
Martínez-González, E.
Masi, S.
Matarrese, S.
McGehee, P.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschênes, M.-A.
Moneti, A.
Montier, L.
Moreno, R.
Morgante, G.
Mortlock, D.
Moss, A.
Mottet, S.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C.B.
Nørgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T.J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G.W.
Prézeau, G.
Prunet, S.
Puget, J.-L.
Rachen, J.P.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rusholme, B.
Sandri, M.
Santos, D.
Sauvé, A.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M.D.
Shellard, E.P.S.
Spencer, L.D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sutton, D.
Suur-Uski, A.-S.
Sygnet, J.-F.
Tauber, J.A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vibert, L.
Vielva, P.
Villa, F.
Wade, L.A.
Wandelt, B.D.
Watson, R.
Wehus, I.K.
Yvon, D.
Zacchei, A.
author_sort Adam, R.
collection CERN
description 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.
id cern-1987163
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2015
record_format invenio
spelling cern-19871632023-03-14T19:43:01Zdoi:10.1051/0004-6361/201525844http://cds.cern.ch/record/1987163engAdam, R.Ade, P.A.R.Aghanim, N.Arnaud, M.Ashdown, M.Aumont, J.Baccigalupi, C.Banday, A.J.Barreiro, R.B.Bartolo, N.Battaner, E.Benabed, K.Benoît, A.Benoit-Lévy, A.Bernard, J.-P.Bersanelli, M.Bertincourt, B.Bielewicz, P.Bock, J.J.Bonavera, L.Bond, J.R.Borrill, J.Bouchet, F.R.Boulanger, F.Bucher, M.Burigana, C.Calabrese, E.Cardoso, J.-F.Catalano, A.Challinor, A.Chamballu, A.Chary, R.-R.Chiang, H.C.Christensen, P.R.Clements, D.L.Colombi, S.Colombo, L.P.L.Combet, C.Couchot, F.Coulais, A.Crill, B.P.Curto, A.Cuttaia, F.Danese, L.Davies, R.D.Davis, R.J.de Bernardis, P.de Rosa, A.de Zotti, G.Delabrouille, J.Delouis, J.-M.Désert, F.-X.Diego, J.M.Dole, H.Donzelli, S.Doré, O.Douspis, M.Ducout, A.Dupac, X.Efstathiou, G.Elsner, F.Enßlin, T.A.Eriksen, H.K.Falgarone, E.Fergusson, J.Finelli, F.Forni, O.Frailis, M.Fraisse, A.A.Franceschi, E.Frejsel, A.Galeotta, S.Galli, S.Ganga, K.Ghosh, T.Giard, M.Giraud-Héraud, Y.Gjerløw, E.González-Nuevo, J.Górski, K.M.Gratton, S.Gruppuso, A.Gudmundsson, J.E.Hansen, F.K.Hanson, D.Harrison, D.L.Henrot-Versillé, S.Herranz, D.Hildebrandt, S.R.Hivon, E.Hobson, M.Holmes, W.A.Hornstrup, A.Hovest, W.Huffenberger, K.M.Hurier, G.Jaffe, A.H.Jaffe, T.R.Jones, W.C.Juvela, M.Keihänen, E.Keskitalo, R.Kisner, T.S.Kneissl, R.Knoche, J.Kunz, M.Kurki-Suonio, H.Lagache, G.Lamarre, J.-M.Lasenby, A.Lattanzi, M.Lawrence, C.R.Le Jeune, M.Leahy, J.P.Lellouch, E.Leonardi, R.Lesgourgues, J.Levrier, F.Liguori, M.Lilje, P.B.Linden-Vørnle, M.López-Caniego, M.Lubin, P.M.Macías-Pérez, J.F.Maggio, G.Maino, D.Mandolesi, N.Mangilli, A.Maris, M.Martin, P.G.Martínez-González, E.Masi, S.Matarrese, S.McGehee, P.Melchiorri, A.Mendes, L.Mennella, A.Migliaccio, M.Mitra, S.Miville-Deschênes, M.-A.Moneti, A.Montier, L.Moreno, R.Morgante, G.Mortlock, D.Moss, A.Mottet, S.Munshi, D.Murphy, J.A.Naselsky, P.Nati, F.Natoli, P.Netterfield, C.B.Nørgaard-Nielsen, H.U.Noviello, F.Novikov, D.Novikov, I.Oxborrow, C.A.Paci, F.Pagano, L.Pajot, F.Paoletti, D.Pasian, F.Patanchon, G.Pearson, T.J.Perdereau, O.Perotto, L.Perrotta, F.Pettorino, V.Piacentini, F.Piat, M.Pierpaoli, E.Pietrobon, D.Plaszczynski, S.Pointecouteau, E.Polenta, G.Pratt, G.W.Prézeau, G.Prunet, S.Puget, J.-L.Rachen, J.P.Reinecke, M.Remazeilles, M.Renault, C.Renzi, A.Ristorcelli, I.Rocha, G.Rosset, C.Rossetti, M.Roudier, G.Rowan-Robinson, M.Rusholme, B.Sandri, M.Santos, D.Sauvé, A.Savelainen, M.Savini, G.Scott, D.Seiffert, M.D.Shellard, E.P.S.Spencer, L.D.Stolyarov, V.Stompor, R.Sudiwala, R.Sutton, D.Suur-Uski, A.-S.Sygnet, J.-F.Tauber, J.A.Terenzi, L.Toffolatti, L.Tomasi, M.Tristram, M.Tucci, M.Tuovinen, J.Valenziano, L.Valiviita, J.Van Tent, B.Vibert, L.Vielva, P.Villa, F.Wade, L.A.Wandelt, B.D.Watson, R.Wehus, I.K.Yvon, D.Zacchei, A.Planck 2015 results. VII. HFI TOI and beam processingAstrophysics and AstronomyThe 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.The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857GHz) in intensity and at four frequencies in linear polarization (100, 143, 217, and 353GHz). 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.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.arXiv:1502.01586oai:cds.cern.ch:19871632015-02-05
spellingShingle Astrophysics and Astronomy
Adam, R.
Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoît, A.
Benoit-Lévy, A.
Bernard, J.-P.
Bersanelli, M.
Bertincourt, B.
Bielewicz, P.
Bock, J.J.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Boulanger, F.
Bucher, M.
Burigana, C.
Calabrese, E.
Cardoso, J.-F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R.-R.
Chiang, H.C.
Christensen, P.R.
Clements, D.L.
Colombi, S.
Colombo, L.P.L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Delouis, J.-M.
Désert, F.-X.
Diego, J.M.
Dole, H.
Donzelli, S.
Doré, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Enßlin, T.A.
Eriksen, H.K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A.A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Héraud, Y.
Gjerløw, E.
González-Nuevo, J.
Górski, K.M.
Gratton, S.
Gruppuso, A.
Gudmundsson, J.E.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
Henrot-Versillé, S.
Herranz, D.
Hildebrandt, S.R.
Hivon, E.
Hobson, M.
Holmes, W.A.
Hornstrup, A.
Hovest, W.
Huffenberger, K.M.
Hurier, G.
Jaffe, A.H.
Jaffe, T.R.
Jones, W.C.
Juvela, M.
Keihänen, E.
Keskitalo, R.
Kisner, T.S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J.-M.
Lasenby, A.
Lattanzi, M.
Lawrence, C.R.
Le Jeune, M.
Leahy, J.P.
Lellouch, E.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P.B.
Linden-Vørnle, M.
López-Caniego, M.
Lubin, P.M.
Macías-Pérez, J.F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P.G.
Martínez-González, E.
Masi, S.
Matarrese, S.
McGehee, P.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschênes, M.-A.
Moneti, A.
Montier, L.
Moreno, R.
Morgante, G.
Mortlock, D.
Moss, A.
Mottet, S.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C.B.
Nørgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T.J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G.W.
Prézeau, G.
Prunet, S.
Puget, J.-L.
Rachen, J.P.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rusholme, B.
Sandri, M.
Santos, D.
Sauvé, A.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M.D.
Shellard, E.P.S.
Spencer, L.D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sutton, D.
Suur-Uski, A.-S.
Sygnet, J.-F.
Tauber, J.A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vibert, L.
Vielva, P.
Villa, F.
Wade, L.A.
Wandelt, B.D.
Watson, R.
Wehus, I.K.
Yvon, D.
Zacchei, A.
Planck 2015 results. VII. HFI TOI and beam processing
title Planck 2015 results. VII. HFI TOI and beam processing
title_full Planck 2015 results. VII. HFI TOI and beam processing
title_fullStr Planck 2015 results. VII. HFI TOI and beam processing
title_full_unstemmed Planck 2015 results. VII. HFI TOI and beam processing
title_short Planck 2015 results. VII. HFI TOI and beam processing
title_sort planck 2015 results. vii. hfi toi and beam processing
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1051/0004-6361/201525844
http://cds.cern.ch/record/1987163
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