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1. Planck Early Results. II. The thermal performance of Planck

Author: Planck Collaboration, Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoit, A., Bernard, J. P., Bersanelli, M., Bhandari, P., Bhatia, R., Bock, J. J., Bonaldi, A., Bond, J. R., Borders, J., Borrill, J., Bouchet, F. R., Bowman, B., Bradshaw, T., Breelle, E., Bucher, M., Burigana, C., Butler, R. C., Cabella, P., Camus, P., Cantalupo, C. M., Cappellini, B., Cardoso, J. F., Catalano, A., Cayon, L., Challinor, A., Chamballu, A., Chambelland, J. P., Charra, J., Charra, M., Chiang, L. Y, Chiang, C., Christensen, P. R., Clements, D. L., Collaudin, B., Colombi, S., Couchot, F., Coulais, A., Crill, B. P., Crook, M., Cuttaia, F., Damasio, C., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Gasperis, G., de Rosa, A., Delabrouille, J., Delouis, J. M., Desert, F. -X., Doerl, U., Dolag, K., Donzelli, S., Dore, O., Douspis, M., Dupac, X., Efstathiou, G., Enslin, T. A., Eriksen, H. K., Finelli, F., Foley, S., Forni, O., Fosalba, P., Fourmond, J. J., Frailis, M., Franceschi, E., Galeotta, S., Ganga, K., Gavila, E., Giard, M., Giardino, G., Giraud-Heraud, Y., Gonzalez-Nuevo, J., Gorski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Guyot, G., Harrison, D., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Hoyland, R. J., Huffenberger, K. M., Israelsson, U., Jaffe, A. H., Jones, W. C., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knox, L., Kurki-Suonio, H., Lagache, G., Lamarre, J. M., Lami, P., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leonardi, R., Leroy, C., Lilje, P. B., Lopez-Caniego, M., Lubin, P. M., Macias-Perez, J. F., Maciaszek, T., MacTavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., McGehee, P., Meinhold, P. R., Melchiorri, A., Melot, F., Mendes, L., Mennella, A., Miville-Deschenes, M. -A., Moneti, A., Montier, L., Mora, J., Morgante, G., Morisset, N., Mortlock, D., Munshi, D., Murphy, A., Naselsky, P., Nash, A., Natoli, P., Netterfield, C. B., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Pajot, F., Pasian, F., Patanchon, G., Pearson, D., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Poutanen, T., Prezeau, G., Prina, M., Prunet, S., Puget, J. L., Rachen, J. P., Rebolo, R., Reinecke, M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rubiino-Martin, J. A., Rusholme, B., Sandri, M., Santos, D., Schaefer, B. M., Scott, D., Seiffert, M. D., Shellard, P., Smoot, G. F., Starck, J. -L., Stassi, P., Stivoli, F., Stolyarov, V., Stompor, R., Sudiwala, R., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Torre, J. -P., Tristram, M., Tuovinen, J., Valenziano, L., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, C., White, S. D. M., Wilkinson, A., Wilson, P., Yvon, D., Zacchei, A., Zhang, B., and Zonca, A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The performance of the Planck instruments in space is enabled by their low operating temperatures, 20K for LFI and 0.1K for HFI, achieved through a combination of passive radiative cooling and three active mechanical coolers. The scientific requirement for very broad frequency coverage led to two detector technologies with widely different temperature and cooling needs. Active coolers could satisfy these needs; a helium cryostat, as used by previous cryogenic space missions (IRAS, COBE, ISO, Spitzer, AKARI), could not. Radiative cooling is provided by three V-groove radiators and a large telescope baffle. The active coolers are a hydrogen sorption cooler (<20K), a 4He Joule-Thomson cooler (4.7K), and a 3He-4He dilution cooler (1.4K and 0.1K). The flight system was at ambient temperature at launch and cooled in space to operating conditions. The HFI bolometer plate reached 93mK on 3 July 2009, 50 days after launch. The solar panel always faces the Sun, shadowing the rest of Planck, andoperates at a mean temperature of 384K. At the other end of the spacecraft, the telescope baffle operates at 42.3K and the telescope primary mirror operates at 35.9K. The temperatures of key parts of the instruments are stabilized by both active and passive methods. Temperature fluctuations are driven by changes in the distance from the Sun, sorption cooler cycling and fluctuations in gas-liquid flow, and fluctuations in cosmic ray flux on the dilution and bolometer plates. These fluctuations do not compromise the science data., Comment: Accepted by A&A. Also available at http://www.rssd.esa.int
Published: 2011
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2. Planck early results: first assessment of the High Frequency Instrument in-flight performance

Author: Planck HFI Core Team, Ade, P. A. R., Aghanim, N., Ansari, R., Arnaud, M., Ashdown, M., Aumont, J., Banday, A. J., Bartelmann, M., Bartlett, J. G., Battaner, E., Benabed, K., Benot, A., Bernard, J. -P., Bersanelli, M., Bhatia, R., Bock, J. J., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bradshaw, T., Brelle, E., Bucher, M., Camus, P., Cardoso, J. -F., Catalano, A., Challinor, A., Chamballu, A., Charra, J., Charra, M., Chary, R. -R., Chiang, C., Church, S., Clements, D. L., Colombi, S., Couchot, F., Coulais, A., Cressiot, C., Crill, B. P., Crook, M., de Bernardis, P., Delabrouille, J., Delouis, J. -M., Désert, F. -X., Dolag, K., Dole, H., Doré, O., Douspis, M., Efstathiou, G., Eng, P., Filliard, C., Forni, O., Fosalba, P., Fourmond, J. -J., Ganga, K., Giard, M., Girard, D., Giraud-Héraud, Y., Gispert, R., Gorski, K. M., Gratton, S., Griffin, M., Guyot, G., Haissinski, J., Harrison, D., Helou, G., Henrot-Versillé, S., Hernandez-Monteagudo, C., Hildebrandt, S. R., Hills, R., Hivon, E., Hobson, M., Holmes, W. A., Huenberger, K. M., Jae, A. H., Jones, W. C., Kaplan, J., Kneissl, R., Knox, L., Lagache, G., Lamarre, J. -M., Lami, P., Lange, A. E., Lasenby, A., Lavabre, A., Lawrence, C. R., Leriche, B., Leroy, C., Longval, Y., Macas-Perez, J. F., Maciaszek, T., MacTavish, C. J., Maei, B., Mandolesi, N., Mann, R., Mansoux, B., Masi, S., Matsumura, T., McGehee, P., Melin, J. -B., Mercier, C., Miville-Deschnes, M. -A., Moneti, A., Montier, L., Mortlock, D., Murphy, A., Nati, F., Nettereld, C. B., Norgaard-Nielsen, H. U., North, C., Noviello, F., Novikov, D., Osborne, S., Paine, C., Pajot, F., Patanchon, G., Peacocke, T., Pearson, T. J., Perdereau, O., Perotto, L., Piacentini, F., Piat, M., Plaszczynski, S., Pointecouteau, E., Pons, R., Ponthieu, N., Prezeau, G., Prunet, S., Puget, J. -L., Reach, W. T., Renault, C., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rowan-Robinson, M., Rusholme, B., Santos, D., Savini, G., Schaefer, B. M., Shellard, P., Spencer, L., Starck, J. -L., Stassi, P., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sygnet, J. -F., Tauber, J. A., Thum, C., Torre, J. -P., Touze, F., Tristram, M., Van Leeuwen, F., Vibert, L., Vibert, D., Wade, L. A., Wandelt, B. D., White, S. D. M., Wiesemeyer, H., Woodcraft, A., Yurchenko, V., Yvon, D., and Zacchei, A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the Cosmic Microwave Background and galactic foregrounds in six wide bands centered at 100, 143, 217, 353, 545 and 857 GHz at an angular resolution of 10' (100 GHz), 7' (143 GHz), and 5' (217 GHz and higher). HFI has been operating flawlessly since launch on 14 May 2009. The bolometers cooled to 100 mK as planned. The settings of the readout electronics, such as the bolometer bias current, that optimize HFI's noise performance on orbit are nearly the same as the ones chosen during ground testing. Observations of Mars, Jupiter, and Saturn verified both the optical system and the time response of the detection chains. The optical beams are close to predictions from physical optics modeling. The time response of the detection chains is close to pre-launch measurements. The detectors suffer from an unexpected high flux of cosmic rays related to low solar activity. Due to the redundancy of Planck's observations strategy, the removal of a few percent of data contaminated by glitches does not affect significantly the sensitivity. The cosmic rays heat up significantly the bolometer plate and the modulation on periods of days to months of the heat load creates a common drift of all bolometer signals which do not affect the scientific capabilities. Only the high energy cosmic rays showers induce inhomogeneous heating which is a probable source of low frequency noise., Comment: Submitted to A&A. 22 pages, 6 tables, 21 figures. One of a set of simultaneous papers for the Planck Mission
Published: 2011
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3. Planck Early Results: The Planck mission

Author: Planck Collaboration, Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Battaner, E., Benabed, K., Bennett, K., Benoît, A., Bernard, J. -P., Bersanelli, M., Bhatia, R., Bock, J. J., Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bradshaw, T., Bremer, M., Bucher, M., Burigana, C., Butler, R. C., Cabella, P., Cantalupo, C. M., Cappellini, B., Cardoso, J. -F., Carr, R., Casale, M., Catalano, A., Cayón, L., Challinor, A., Chamballu, A., Charra, J., Chary, R. -R., Chiang, L. -Y, Chiang, C., Christensen, P. R., Clements, D. L., Colombi, S., Couchot, F., Coulais, A., Crill, B. P., Crone, G., Crook, M., Cuttaia, F., Danese, L., D'Arcangelo, O., Davies, R. D., Davis, R. J., de Bernardis, P., de Bruin, J., de Gasperis, G., de Rosa, A., de Zotti, G., Delabrouille, J., Delouis, J. -M., Dèsert, F. -X., Dick, J., Dickinson, C., Dolag, K., Dole, H., Donzelli, S., Dorè, O., Dörl, U., Douspis, M., Dupac, X., Efstathiou, G., Enfllin, T. A., Eriksen, H. K., Finelli, F., Foley, S., Forni, O., Fosalba, P., Frailis, M., Franceschi, E., Freschi, M., Gaier, T. C., Galeotta, S., Gallegos, J., Gandolfo, B., Ganga, K., Giard, M., Giardino, G., Gienger, G., Giraud-Hèraud, Y., González, J., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Guyot, G., Haissinski, J., Hansen, F. K., Harrison, D., Helou, G., Henrot-Versillè, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Hoyland, R. J., Huffenberger, K. M., Jaffe, A. H., Jagemann, T., Jones, W. C., Juillet, J. J., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knox, L., Krassenburg, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lange, A. E., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Leroy, C., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lowe, S., Lubin, P. M., Macìas-Pèrez, J. F., Maciaszek, T., MacTavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martìnez-González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., McDonald, A., McGehee, P., Meinhold, P. R., Melchiorri, A., Melin, J. -B., Mendes, L., Mennella, A., Mevi, C., Miniscalco, R., Mitra, S., Miville-Deschínes, M. -A., Moneti, A., Montier, L., Morgante, G., Morisset, N., Mortlock, D., Munshi, D., Murphy, A., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I. J., Ortiz, I., Osborne, S., Osuna, P., Oxborrow, C. A., Pajot, F., Paladini, R., Partridge, B., Pasian, F., Passvogel, T., Patanchon, G., Pearson, D., Pearson, T. J., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Prèzeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Reix, J. -M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rowan-Robinson, M., Rubiñ-Martìn, J. A., Rusholme, B., Salerno, E., Sandri, M., Santos, D., Savini, G., Schaefer, B. M., Scott, D., Seiffert, M. D., Shellard, P., Simonetto, A., Smoot, G. F., Sozzi, C., Starck, J. -L., Sternberg, J., Stivoli, F., Stolyarov, V., Stompor, R., Stringhetti, L., Sudiwala, R., Sunyaev, R., Sygnet, J. -F., Tapiador, D., Tauber, J. A., Tavagnacco, D., Taylor, D., Terenzi, L., Texier, D., Toffolatti, L., Tomasi, M., Torre, J. -P., Tristram, M., Tuovinen, J., Türler, M., Tuttlebee, M., Umana, G., Valenziano, L., Valiviita, J., Varis, J., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, C., White, S. D. M., White, M., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: The European Space Agency's Planck satellite was launched on 14 May 2009, and has been surveying the sky stably and continuously since 13 August 2009. Its performance is well in line with expectations, and it will continue to gather scientific data until the end of its cryogenic lifetime. We give an overview of the history of Planck in its first year of operations, and describe some of the key performance aspects of the satellite. This paper is part of a package submitted in conjunction with Planck's Early Release Compact Source Catalogue, the first data product based on Planck to be released publicly. The package describes the scientific performance of the Planck payload, and presents results on a variety of astrophysical topics related to the sources included in the Catalogue, as well as selected topics on diffuse emission., Comment: This is part of a package of Planck papers labelled in their titles as "Planck Early Results". The whole package can also be downloaded from http://www.rssd.esa.int/Planck. This paper was accepted by Astronomy & Astrophysics on 31 May 2011
Published: 2011
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4. The Planck High Frequency Instrument, a 3rd generation CMB experiment, and a full sky submillimeter survey

Author: Lamarre, J. M., Puget, J. L., Bouchet, F., Ade, P. A. R., Benoit, A., Bernard, J. P., Bock, J., De Bernardis, P., Charra, J., Couchot, F., Delabrouille, J., Efstathiou, G., Giard, M., Guyot, G., Lange, A., Maffei, B., Murphy, A., Pajot, F., Piat, M., Ristorcelli, I., Santos, D., Sudiwala, R., Sygnet, J. F., Torre, J. P., Yurchenko, V., and Yvon, D.
Subjects: Astrophysics
Abstract: The High Frequency Instrument (HFI) of Planck is the most sensitive CMB experiment ever planned. Statistical fluctuations (photon noise) of the CMB itself will be the major limitation to the sensitivity of the CMB channels. Higher frequency channels will measure galactic foregrounds. Together with the Low Frequency Instrument, this will make a unique tool to measure the full sky and to separate the various components of its spectrum. Measurement of the polarization of these various components will give a new picture of the CMB. In addition, HFI will provide the scientific community with new full sky maps of intensity and polarization at six frequencies, with unprecedented angular resolution and sensitivity. This paper describes the logics that prevailed to define the HFI and the performances expected from this instrument. It details several features of the HFI design that have not been published up to now., Comment: To be published in the proceedings of the workshop on "The Cosmic Microwave Background and its Polarization", New Astronomy Reviews, (eds., S. Hanany and R.A. Olive)
Published: 2003
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5. Are Solar Acoustic Modes Correlated ?

Author: Foglizzo, T., Garcia, R. A., Boumier, P., Charra, J., Gabriel, A. H., Grec, G., Robillot, J. M., Cortes, T. Roca, Turck-Chieze, S., and Ulrich, R. K.
Subjects: Astrophysics
Abstract: We have studied the statistical properties of the energy of individual acoustic modes, extracted from 310 days of GOLF data near the solar minimum. The exponential distribution of the energy of each mode is clearly seen. The modes are found to be uncorrelated with a +-0.6 % accuracy, thus supporting the hypothesis of stochastic excitation by the solar convection. Nevertheless, the same analysis performed on the same modes just before the solar maximum, using IPHIR data, rejects the hypothesis of no correlation at a 99.3 % confidence level. A simple model suggests that 31.3 +-9.4 % of the energy of each mode is coherent among the modes studied in IPHIR data, correponding to a mean correlation of 10.7 +-5.9 %., Comment: 10 pages A&A Latex, 13 EPSF figures, to appear in A&A
Published: 1997

6. First Results on p Modes from GOLF Experiment

Author: Lazrek, M., Baudin, F., Bertello, L., Boumier, P., Charra, J., Fierry-Fraillon, D., Fossat, E., Gabriel, A. H., García, R. A., Gelly, B., Gouiffes, C., Grec, G., Pallé, P. L., Hernández, F. Pérez, Régulo, C., Renaud, C., Robillot, J.-M., Cortés, T. Roca, Turck-Chièze, S., Ulrich, R. K., Fleck, B., editor, and Švestka, Z., editor
Published: 1997
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7. Performance and Early Results from the GOLF Instrument Flown on the SOHO Mission

Author: Gabriel, A. H., Charra, J., Grec, G., Robillot, J.-M., Cortés, T. Roca, Turck-Chièze, S., Ulrich, R., Basu, S., Baudin, F., Bertello, L., Boumier, P., Charra, M., Christensen-Dalsgaard, J., Decaudin, M., Dzitko, H., Foglizzo, T., Fossat, E., García, R. A., Herreros, J. M., Lazrek, M., Pallé, P. L., Pétrou, N., Renaud, C., Régulo, C., Fleck, B., editor, and Švestka, Z., editor
Published: 1997
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8. First View of the Solar Core from GOLF Acoustic Modes

Author: Turck-Chièze, S., Basu, S., Brun, A. S., Christemsen-Dalsgaard, J., Eff-Darwich, A., Lopes, I., Hernández, F. Pérez, Berthomieu, G., Provost, J., Ulrich, R. K., Baudin, F., Boumier, P., Charra, J., Gabriel, A. H., Garcia, R. A., Grec, G., Renaud, C., Robillot, J. M., Cortés, T. Roca, Fleck, B., editor, and Švestka, Z., editor
Published: 1997
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9. Global Oscillations at Low Frequency from the Soho Mission (GOLF)

Author: Gabriel, A. H., Grec, G., Charra, J., Robillot, J.-M., Roca Cortés, T., Turck-Chièze, S., Bocchia, R., Boumier, P., Cantin, M., Cespédes, E., Cougrand, B., Crétolle, J., Damé, L., Decaudin, M., Delache, P., Denis, N., Duc, R., Dzitko, H., Fossat, E., Fourmond, J.-J., García, R. A., Gough, D., Grivel, C., Herreros, J. M., Lagardère, H., Moalic, J.-P., Pallé, P. L., Pétrou, N., Sanchez, M., Ulrich, R., Van Der Raay, H. B., Fleck, B., editor, Domingo, V., editor, and Poland, A., editor
Published: 1995
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10. First Results on it p Modes from GOLF Experiment

Author: Lazrek, M., Baudin, F., Bertello, L., Boumier, P., Charra, J., Fierry-Fraillon, D., Fossat, E., Gabriel, A. H., García, R. A., Gelly, B., Gouiffes, C., Grec, G., Pallé, P. L., Pérez Hernández, F., Régulo, C., Renaud, C., Robillot, J.-M., Roca Cortés, T., Turck-Chièze, S., and Ulrich, R. K.
Published: 1997
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11. Golf Results: Today’s View on the Solar Modes

Author: Grec, G., primary, Turck-Chièze, S., additional, Lazrek, M., additional, Roca Cortés, T., additional, Bertello, L., additional, Baudin, F., additional, Boumier, P., additional, Charra, J., additional, Fierry-Fraillon, D., additional, Fossat, E., additional, Gabriel, A. H., additional, Garcia, R. A., additional, Gelly, B., additional, Gouiffes, C., additional, Régulo, C., additional, Renaud, C., additional, Robillot, J. M., additional, and Ulrich, R. K., additional
Published: 1997
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12. Performance and First Results from the Golf Instrument on Soho

Author: Gabriel, A. H., primary, Charra, J., additional, Grec, G., additional, Robillot, J.-M., additional, Roca Cortés, T., additional, Turck-Chièze, S., additional, Ulrich, R., additional, Baudin, F., additional, Bertello, L., additional, Boumier, P., additional, Decaudin, M., additional, Dzitko, H., additional, Foglizzo, T., additional, Fossat, E., additional, García, R. A., additional, Herreros, J. M., additional, Lazrek, M., additional, Pallé, P. L., additional, Pétrou, N., additional, Renaud, C., additional, and Régulo, G., additional
Published: 1997
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13. The spatial GOLF project

Author: Turck-Chièze, S., primary, Bocchia, R., additional, Boumier, P., additional, Cantin, M., additional, Charra, J., additional, Cougrand, B., additional, Cretolle, J., additional, Denis, N., additional, Duc, R., additional, Dzitko, H., additional, Decaudin, M., additional, Gabriel, A., additional, Herreros, J., additional, Grec, G., additional, Petrou, N., additional, Cortes, T. Roca, additional, and Robillot, J.M., additional
Published: 1994
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14. Planck pre-launch status: The Planck mission

Author: Tauber, J, Mandolesi, N, Puget, J, Banos, T, Bersanelli, M, Bouchet, F, Butler, R, Charra, J, Crone, G, Dodsworth, J, Efstathiou, G, Gispert, R, Guyot, G, Gregorio, A, Juillet, J, Lamarre, J, Laureijs, R, Lawrence, C, NØRGAARD NIELSEN, H, Passvogel, T, Reix, J, Texier, D, Vibert, L, Zacchei, A, Ade, P, Aghanim, N, Aja, B, Alippi, E, Aloy, L, Armand, P, Arnaud, M, Arondel, A, ARREOLA VILLANUEVA, A, Artal, E, Artina, E, Arts, A, Ashdown, M, Aumont, J, Azzaro, M, Bacchetta, A, Baccigalupi, C, Baker, M, Balasini, M, Balbi, A, Banday, A, Barbier, G, Barreiro, R, Bartelmann, M, Battaglia, P, Battaner, E, Benabed, K, Beney, J, Beneyton, R, Bennett, K, Benoit, A, Bernard, J, Bhandari, P, Bhatia, R, Biggi, M, Biggins, R, Billig, G, Blanc, Y, Blavot, H, Bock, J, Bonaldi, A, Bond, R, Bonis, J, Borders, J, Borrill, J, Boschini, L, Boulanger, F, Bouvier, J, Bouzit, M, Bowman, R, Bréelle, E, Bradshaw, T, Braghin, M, Bremer, M, Brienza, D, Broszkiewicz, D, Burigana, C, Burkhalter, M, Cabella, P, Cafferty, T, Cairola, M, Caminade, S, Camus, P, Cantalupo, C, Cappellini, B, Cardoso, J, Carr, R, Catalano, A, Cayón, L, Cesa, M, Chaigneau, M, Challinor, A, Chamballu, A, Chambelland, J, Charra, M, Chiang, L, Chlewicki, G, Christensen, P, Church, S, Ciancietta, E, Cibrario, M, Cizeron, R, Clements, D, Collaudin, B, Colley, J, Colombi, S, Colombo, A, Colombo, F, Corre, O, Couchot, F, Cougrand, B, Coulais, A, Couzin, P, Crane, B, Crill, B, Crook, M, Crumb, D, Cuttaia, F, Dörl, U, DA SILVA, P, Daddato, R, Damasio, C, Danese, L, D'Aquino, G, D'Arcangelo, O, Dassas, K, Davies, R, Davies, W, Davis, R, DE BERNARDIS, P, DE CHAMBURE, D, DE GASPERIS, G, DE LA FUENTE, M, DE PACO, P, DE ROSA, A, DE TROIA, G, DE ZOTTI, G, Dehamme, M, Delabrouille, J, Delouis, J, Désert, F, DI GIROLAMO, G, Dickinson, C, Doelling, E, Dolag, K, Domken, I, Douspis, M, Doyle, D, Du, S, Dubruel, D, Dufour, C, Dumesnil, C, Dupac, X, Duret, P, Eder, C, Elfving, A, Enlin, T, Eng, P, English, K, Eriksen, H, Estaria, P, Falvella, M, Ferrari, F, Finelli, F, Fishman, A, Fogliani, S, Foley, S, Fonseca, A, Forma, G, Forni, O, Fosalba, P, Fourmond, J, Frailis, M, Franceschet, C, Franceschi, E, François, S, Frerking, M, GÓMEZ REÑASCO, M, Górski, K, Gaier, T, Galeotta, S, Ganga, K, GARCÍA LÁZARO, J, Garnica, A, Gaspard, M, Gavila, E, Giard, M, Giardino, G, Gienger, G, GIRAUD HERAUD, Y, Glorian, J, Griffin, M, Gruppuso, A, Guglielmi, L, Guichon, D, Guillaume, B, Guillouet, P, Haissinski, J, Hansen, F, Hardy, J, Harrison, D, Hazell, A, Hechler, M, Heckenauer, V, Heinzer, D, Hell, R, HENROT VERSILLÉ, S, HERNÁNDEZ MONTEAGUDO, C, Herranz, D, Herreros, J, Hervier, V, Heske, A, Heurtel, A, Hildebrandt, S, Hills, R, Hivon, E, Hobson, M, Hollert, D, Holmes, W, Hornstrup, A, Hovest, W, Hoyland, R, Huey, G, Huffenberger, K, Hughes, N, Israelsson, U, Jackson, B, Jaffe, A, Jaffe, T, Jagemann, T, Jessen, N, Jewell, J, Jones, W, Juvela, M, Kaplan, J, Karlman, P, Keck, F, Keihänen, E, King, M, Kisner, T, Kletzkine, P, Kneissl, R, Knoche, J, Knox, L, Koch, T, Krassenburg, M, KURKI SUONIO, H, Lähteenmäki, A, Lagache, G, Lagorio, E, Lami, P, Lande, J, Lange, A, Langlet, F, Lapini, R, Lapolla, M, Lasenby, A, LE JEUNE, M, Leahy, J, Lefebvre, M, Legrand, F, LE MEUR, G, Leonardi, R, Leriche, B, Leroy, C, Leutenegger, P, Levin, S, Lilje, P, Lindensmith, C, LINDEN VØRNLE, M, Loc, A, Longval, Y, Lubin, P, Luchik, T, Luthold, I, MACIAS PEREZ, J, Maciaszek, T, Mactavish, C, Madden, S, Maffei, B, Magneville, C, Maino, D, Mambretti, A, Mansoux, B, Marchioro, D, Maris, M, Marliani, F, Marrucho, J, MARTÍ CANALES, J, MARTÍNEZ GONZÁLEZ, E, MARTÍN POLEGRE, A, Martin, P, Marty, C, Marty, W, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, Mcdonald, A, Mcgrath, P, Mediavilla, A, Meinhold, P, Mélin, J, Melot, F, Mendes, L, Mennella, A, Mervier, C, Meslier, L, Miccolis, M, MIVILLE DESCHENES, M, Moneti, A, Montet, D, Montier, L, Mora, J, Morgante, G, Morigi, G, Morinaud, G, Morisset, N, Mortlock, D, Mottet, S, Mulder, J, Munshi, D, Murphy, A, Murphy, P, Musi, P, Narbonne, J, Naselsky, P, Nash, A, Nati, F, Natoli, P, Netterfield, B, Newell, J, Nexon, M, Nicolas, C, Nielsen, P, Ninane, N, Noviello, F, Novikov, D, Novikov, I, O'Dwyer, I, Oldeman, P, Olivier, P, Ouchet, L, Oxborrow, C, PÉREZ CUEVAS, L, Pagan, L, Paine, C, Pajot, F, Paladini, R, Pancher, F, Panh, J, Parks, G, Parnaudeau, P, Partridge, B, Parvin, B, Pascual, J, Pasian, F, Pearson, D, Pearson, T, Pecora, M, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Piersanti, O, Plaige, E, Plaszczynski, S, Platania, P, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poulleau, G, Poutanen, T, Prézeau, G, Pradell, L, Prina, M, Prunet, S, Rachen, J, Rambaud, D, Rame, F, Rasmussen, I, Rautakoski, J, Reach, W, Rebolo, R, Reinecke, M, Reiter, J, Renault, C, Ricciardi, S, Rideau, P, Riller, T, Ristorcelli, I, Riti, J, Rocha, G, Roche, Y, Pons, R, Rohlfs, R, Romero, D, Roose, S, Rosset, C, Rouberol, S, ROWAN ROBINSON, M, RUBIÑO MARTÍN, J, Rusconi, P, Rusholme, B, Salama, M, Salerno, E, Sandri, M, Santos, D, Sanz, J, Sauter, L, Sauvage, F, Savini, G, Schmelzel, M, Schnorhk, A, Schwarz, W, Scott, D, Seiffert, M, Shellard, P, Shih, C, Sias, M, Silk, J, Silvestri, R, Sippel, R, Smoot, G, Starck, J, Stassi, P, Sternberg, J, Stivoli, F, Stolyarov, V, Stompor, R, Stringhetti, L, Strommen, D, Stute, T, Sudiwala, R, Sugimura, R, Sunyaev, R, Sygnet, J, Türler, M, Taddei, E, Tallon, J, Tamiatto, C, Taurigna, M, Taylor, D, Terenzi, L, Thuerey, S, Tillis, J, Tofani, G, Toffolatti, L, Tommasi, E, Tomasi, M, Tonazzini, E, Torre, J, Tosti, S, Touze, F, Tristram, M, Tuovinen, J, Tuttlebee, M, Umana, G, Valenziano, L, Vallée, D, VAN DER VLIS, M, VAN LEEUWEN, F, Vanel, J, VAN TENT, B, Varis, J, Vassallo, E, Vescovi, C, Vezzu, F, Vibert, D, Vielva, P, Vierra, J, Villa, F, Vittorio, N, Vuerli, C, Wade, L, Walker, A, Wandelt, B, Watson, C, Werner, D, White, M, White, S, Wilkinson, A, Wilson, P, Woodcraft, A, Yoffo, B, Yun, M, Yurchenko, V, Yvon, D, Zhang, B, Zimmermann, O, Zonca, A, Zorita, D, TAUBER J. A, MANDOLESI N, PUGET J. L, BANOS T, BERSANELLI M, BOUCHET F. R, BUTLER R. C, CHARRA J, CRONE G, DODSWORTH J, EFSTATHIOU G, GISPERT R, GUYOT G, GREGORIO A, JUILLET J. J, LAMARRE J. M, LAUREIJS R. J, LAWRENCE C. R, NØRGAARD NIELSEN H. U, PASSVOGEL T, REIX J. M, TEXIER D, VIBERT L, ZACCHEI A, ADE P. A. R, AGHANIM N, AJA B, ALIPPI E, ALOY L, ARMAND P, ARNAUD M, ARONDEL A, ARREOLA VILLANUEVA A, ARTAL E, ARTINA E, ARTS A, ASHDOWN M, AUMONT J, AZZARO M, BACCHETTA A, BACCIGALUPI C, BAKER M, BALASINI M, BALBI A, BANDAY A. J, BARBIER G, BARREIRO R. B, BARTELMANN M, BATTAGLIA P, BATTANER E, BENABED K, BENEY J. L, BENEYTON R, BENNETT K, BENOIT A, BERNARD J. P, BHANDARI P, BHATIA R, BIGGI M, BIGGINS R, BILLIG G, BLANC Y, BLAVOT H, BOCK J. J, BONALDI A, BOND R, BONIS J, BORDERS J, BORRILL J, BOSCHINI L, BOULANGER F, BOUVIER J, BOUZIT M, BOWMAN R, BRÉELLE E, BRADSHAW T, BRAGHIN M, BREMER M, BRIENZA, DANIELE, BROSZKIEWICZ D, BURIGANA C, BURKHALTER M, CABELLA, PAOLO, CAFFERTY T, CAIROLA M, CAMINADE S, CAMUS P, CANTALUPO C. M, CAPPELLINI B, CARDOSO J. F, CARR R, CATALANO, Andrea, CAYÓN L, CESA M, CHAIGNEAU M, CHALLINOR A, CHAMBALLU A, CHAMBELLAND J. P, CHARRA M, CHIANG L. Y, CHLEWICKI G, CHRISTENSEN P. R, CHURCH S, CIANCIETTA E, CIBRARIO M, CIZERON R, CLEMENTS D, COLLAUDIN B, COLLEY J. M, COLOMBI S, COLOMBO A, COLOMBO F, CORRE O, COUCHOT F, COUGRAND B, COULAIS A, COUZIN P, CRANE B, CRILL B, CROOK M, CRUMB D, CUTTAIA F, DÖRL U, DA SILVA P, DADDATO R, DAMASIO C, DANESE L, D'AQUINO G, D'ARCANGELO O, DASSAS K, DAVIES R. D, DAVIES W, DAVIS R. J, DE BERNARDIS, Paolo, DE CHAMBURE D, DE GASPERIS G, DE LA FUENTE M. L, DE PACO P, DE ROSA A, DE TROIA, Grazia, DE ZOTTI G, DEHAMME M, DELABROUILLE J, DELOUIS J. M, DÉSERT F. X, DI GIROLAMO G, DICKINSON C, DOELLING E, DOLAG K, DOMKEN I, DOUSPIS M, DOYLE D, DU S, DUBRUEL D, DUFOUR C, DUMESNIL C, DUPAC X, DURET P, EDER C, ELFVING A, ENLIN T. A, ENG P, ENGLISH K, ERIKSEN H. K, ESTARIA P, FALVELLA M. C, FERRARI F, FINELLI F, FISHMAN A, FOGLIANI S, FOLEY S, FONSECA A, FORMA G, FORNI O, FOSALBA P, FOURMOND J. J, FRAILIS M, FRANCESCHET C, FRANCESCHI E, FRANÇOIS S, FRERKING M, GÓMEZ REÑASCO M. F, GÓRSKI K. M, GAIER T. C, GALEOTTA S, GANGA K, GARCÍA LÁZARO J, GARNICA A, GASPARD M, GAVILA E, GIARD M, GIARDINO G, GIENGER G, GIRAUD HERAUD Y, GLORIAN J. M, GRIFFIN M, GRUPPUSO A, GUGLIELMI L, GUICHON D, GUILLAUME B, GUILLOUET P, HAISSINSKI J, HANSEN F. K, HARDY J, HARRISON D, HAZELL A, HECHLER M, HECKENAUER V, HEINZER D, HELL R, HENROT VERSILLÉ S, HERNÁNDEZ MONTEAGUDO C, HERRANZ D, HERREROS J. M, HERVIER V, HESKE A, HEURTEL A, HILDEBRANDT S. R, HILLS R, HIVON E, HOBSON M, HOLLERT D, HOLMES W, HORNSTRUP A, HOVEST W, HOYLAND R. J, HUEY G, HUFFENBERGER K. M, HUGHES N, ISRAELSSON U, JACKSON B, JAFFE A, JAFFE T. R, JAGEMANN T, JESSEN N. C, JEWELL J, JONES W, JUVELA M, KAPLAN J, KARLMAN P, KECK F, KEIHÄNEN E, KING M, KISNER T. S, KLETZKINE P, KNEISSL R, KNOCHE J, KNOX L, KOCH T, KRASSENBURG M, KURKI SUONIO H, LÄHTEENMÄKI A, LAGACHE G, LAGORIO E, LAMI P, LANDE J, LANGE A, LANGLET F, LAPINI R, LAPOLLA M, LASENBY A, LE JEUNE M, LEAHY J. P, LEFEBVRE M, LEGRAND F, LE MEUR G, LEONARDI R, LERICHE B, LEROY C, LEUTENEGGER P, LEVIN S. M, LILJE P. B, LINDENSMITH C, LINDEN VØRNLE M, LOC A, LONGVAL Y, LUBIN P. M, LUCHIK T, LUTHOLD I, MACIAS PEREZ J. F, MACIASZEK T, MACTAVISH C, MADDEN S, MAFFEI B, MAGNEVILLE C, MAINO D, MAMBRETTI A, MANSOUX B, MARCHIORO D, MARIS M, MARLIANI F, MARRUCHO J. C, MARTÍ CANALES J, MARTÍNEZ GONZÁLEZ E, MARTÍN POLEGRE A, MARTIN P, MARTY C, MARTY W, MASI, Silvia, MASSARDI M, MATARRESE S, MATTHAI F, MAZZOTTA P, MCDONALD A, MCGRATH P, MEDIAVILLA A, MEINHOLD P. R, MÉLIN J. B, MELOT F, MENDES L, MENNELLA A, MERVIER C, MESLIER L, MICCOLIS M, MIVILLE DESCHENES M. A, MONETI A, MONTET D, MONTIER L, MORA J, MORGANTE G, MORIGI G, MORINAUD G, MORISSET N, MORTLOCK D, MOTTET S, MULDER J, MUNSHI D, MURPHY A, MURPHY P, MUSI P, NARBONNE J, NASELSKY P, NASH A, NATI, FEDERICO, NATOLI P, NETTERFIELD B, NEWELL J, NEXON M, NICOLAS C, NIELSEN P. H, NINANE N, NOVIELLO F, NOVIKOV D, NOVIKOV I, O'DWYER I. J, OLDEMAN P, OLIVIER P, OUCHET L, OXBORROW C. A, PÉREZ CUEVAS L, PAGAN L, PAINE C, PAJOT F, PALADINI R, PANCHER F, PANH J, PARKS G, PARNAUDEAU P, PARTRIDGE B, PARVIN B, PASCUAL J. P, PASIAN F, PEARSON D. P, PEARSON T, PECORA M, PERDEREAU O, PEROTTO L, PERROTTA F, PIACENTINI, Francesco, PIAT M, PIERPAOLI E, PIERSANTI O, PLAIGE E, PLASZCZYNSKI S, PLATANIA P, POINTECOUTEAU E, POLENTA, GIANLUCA, PONTHIEU N, POPA L, POULLEAU G, POUTANEN T, PRÉZEAU G, PRADELL L, PRINA M, PRUNET S, RACHEN J. P, RAMBAUD D, RAME F, RASMUSSEN I, RAUTAKOSKI J, REACH W. T, REBOLO R, REINECKE M, REITER J, RENAULT C, RICCIARDI, Sara, RIDEAU P, RILLER T, RISTORCELLI I, RITI J. B, ROCHA G, ROCHE Y, PONS R, ROHLFS R, ROMERO D, ROOSE S, ROSSET C, ROUBEROL S, ROWAN ROBINSON M, RUBIÑO MARTÍN J. A, RUSCONI P, RUSHOLME B, SALAMA M, SALERNO E, SANDRI M, SANTOS D, SANZ J. L, SAUTER L, SAUVAGE F, SAVINI, Giorgio, SCHMELZEL M, SCHNORHK A, SCHWARZ W, SCOTT D, SEIFFERT M. D, SHELLARD P, SHIH C, SIAS M, SILK J. I, SILVESTRI R, SIPPEL R, SMOOT G. F, STARCK J. L, STASSI P, STERNBERG J, STIVOLI, federico, STOLYAROV V, STOMPOR R, STRINGHETTI L, STROMMEN D, STUTE T, SUDIWALA R, SUGIMURA R, SUNYAEV R, SYGNET J. F, TÜRLER M, TADDEI E, TALLON J, TAMIATTO C, TAURIGNA M, TAYLOR D, TERENZI L, THUEREY S, TILLIS J, TOFANI G, TOFFOLATTI L, TOMMASI E, TOMASI M, TONAZZINI E, TORRE J. P, TOSTI S, TOUZE F, TRISTRAM M, TUOVINEN J, TUTTLEBEE M, UMANA G, VALENZIANO L, VALLÉE D, VAN DER VLIS M, VAN LEEUWEN F, VANEL J. C, VAN TENT B, VARIS J, VASSALLO E, VESCOVI C, VEZZU F, VIBERT D, VIELVA P, VIERRA J, VILLA F, VITTORIO N, VUERLI C, WADE L. A, WALKER A. R, WANDELT B. D, WATSON C, WERNER D, WHITE M, WHITE S. D. M, WILKINSON A, WILSON P, WOODCRAFT A, YOFFO B, YUN M, YURCHENKO V, YVON D, ZHANG B, ZIMMERMANN O, ZONCA A, ZORITA D., Tauber, J, Mandolesi, N, Puget, J, Banos, T, Bersanelli, M, Bouchet, F, Butler, R, Charra, J, Crone, G, Dodsworth, J, Efstathiou, G, Gispert, R, Guyot, G, Gregorio, A, Juillet, J, Lamarre, J, Laureijs, R, Lawrence, C, NØRGAARD NIELSEN, H, Passvogel, T, Reix, J, Texier, D, Vibert, L, Zacchei, A, Ade, P, Aghanim, N, Aja, B, Alippi, E, Aloy, L, Armand, P, Arnaud, M, Arondel, A, ARREOLA VILLANUEVA, A, Artal, E, Artina, E, Arts, A, Ashdown, M, Aumont, J, Azzaro, M, Bacchetta, A, Baccigalupi, C, Baker, M, Balasini, M, Balbi, A, Banday, A, Barbier, G, Barreiro, R, Bartelmann, M, Battaglia, P, Battaner, E, Benabed, K, Beney, J, Beneyton, R, Bennett, K, Benoit, A, Bernard, J, Bhandari, P, Bhatia, R, Biggi, M, Biggins, R, Billig, G, Blanc, Y, Blavot, H, Bock, J, Bonaldi, A, Bond, R, Bonis, J, Borders, J, Borrill, J, Boschini, L, Boulanger, F, Bouvier, J, Bouzit, M, Bowman, R, Bréelle, E, Bradshaw, T, Braghin, M, Bremer, M, Brienza, D, Broszkiewicz, D, Burigana, C, Burkhalter, M, Cabella, P, Cafferty, T, Cairola, M, Caminade, S, Camus, P, Cantalupo, C, Cappellini, B, Cardoso, J, Carr, R, Catalano, A, Cayón, L, Cesa, M, Chaigneau, M, Challinor, A, Chamballu, A, Chambelland, J, Charra, M, Chiang, L, Chlewicki, G, Christensen, P, Church, S, Ciancietta, E, Cibrario, M, Cizeron, R, Clements, D, Collaudin, B, Colley, J, Colombi, S, Colombo, A, Colombo, F, Corre, O, Couchot, F, Cougrand, B, Coulais, A, Couzin, P, Crane, B, Crill, B, Crook, M, Crumb, D, Cuttaia, F, Dörl, U, DA SILVA, P, Daddato, R, Damasio, C, Danese, L, D'Aquino, G, D'Arcangelo, O, Dassas, K, Davies, R, Davies, W, Davis, R, DE BERNARDIS, P, DE CHAMBURE, D, DE GASPERIS, G, DE LA FUENTE, M, DE PACO, P, DE ROSA, A, DE TROIA, G, DE ZOTTI, G, Dehamme, M, Delabrouille, J, Delouis, J, Désert, F, DI GIROLAMO, G, Dickinson, C, Doelling, E, Dolag, K, Domken, I, Douspis, M, Doyle, D, Du, S, Dubruel, D, Dufour, C, Dumesnil, C, Dupac, X, Duret, P, Eder, C, Elfving, A, Enlin, T, Eng, P, English, K, Eriksen, H, Estaria, P, Falvella, M, Ferrari, F, Finelli, F, Fishman, A, Fogliani, S, Foley, S, Fonseca, A, Forma, G, Forni, O, Fosalba, P, Fourmond, J, Frailis, M, Franceschet, C, Franceschi, E, François, S, Frerking, M, GÓMEZ REÑASCO, M, Górski, K, Gaier, T, Galeotta, S, Ganga, K, GARCÍA LÁZARO, J, Garnica, A, Gaspard, M, Gavila, E, Giard, M, Giardino, G, Gienger, G, GIRAUD HERAUD, Y, Glorian, J, Griffin, M, Gruppuso, A, Guglielmi, L, Guichon, D, Guillaume, B, Guillouet, P, Haissinski, J, Hansen, F, Hardy, J, Harrison, D, Hazell, A, Hechler, M, Heckenauer, V, Heinzer, D, Hell, R, HENROT VERSILLÉ, S, HERNÁNDEZ MONTEAGUDO, C, Herranz, D, Herreros, J, Hervier, V, Heske, A, Heurtel, A, Hildebrandt, S, Hills, R, Hivon, E, Hobson, M, Hollert, D, Holmes, W, Hornstrup, A, Hovest, W, Hoyland, R, Huey, G, Huffenberger, K, Hughes, N, Israelsson, U, Jackson, B, Jaffe, A, Jaffe, T, Jagemann, T, Jessen, N, Jewell, J, Jones, W, Juvela, M, Kaplan, J, Karlman, P, Keck, F, Keihänen, E, King, M, Kisner, T, Kletzkine, P, Kneissl, R, Knoche, J, Knox, L, Koch, T, Krassenburg, M, KURKI SUONIO, H, Lähteenmäki, A, Lagache, G, Lagorio, E, Lami, P, Lande, J, Lange, A, Langlet, F, Lapini, R, Lapolla, M, Lasenby, A, LE JEUNE, M, Leahy, J, Lefebvre, M, Legrand, F, LE MEUR, G, Leonardi, R, Leriche, B, Leroy, C, Leutenegger, P, Levin, S, Lilje, P, Lindensmith, C, LINDEN VØRNLE, M, Loc, A, Longval, Y, Lubin, P, Luchik, T, Luthold, I, MACIAS PEREZ, J, Maciaszek, T, Mactavish, C, Madden, S, Maffei, B, Magneville, C, Maino, D, Mambretti, A, Mansoux, B, Marchioro, D, Maris, M, Marliani, F, Marrucho, J, MARTÍ CANALES, J, MARTÍNEZ GONZÁLEZ, E, MARTÍN POLEGRE, A, Martin, P, Marty, C, Marty, W, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, Mcdonald, A, Mcgrath, P, Mediavilla, A, Meinhold, P, Mélin, J, Melot, F, Mendes, L, Mennella, A, Mervier, C, Meslier, L, Miccolis, M, MIVILLE DESCHENES, M, Moneti, A, Montet, D, Montier, L, Mora, J, Morgante, G, Morigi, G, Morinaud, G, Morisset, N, Mortlock, D, Mottet, S, Mulder, J, Munshi, D, Murphy, A, Murphy, P, Musi, P, Narbonne, J, Naselsky, P, Nash, A, Nati, F, Natoli, P, Netterfield, B, Newell, J, Nexon, M, Nicolas, C, Nielsen, P, Ninane, N, Noviello, F, Novikov, D, Novikov, I, O'Dwyer, I, Oldeman, P, Olivier, P, Ouchet, L, Oxborrow, C, PÉREZ CUEVAS, L, Pagan, L, Paine, C, Pajot, F, Paladini, R, Pancher, F, Panh, J, Parks, G, Parnaudeau, P, Partridge, B, Parvin, B, Pascual, J, Pasian, F, Pearson, D, Pearson, T, Pecora, M, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Piersanti, O, Plaige, E, Plaszczynski, S, Platania, P, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poulleau, G, Poutanen, T, Prézeau, G, Pradell, L, Prina, M, Prunet, S, Rachen, J, Rambaud, D, Rame, F, Rasmussen, I, Rautakoski, J, Reach, W, Rebolo, R, Reinecke, M, Reiter, J, Renault, C, Ricciardi, S, Rideau, P, Riller, T, Ristorcelli, I, Riti, J, Rocha, G, Roche, Y, Pons, R, Rohlfs, R, Romero, D, Roose, S, Rosset, C, Rouberol, S, ROWAN ROBINSON, M, RUBIÑO MARTÍN, J, Rusconi, P, Rusholme, B, Salama, M, Salerno, E, Sandri, M, Santos, D, Sanz, J, Sauter, L, Sauvage, F, Savini, G, Schmelzel, M, Schnorhk, A, Schwarz, W, Scott, D, Seiffert, M, Shellard, P, Shih, C, Sias, M, Silk, J, Silvestri, R, Sippel, R, Smoot, G, Starck, J, Stassi, P, Sternberg, J, Stivoli, F, Stolyarov, V, Stompor, R, Stringhetti, L, Strommen, D, Stute, T, Sudiwala, R, Sugimura, R, Sunyaev, R, Sygnet, J, Türler, M, Taddei, E, Tallon, J, Tamiatto, C, Taurigna, M, Taylor, D, Terenzi, L, Thuerey, S, Tillis, J, Tofani, G, Toffolatti, L, Tommasi, E, Tomasi, M, Tonazzini, E, Torre, J, Tosti, S, Touze, F, Tristram, M, Tuovinen, J, Tuttlebee, M, Umana, G, Valenziano, L, Vallée, D, VAN DER VLIS, M, VAN LEEUWEN, F, Vanel, J, VAN TENT, B, Varis, J, Vassallo, E, Vescovi, C, Vezzu, F, Vibert, D, Vielva, P, Vierra, J, Villa, F, Vittorio, N, Vuerli, C, Wade, L, Walker, A, Wandelt, B, Watson, C, Werner, D, White, M, White, S, Wilkinson, A, Wilson, P, Woodcraft, A, Yoffo, B, Yun, M, Yurchenko, V, Yvon, D, Zhang, B, Zimmermann, O, Zonca, A, Zorita, D, TAUBER J. A, MANDOLESI N, PUGET J. L, BANOS T, BERSANELLI M, BOUCHET F. R, BUTLER R. C, CHARRA J, CRONE G, DODSWORTH J, EFSTATHIOU G, GISPERT R, GUYOT G, GREGORIO A, JUILLET J. J, LAMARRE J. M, LAUREIJS R. J, LAWRENCE C. R, NØRGAARD NIELSEN H. U, PASSVOGEL T, REIX J. M, TEXIER D, VIBERT L, ZACCHEI A, ADE P. A. R, AGHANIM N, AJA B, ALIPPI E, ALOY L, ARMAND P, ARNAUD M, ARONDEL A, ARREOLA VILLANUEVA A, ARTAL E, ARTINA E, ARTS A, ASHDOWN M, AUMONT J, AZZARO M, BACCHETTA A, BACCIGALUPI C, BAKER M, BALASINI M, BALBI A, BANDAY A. J, BARBIER G, BARREIRO R. B, BARTELMANN M, BATTAGLIA P, BATTANER E, BENABED K, BENEY J. L, BENEYTON R, BENNETT K, BENOIT A, BERNARD J. P, BHANDARI P, BHATIA R, BIGGI M, BIGGINS R, BILLIG G, BLANC Y, BLAVOT H, BOCK J. 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T, REBOLO R, REINECKE M, REITER J, RENAULT C, RICCIARDI, Sara, RIDEAU P, RILLER T, RISTORCELLI I, RITI J. B, ROCHA G, ROCHE Y, PONS R, ROHLFS R, ROMERO D, ROOSE S, ROSSET C, ROUBEROL S, ROWAN ROBINSON M, RUBIÑO MARTÍN J. A, RUSCONI P, RUSHOLME B, SALAMA M, SALERNO E, SANDRI M, SANTOS D, SANZ J. L, SAUTER L, SAUVAGE F, SAVINI, Giorgio, SCHMELZEL M, SCHNORHK A, SCHWARZ W, SCOTT D, SEIFFERT M. D, SHELLARD P, SHIH C, SIAS M, SILK J. I, SILVESTRI R, SIPPEL R, SMOOT G. F, STARCK J. L, STASSI P, STERNBERG J, STIVOLI, federico, STOLYAROV V, STOMPOR R, STRINGHETTI L, STROMMEN D, STUTE T, SUDIWALA R, SUGIMURA R, SUNYAEV R, SYGNET J. F, TÜRLER M, TADDEI E, TALLON J, TAMIATTO C, TAURIGNA M, TAYLOR D, TERENZI L, THUEREY S, TILLIS J, TOFANI G, TOFFOLATTI L, TOMMASI E, TOMASI M, TONAZZINI E, TORRE J. P, TOSTI S, TOUZE F, TRISTRAM M, TUOVINEN J, TUTTLEBEE M, UMANA G, VALENZIANO L, VALLÉE D, VAN DER VLIS M, VAN LEEUWEN F, VANEL J. C, VAN TENT B, VARIS J, VASSALLO E, VESCOVI C, VEZZU F, VIBERT D, VIELVA P, VIERRA J, VILLA F, VITTORIO N, VUERLI C, WADE L. A, WALKER A. R, WANDELT B. D, WATSON C, WERNER D, WHITE M, WHITE S. D. M, WILKINSON A, WILSON P, WOODCRAFT A, YOFFO B, YUN M, YURCHENKO V, YVON D, ZHANG B, ZIMMERMANN O, ZONCA A, and ZORITA D.
Abstract: The European Space Agency's Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies of the CMB over the whole sky, with unprecedented sensitivity (${{\Delta T}\over T}$ ~ 2 × 10-6) and angular resolution (~5 arcmin). Planck will provide a major source of information relevant to many fundamental cosmological problems and will test current theories of the early evolution of the Universe and the origin of structure. It will also address a wide range of areas of astrophysical research related to the Milky Way as well as external galaxies and clusters of galaxies. The ability of Planck to measure polarization across a wide frequency range (30-350 GHz), with high precision and accuracy, and over the whole sky, will provide unique insight, not only into specific cosmological questions, but also into the properties of the interstellar medium. This paper is part of a series which describes the technical capabilities of the Planck scientific payload. It is based on the knowledge gathered during the on-ground calibration campaigns of the major subsystems, principally its telescope and its two scientific instruments, and of tests at fully integrated satellite level. It represents the best estimate before launch of the technical performance that the satellite and its payload will achieve in flight. In this paper, we summarise the main elements of the payload performance, which is described in detail in the accompanying papers. In addition, we describe the satellite performance elements which are most relevant for science, and provide an overview of the plans for scientific operations and data analysis.
Published: 2010

15. Planck early results. II. The Thermal performance of Planck

Author: Poutanen, T., Natoli, P., Polenta, G., Bréelle, E., Bucher, M., Cardoso, J.-F., Catalano, A., Delabrouille, J., Ganga, K., Giraud-Héraud, Y., Patanchon, G., Piat, M., Rosset, C., Smoot, G.F., Stompor, R., Ashdown, M., Hobson, M., Lasenby, A., Stolyarov, V., Bhatia, R., Kneissl, R., Bond, J.R., Miville-Deschênes, M.-A., MacIaszek, T., Banday, A.J., Bernard, J.-P., Forni, O., Giard, M., Leroy, C., Montier, L., Pointecouteau, E., Ristorcelli, I., Bock, J.J., Doré, O., Helou, G., Hildebrandt, S.R., Prézeau, G., Rocha, G., Seiffert, M.D., Lilje, P.B., Challinor, A., Shellard, P., Starck, J.-L., Yvon, D., Hornstrup, Allan, Toffolatti, L., Netterfield, C.B., Scott, D., Juvela, M., Keihänen, E., Keskitalo, R., Kurki-Suonio, H., Chiang, C., Jones, W.C., Cayón, L., Knox, L., Leonardi, R., Lubin, P.M., Meinhold, P.R., Zonca, A., Wandelt, B.D., Matarrese, S., De Bernardis, P., Masi, S., Melchiorri, A., Piacentini, F., Bersanelli, M., Maino, D., Mennella, A., Tomasi, M., Gregorio, A., Balbi, A., Cabella, P., De Gasperis, G., Mazzotta, P., Vittorio, N., Christensen, P.R., Naselsky, P., Rebolo, R., Rubiño-Martín, J.A., Dupac, X., Mendes, L., Baker, M., Foley, S., Watson, C., Damasio, C., Giardino, G., Laureijs, R.J., Tauber, J.A., Bonaldi, A., Frailis, M., Galeotta, S., Maris, M., Pasian, F., Zacchei, A., Burigana, C., Butler, R.C., Cuttaia, F., De Rosa, A., Finelli, F., Franceschi, E., Gruppuso, A., Mandolesi, N., Morgante, G., Ricciardi, S., Sandri, M., Terenzi, L., Valenziano, L., Villa, F., Cappellini, B., Donzelli, S., Stivoli, F., Guyot, G., Désert, F.-X., Morisset, N., Chamballu, A., Clements, D.L., Jaffe, A.H., Mortlock, D., Novikov, D., McGehee, P., Rusholme, B., Benoît, A., Camus, P., Aghanim, N., Aumont, J., Charra, J., Charra, M., Douspis, M., Fourmond, J.-J., Lagache, G., Lami, P., Pajot, F., Ponthieu, N., Puget, J.-L., Torre, J.-P., Vibert, L., Benabed, K., Bouchet, F.R., Colombi, S., Delouis, J.-M., Hivon, E., Moneti, A., Prunet, S., Sygnet, J.-F., Fosalba, P., Chiang, L.-Y., Efstathiou, G., Gratton, S., Harrison, D., Munshi, D., Eriksen, H.K., Hoyland, R.J., Barreiro, R.B., Herranz, D., López-Caniego, M., Martínez-González, E., Vielva, P., Platania, P., Bhandari, P., Borders, J., Bowman, B., Chambelland, J.P., Crill, B.P., Górski, K.M., Holmes, W.A., Israelsson, U., Lawrence, C.R., Lee, R., Mora, J., Nash, A., O'Dwyer, I.J., Pearson, D., Prina, M., Wade, L.A., Wilson, P., Zhang, B., Davies, R.D., Davis, R.J., Maffei, B., Wilkinson, A., MacTavish, C.J., Coulais, A., Lamarre, J.-M., Arnaud, M., MacÍas-Pérez, J.F., Melot, F., Perotto, L., Renault, C., Santos, D., Stassi, P., Couchot, F., Filliard, C., Henrot-Versillé, S., Lavabre, A., Perdereau, O., Plaszczynski, S., Tristram, M., Borrill, J., Cantalupo, C.M., Kisner, T.S., Dolag, K., Dörl, U., Enßlin, T.A., Hernández-Monteagudo, C., Hovest, W., Matthai, F., Rachen, J.P., Reinecke, M., Riller, T., White, S.D.M., Tuovinen, J., Murphy, A., Novikov, I., Savini, G., Bradshaw, T., Crook, M., Baccigalupi, C., Danese, L., González-Nuevo, J., Leach, S., Perrotta, F., Mann, R., Ade, P.A.R., Sudiwala, R., Osborne, S., Collaudin, B., Gavila, E., Schaefer, B.M., Battaner, E., Huffenberger, K.M., Universidad de Cantabria, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique (ex SAP) (DAP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), HELFA - Hélium : du fondamental aux applications, Institut Néel (NEEL), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS), Cryo - Cryogénie, Laboratoire Traitement et Communication de l'Information (LTCI), Télécom ParisTech-Institut Mines-Télécom [Paris] (IMT)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Thales Alenia Space (TAS), THALES, Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Centre National d'Études Spatiales [Toulouse] (CNES), Laboratoire de Recherche en Informatique (LRI), Université Paris-Sud - Paris 11 (UP11)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS), PLANCK, Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Hélium : du fondamental aux applications (HELFA), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Cryogénie (Cryo), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG ), Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Department of Physics, Helsinki Institute of Physics, Hélium : du fondamental aux applications (NEEL - HELFA), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Cryogénie (NEEL - Cryo), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoit, A., Bernard, J. P., Bersanelli, M., Bhandari, P., Bhatia, R., Bock, J. J., Bonaldi, A., Bond, J. R., Borders, J., Borrill, J., Bouchet, F. R., Bowman, B., Bradshaw, T., Breelle, E., Bucher, M., Burigana, C., Butler, R. C., Cabella, P., Camus, P., Cantalupo, C. M., Cappellini, B., Cardoso, J. F., Catalano, A., Cayon, L., Challinor, A., Chamballu, A., Chambelland, J. P., Charra, J., Charra, M., Y. Chiang, L., Chiang, C., Christensen, P. R., Clements, D. L., Collaudin, B., Colombi, S., Couchot, F., Coulais, A., Crill, B. P., Crook, M., Cuttaia, F., Damasio, C., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Gasperis, G., de Rosa, A., Delabrouille, J., Delouis, J. M., Desert, F. X., Doerl, U., Dolag, K., Donzelli, S., Dore, O., Douspis, M., Dupac, X., Efstathiou, G., Enslin, T. A., Eriksen, H. K., Finelli, F., Foley, S., Forni, O., Fosalba, P., Fourmond, J. J., Frailis, M., Franceschi, E., Galeotta, S., Ganga, K., Gavila, E., Giard, M., Giardino, G., Giraud Heraud, Y., Gonzalez Nuevo, J., Gorski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Guyot, G., Harrison, D., Helou, G., Henrot Versille, S., Hernandez Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Hoyland, R. J., Huffenberger, K. M., Israelsson, U., Jaffe, A. H., Jones, W. C., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knox, L., Kurki Suonio, H., Lagache, G., Lamarre, J. M., Lami, P., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leonardi, R., Leroy, C., Lilje, P. B., Lopez Caniego, M., Lubin, P. M., Macias Perez, J. F., Maciaszek, T., Mactavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martinez Gonzalez, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Mcgehee, P., Meinhold, P. R., Melchiorri, A., Melot, F., Mendes, L., Mennella, A., Miville Deschenes, M. A., Moneti, A., Montier, L., Mora, J., Morgante, G., Morisset, N., Mortlock, D., Munshi, D., Murphy, A., Naselsky, P., Nash, A., Natoli, P., Netterfield, C. B., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Pajot, F., Pasian, F., Patanchon, G., Pearson, D., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Poutanen, T., Prezeau, G., Prina, M., Prunet, S., Puget, J. L., Rachen, J. P., Rebolo, R., Reinecke, M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rubiino Martin, J. A., Rusholme, B., Sandri, M., Santos, D., Schaefer, B. M., Scott, D., Seiffert, M. D., Shellard, P., Smoot, G. F., Starck, J. L., Stassi, P., Stivoli, F., Stolyarov, V., Stompor, R., Sudiwala, R., Sygnet, J. F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Torre, J. P., Tristram, M., Tuovinen, J., Valenziano, L., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, C., White, S. D. M., Wilkinson, A., Wilson, P., Yvon, D., Zacchei, A., Zhang, B., and Zonca, A.
Subjects: instruments [space vehicles], Experimental Physics, cosmic background radiation, Cosmic background radiation, 7. Clean energy, 01 natural sciences, law.invention, law, CMB physics, Space vehicles: instruments, Instrumentation: detectors, 010303 astronomy & astrophysics, QB, detectors, Physics, instrumentation, Planck ESA mission, instruments, symbols, Astrophysics - Instrumentation and Methods for Astrophysics, Cryostat, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Radiative cooling, space vehicles, space vehicles: instruments, instrumentation: detectors, education, FOS: Physical sciences, Cosmic ray, Cosmic backround radiation, Primary mirror, Telescope, symbols.namesake, Optics, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Instrumentation, Space vehicles, Planck, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), detectors [instrumentation], Spacecraft, business.industry, Bolometer, Astronomy and Astrophysics, 115 Astronomy, Space science, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Space and Planetary Science, business
Abstract: 31 páginas, 36 figuras, 11 tablas.-- Planck Collaboration: et al., The performance of the Planck instruments in space is enabled by their low operating temperatures, 20 K for LFI and 0.1 K for HFI, achieved through a combination of passive radiative cooling and three active mechanical coolers. The scientific requirement for very broad frequency coverage led to two detector technologies with widely different temperature and cooling needs. Active coolers could satisfy these needs; a helium cryostat, as used by previous cryogenic space missions (IRAS, COBE, ISO, Spitzer, AKARI), could not. Radiative cooling is provided by three V-groove radiators and a large telescope baffle. The active coolers are a hydrogen sorption cooler (, The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and DEISA (EU).
Published: 2011

16. Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance

Author: Bartlett, J.G., Bréelle, E., Bucher, M., Cardoso, J.-F., Catalano, A., Cressiot, C., Delabrouille, J., Ganga, K., Giraud-Héraud, Y., Kaplan, J., Patanchon, G., Piat, M., Rosset, C., Roudier, G., Stompor, R., Ashdown, M., Hills, R., Hobson, M., Lasenby, A., Stolyarov, V., Bhatia, R., Kneissl, R., Bond, J.R., Miville-Deschênes, M.-A., MacIaszek, T., Banday, A.J., Bernard, J.-P., Forni, O., Giard, M., Leroy, C., Montier, L., Pointecouteau, E., Pons, R., Ristorcelli, I., Bock, J.J., Doré, O., Helou, G., Hildebrandt, S.R., Matsumura, T., Pearson, T.J., Prézeau, G., Rocha, G., Challinor, A., Shellard, P., Melin, J.-B., Starck, J.-L., Yvon, D., Nørgaard-Nielsen, Hans Ulrik, Netterfield, C.B., Chiang, C., Jones, W.C., Knox, L., Wandelt, B.D., De Bernardis, P., Masi, S., Nati, F., Piacentini, F., Bersanelli, M., Tauber, J.A., Zacchei, A., Mandolesi, N., Guyot, G., Désert, F.-X., Chamballu, A., Clements, D.L., Jaffe, A.H., Mortlock, D., Novikov, D., Rowan-Robinson, M., Chary, R.-R., Lange, A.E., McGehee, P., Rusholme, B., Benoît, A., Camus, P., Aghanim, N., Aumont, J., Boulanger, F., Charra, J., Charra, M., Dole, H., Douspis, M., Eng, P., Fourmond, J.-J., Gispert, R., Lagache, G., Lami, P., Leriche, B., Longval, Y., Mercier, C., Noviello, F., Pajot, F., Ponthieu, N., Puget, J.-L., Torre, J.-P., Vibert, L., Benabed, K., Bouchet, F.R., Colombi, S., Delouis, J.-M., Hivon, E., Moneti, A., Prunet, S., Sygnet, J.-F., Fosalba, P., Wiesemeyer, H., Thum, C., Efstathiou, G., Gratton, S., Harrison, D., Van Leeuwen, F., Crill, B.P., Górski, K.M., Holmes, W.A., Lawrence, C.R., Paine, C., Wade, L.A., Maffei, B., MacTavish, C.J., Coulais, A., Lamarre, J.-M., Arnaud, M., Vibert, D., Girard, D., MacÍas-Pérez, J.F., Perotto, L., Renault, C., Santos, D., Stassi, P., Ansari, R., Couchot, F., Filliard, C., Haissinski, J., Henrot-Versillé, S., Lavabre, A., Mansoux, B., Perdereau, O., Plaszczynski, S., Touze, F., Tristram, M., Borrill, J., Bartelmann, M., Dolag, K., Hernández-Monteagudo, C., Sunyaev, R., White, S.D.M., Murphy, A., Peacocke, T., Yurchenko, V., Savini, G., Bradshaw, T., Crook, M., Mann, R., Ade, P.A.R., Griffin, M., North, C., Spencer, L., Sudiwala, R., Woodcraft, A., Church, S., Osborne, S., Schaefer, B.M., Reach, W.T., Battaner, E., Huffenberger, K.M., Hfi Core Team, P, Ade, P, Aghanim, N, Ansari, R, Arnaud, M, Ashdown, M, Aumont, J, Banday, A, Bartelmann, M, Bartlett, J, Battaner, E, Benabed, K, Benoit, A, Bernard, J, Bersanelli, M, Bhatia, R, Bock, J, Bond, J, Borrill, J, Bouchet, F, Boulanger, F, Bradshaw, T, Breelle, E, Bucher, M, Camus, P, Cardoso, J, Catalano, A, Challinor, A, Chamballu, A, Charra, J, Charra, M, Chary, R, Chiang, C, Church, S, Clements, D, Colombi, S, Couchot, F, Coulais, A, Cressiot, C, Crill, B, Crook, M, De Bernardis, P, Delabrouille, J, Delouis, J, Desert, F, Dolag, K, Dole, H, Dore, O, Douspis, M, Efstathiou, G, Eng, P, Filliard, C, Forni, O, Fosalba, P, Fourmond, J, Ganga, K, Giard, M, Girard, D, Giraud-Heraud, Y, Gispert, R, Gorski, K, Gratton, S, Griffin, M, Guyot, G, Haissinski, J, Harrison, D, Helou, G, Henrot-Versille, S, Hernandez-Monteagudo, C, Hildebrandt, S, Hills, R, Hivon, E, Hobson, M, Holmes, W, Huffenberger, K, Jaffe, A, Jones, W, Kaplan, J, Kneissl, R, Knox, L, Lagache, G, Lamarre, J, Lami, P, Lange, A, Lasenby, A, Lavabre, A, Lawrence, C, Leriche, B, Leroy, C, Longval, Y, Macias-Perez, J, Maciaszek, T, Mactavish, C, Maffei, B, Mandolesi, N, Mann, R, Mansoux, B, Masi, S, Matsumura, T, Mcgehee, P, Melin, J, Mercier, C, Miville-Deschenes, M, Moneti, A, Montier, L, Mortlock, D, Murphy, A, Nati, F, Netterfield, C, Norgaard-Nielsen, H, Nørgaard-Nielsen, H, North, C, Noviello, F, Novikov, D, Osborne, S, Paine, C, Pajot, F, Patanchon, G, Peacocke, T, Pearson, T, Perdereau, O, Perotto, L, Piacentini, F, Piat, M, Plaszczynski, S, Pointecouteau, E, Pons, R, Ponthieu, N, Prezeau, G, Prunet, S, Puget, J, Reach, W, Renault, C, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rowan-Robinson, M, Rusholme, B, Santos, D, Savini, G, Schaefer, B, Shellard, P, Spencer, L, Starck, J, Stassi, P, Stolyarov, V, Stompor, R, Sudiwala, R, Sunyaev, R, Sygnet, J, Tauber, J, Thum, C, Torre, J, Touze, F, Tristram, M, Van Leeuwen, F, Vibert, L, Vibert, D, Wade, L, Wandelt, B, White, S, Wiesemeyer, H, Woodcraft, A, Yurchenko, V, Yvon, D, Zacchei, A, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Cryogénie (Cryo), Laboratoire Traitement et Communication de l'Information (LTCI), Télécom ParisTech-Institut Mines-Télécom [Paris] (IMT)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG ), Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de RadioAstronomie Millimétrique (IRAM), Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), PLANCK, Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL), Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry]), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), HELFA - Hélium : du fondamental aux applications, Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Cryo - Cryogénie, École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Cryogénie (NEEL - Cryo), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), and Science and Technology Facilities Council (STFC)
Subjects: observation, CRYOCOOLER, POWER SPECTRUM, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], HFI, Cosmic microwave background, Method, Cosmic background radiation, 01 natural sciences, 7. Clean energy, law.invention, law, Ultra-high-energy cosmic ray, 010303 astronomy & astrophysics, Instrumentation, MISSION, QB, CALIBRATION, Physics, BOLOMETERS, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Physical optics, Cosmology, instrumentation: photometers, Physical Sciences, astro-ph.CO, symbols, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, data analysi, BOOMERANG, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Infrasound, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, Optics, 0201 Astronomical and Space Sciences, 0103 physical sciences, PRE-LAUNCH STATUS, photometer, Planck, Instrumentation and Methods for Astrophysics (astro-ph.IM), ANISOTROPY, Science & Technology, detector, methods, detectors, data analysis, cosmology: observations, cosmic background radiation, methods: data analysis, cosmology, photometers, instrumentation, instrumentation: detectors, observations, 010308 nuclear & particles physics, business.industry, Bolometer, Astronomy and Astrophysics, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Space and Planetary Science, business, SYSTEM, astro-ph.IM
Abstract: The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the Cosmic Microwave Background and galactic foregrounds in six wide bands centered at 100, 143, 217, 353, 545 and 857 GHz at an angular resolution of 10' (100 GHz), 7' (143 GHz), and 5' (217 GHz and higher). HFI has been operating flawlessly since launch on 14 May 2009. The bolometers cooled to 100 mK as planned. The settings of the readout electronics, such as the bolometer bias current, that optimize HFI's noise performance on orbit are nearly the same as the ones chosen during ground testing. Observations of Mars, Jupiter, and Saturn verified both the optical system and the time response of the detection chains. The optical beams are close to predictions from physical optics modeling. The time response of the detection chains is close to pre-launch measurements. The detectors suffer from an unexpected high flux of cosmic rays related to low solar activity. Due to the redundancy of Planck's observations strategy, the removal of a few percent of data contaminated by glitches does not affect significantly the sensitivity. The cosmic rays heat up significantly the bolometer plate and the modulation on periods of days to months of the heat load creates a common drift of all bolometer signals which do not affect the scientific capabilities. Only the high energy cosmic rays showers induce inhomogeneous heating which is a probable source of low frequency noise., Submitted to A&A. 22 pages, 6 tables, 21 figures. One of a set of simultaneous papers for the Planck Mission
Published: 2011

17. Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance

Author: Ade, P.A.R., Aghanim, N., Ansari, R., Arnaud, M., Ashdown, M., Aumont, J., Banday, A.J., Bartelmann, M., Bartlett, J.G., Battaner, E., Benabed, K., Benoit, A., Bernard, J.-P., Bersanelli, M., Bhatia, R., Bock, J.J., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Bradshaw, T., Breelle, E., Bucher, M., Camus, P., Cardoso, J.-F., Catalano, A., Challinor, A., Chamballu, A., Charra, J., Charra, M., Chary, R.-R., Chiang, C., Church, S., Clements, D.L., Colombi, S., Couchot, F., Coulais, A., Cressiot, C., Crill, B.P., Crook, M., De Bernardis, P., Delabrouille, J., Delouis, J.-M., Desert, F.-X., Dolag, K., Dole, H., Dore, O., Douspis, M., Efstathiou, G., Eng, P., Filliard, C., Forni, O., Fosalba, P., Fourmond, J.-J., Ganga, K., Giard, M., Girard, D., Giraud-Héraud, Y., Gispert, R., Gorski, K.M., Gratton, S., Griffin, M., Guyot, G., Haissinski, J., Harrison, D., Helou, G., Henrot-Versille, S., Hernandes-Monteagudo, C., Hildebrandt, S.R., Hills, R., Hivon, E., Hobson, M., Holmes, W.A., Huffenberger, K.M., Jaffe, A.H., Jones, W.C., Kaplan, J., Kneissl, R., Knox, L., Lagache, G., Lamarre, J.-M., Lami, P., Lange, A.E., Lasenby, A., Lavabre, A., Lawrence, C.R., Leriche, B., Leroy, C., Longval, Y., Macias-Perez, J.F., Maciaszek, T., MacTavish, C.J., Maffei, B., Mandolesi, N., Mann, R., Mansoux, B., Masi, S., Matsumura, T., McGehee, P., Melin, J.-B., Mercier, C., Miville-Deschenes, M.-A., Moneti, A., Montier, L., Mortlock, D., Murphy, A., Nati, F., Netterfield, C.B., Norgaard-Nielsen, H.U., North, C., Noviello, F., Novikov, D., Osborne, S., Paine, C., Pajot, F., Patanchon, G., Peacocke, T., Pearson, T.J., Perdereau, O., Perotto, L., Piacentini, F., Piat, M., Plaszczynski, S., Pointecouteau, E., Pons, R., Ponthieu, N., Prezeau, G., Prunet, S., Puget, J.-L., Reach, W.T., Renault, C., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rowan-Robinson, M., Rusholme, B., Santos, D., Savini, G., Schaefer, B.M., Shellard, P., Spencer, L., Starck, J.-L., Stassi, P., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sygnet, J.-F., Tauber, J.A., Thum, C., Torre, J.-P., Touze, F., Tristram, M., van Leeuwen, B.-J., Vibert, L., Vibert, D., Wade, L.A., White, S.D.M., Wiesemeyer, H., Woodcraft, A., Yurchenko, V., Yvon, D., and Zacchei, A.
Subjects: Experimental Physics, Astrophysics::Instrumentation and Methods for Astrophysics
Abstract: The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the cosmic microwave background and Galactic foregrounds in six ∼30% bands centered at 100, 143, 217, 353, 545, and 857 GHz at an angular resolution of 10 (100 GHz), 7 (143 GHz), and 5 (217 GHz and higher). HFI has been operating flawlessly since launch on 14 May 2009, with the bolometers reaching 100 mK the first week of July. The settings of the readout electronics, including bolometer bias currents, that optimize HFI’s noise performance on orbit are nearly the same as the ones chosen during ground testing. Observations of Mars, Jupiter, and Saturn have confirmed that the optical beams and the time responses of the detection chains are in good agreement with the predictions of physical optics modeling and pre-launch measurements. The Detectors suffer from a high flux of cosmic rays due to historically low levels of solar activity. As a result of the redundancy of Planck’s observation strategy, the removal of a few percent of data contaminated by glitches does not significantly affect the instrumental sensitivity. The cosmic ray flux represents a significant and variable heat load on the sub-Kelvin stage. Temporal variation and the inhomogeneous distribution of the flux results in thermal fluctuations that are a probable source of low frequency noise. The removal of systematic effects in the time ordered data provides a signal with an average noise equivalent power that is 70% of the goal in the 0.6−2.5 Hz range. This is slightly higher than was achieved during the pre-launch characterization but better than predicted in the early phases of the project. The improvement over the goal is a result of the low level of instrumental background loading achieved by the optical and thermal design of the HFI.
Published: 2011

18. The Planck High Frequency Instrument, a 3rd generation CMB experiment, and a full sky submillimeter survey

Author: Lamarre, J. M., Puget, J. L., Bouchet, F., Ade, P. A. R., Benoit, A., Bernard, J. P., Bock, J., DE BERNARDIS, Paolo, Charra, J., Couchot, F., Delabrouille, J., Efstathiou, G., Giard, M., Guyot, G., Lange, A., Maffei, B., Murphy, A., Pajot, F., Piat, M., Ristorcelli, I., Santos, D., Sudiwala, R., Sygnet, J. F., Torre, J. P., and Yvon, V. YURCHENKO AND D.
Published: 2004

19. Planck Ground Segment Interface Requirements Document

Author: Aloy, L., Bremer, M., Byutler, C., Charra, J., Guglielmi, L., Laureijs, R.J., Mercier, Claude, Peccia, N., Schmidt, M., Tauber, J., and ZACCHEI, Andrea
Published: 2002

20. The High Frequency Instrument of Planck: Design and Performances

Author: J-M, Lamarre, Ade, P. A. R., Angélique Benoit, Bernardis, P., Bock, J., Freddy Bouchet, Bradshaw, T., Charra, J., François Couchot, Delabrouille, J., Efstathiuo, G., Giard, M., Giraud-Heraud, Y., Gispert, R., Griffin, M., Lange, A., Murphy, A., Pajot, F., J-L, Puget, Ristorcelli, I., Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Lantz, Simone
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
Published: 2000

21. Planck early results. I. The Planck mission

Author: Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A.J., Barreiro, R.B., Bartlett, J.G., Battaner, E., Benabed, K., Bennett, D., Benoit, A., Bernard, J.-P., Bersanelli, M., Bhatia, R., Bock, J.J., Bonaldi, A., Bond, J.R., Borrill, J., Bouchet, F.R., Bradshaw, T., Bremer, M., Bucher, M., Burigana, C., Butler, R.C., Cabella, P., Cantalupo, C.M., Cappellini, B., Cardoso, J.-F., Carr, R., Casale, M., Catalano, A., Cayon, L., Challinor, A., Chamballu, A., Charra, J., Chary, R.-R., Chiang, L.-Y., Chiang, C., Christensen, P.R., Clements, D.L., Colombi, S., Couchot, F., Coulais, A., Crill, B.P., Crone, G., Crook, M., Cuttaia, F., Danese, L., D'Arcangelo, O., Davies, R.D., De Bernardis, P., de Bruin, J., de Gasperis, G., de Rosa, A., de Zotti, G., Delabrouille, J., Delouis, J.-M., Desert, F.-X., Dick, J., Dickinson, C., Dolag, K., Dole, H., Donzelli, S., Dore, O., Dorl, U., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T.A., Eriksen, H.K., Finelli, F., Foley, S., Forni, O., Fosalba, P., Frailis, M., Franceschi, E., Freschi, M., Gaier, T.C., Galeotta, S., Gallegos, J., Gandolfo, B., Ganga, K., Giard, M., Giardino, G., Gienger, G., Giraud-Héraud, Y., Gonzalez, J., Gonzalez-Nuevo, J., Gorkski, M., Gratton, S., Gregorio, A., Grupposo, A., Guyot, G., Haissinski, J., Hansen, F.K., Harrison, D., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Hoyland, R.J., Huffenberger, K.M., Jaffe, A.H., Jagemann, T., Jones, W.C., Juillet, J.J., Juvela, M., Kangaslahti, P., Keihanen, E., Keskitalo, R., Kisner, T.S., Kneissl, R., Knox, L., Krassenburg, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J.-M., Lange, A.E., Lasenby, A., Laureijs, R.J., Lawrence, C.R., Leach, S., Leahy, J.P., Leonardi, R., Leroy, C., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lowe, S., Lubin, P.M., Macias-Perez, J.F., Maciaszek, T., MacTavish, C.J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martinez-Gonzalez, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., McDonald, A., McGehee, P., Meinhold, P.R., Melchiorri, A., Melin, J.-B., Mendes, L., Mennella, A., Mevi, C., Miniscalco, R., Mitra, S., Miville-Deschenes, M.-A., Moneti, A., Montier, L., Morgante, G., Morrisset, N., Mortlock, D., Munshi, D., Murphy, J.Anthony, Naselsky, P., Natoli, P., Netterfield, C.B., Norgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I.J., Ortiz, I., Osborne, S., Osuna, P., Oxborrow, C.A., Pajot, F., Paladini, R., Partridge, B., Pasian, F., Passvogel, T., Patanchon, G., Pearson, D., Pearson, T.J., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Prezeau, G., Prunet, S., Puget, J.-L., Rachen, J.P., Reach, W.T., Rebolo, R., Reinecke, M., Reix, J.-M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rowan-Robinson, M., Rubino-Martin, J.A., Rusholme, B., Salerno, E., Sandri, M., Santos, D., Savini, G., Schaefer, B.M., Scott, D., Seiffert, M.D., Shellard, P., Simonetto, A., Smoot, G.F., Sozzi, C., Starck, J.-L., Sternberg, J., Stivoli, F., Stolyarov, V., Sudiwala, R., Sunyaev, R., Sygnet, J.-F., Tapiador, D., Tauber, J.A., Tavagnacco, D., Taylor, D., Terenzi, L., Texier, D., Toffolatti, L., Tomasi, M., Torre, J.-P., Tristram, M., Tuovinen, J., Turler, M., Tuttlebee, M., Umana, G., Valenziano, L., Valiviita, J., Varis, J., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L.A., Wandelt, B.D., Watson, C., White, S.D.M., White, M., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A.J., Barreiro, R.B., Bartlett, J.G., Battaner, E., Benabed, K., Bennett, D., Benoit, A., Bernard, J.-P., Bersanelli, M., Bhatia, R., Bock, J.J., Bonaldi, A., Bond, J.R., Borrill, J., Bouchet, F.R., Bradshaw, T., Bremer, M., Bucher, M., Burigana, C., Butler, R.C., Cabella, P., Cantalupo, C.M., Cappellini, B., Cardoso, J.-F., Carr, R., Casale, M., Catalano, A., Cayon, L., Challinor, A., Chamballu, A., Charra, J., Chary, R.-R., Chiang, L.-Y., Chiang, C., Christensen, P.R., Clements, D.L., Colombi, S., Couchot, F., Coulais, A., Crill, B.P., Crone, G., Crook, M., Cuttaia, F., Danese, L., D'Arcangelo, O., Davies, R.D., De Bernardis, P., de Bruin, J., de Gasperis, G., de Rosa, A., de Zotti, G., Delabrouille, J., Delouis, J.-M., Desert, F.-X., Dick, J., Dickinson, C., Dolag, K., Dole, H., Donzelli, S., Dore, O., Dorl, U., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T.A., Eriksen, H.K., Finelli, F., Foley, S., Forni, O., Fosalba, P., Frailis, M., Franceschi, E., Freschi, M., Gaier, T.C., Galeotta, S., Gallegos, J., Gandolfo, B., Ganga, K., Giard, M., Giardino, G., Gienger, G., Giraud-Héraud, Y., Gonzalez, J., Gonzalez-Nuevo, J., Gorkski, M., Gratton, S., Gregorio, A., Grupposo, A., Guyot, G., Haissinski, J., Hansen, F.K., Harrison, D., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Hoyland, R.J., Huffenberger, K.M., Jaffe, A.H., Jagemann, T., Jones, W.C., Juillet, J.J., Juvela, M., Kangaslahti, P., Keihanen, E., Keskitalo, R., Kisner, T.S., Kneissl, R., Knox, L., Krassenburg, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J.-M., Lange, A.E., Lasenby, A., Laureijs, R.J., Lawrence, C.R., Leach, S., Leahy, J.P., Leonardi, R., Leroy, C., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lowe, S., Lubin, P.M., Macias-Perez, J.F., Maciaszek, T., MacTavish, C.J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martinez-Gonzalez, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., McDonald, A., McGehee, P., Meinhold, P.R., Melchiorri, A., Melin, J.-B., Mendes, L., Mennella, A., Mevi, C., Miniscalco, R., Mitra, S., Miville-Deschenes, M.-A., Moneti, A., Montier, L., Morgante, G., Morrisset, N., Mortlock, D., Munshi, D., Murphy, J.Anthony, Naselsky, P., Natoli, P., Netterfield, C.B., Norgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I.J., Ortiz, I., Osborne, S., Osuna, P., Oxborrow, C.A., Pajot, F., Paladini, R., Partridge, B., Pasian, F., Passvogel, T., Patanchon, G., Pearson, D., Pearson, T.J., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Prezeau, G., Prunet, S., Puget, J.-L., Rachen, J.P., Reach, W.T., Rebolo, R., Reinecke, M., Reix, J.-M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rowan-Robinson, M., Rubino-Martin, J.A., Rusholme, B., Salerno, E., Sandri, M., Santos, D., Savini, G., Schaefer, B.M., Scott, D., Seiffert, M.D., Shellard, P., Simonetto, A., Smoot, G.F., Sozzi, C., Starck, J.-L., Sternberg, J., Stivoli, F., Stolyarov, V., Sudiwala, R., Sunyaev, R., Sygnet, J.-F., Tapiador, D., Tauber, J.A., Tavagnacco, D., Taylor, D., Terenzi, L., Texier, D., Toffolatti, L., Tomasi, M., Torre, J.-P., Tristram, M., Tuovinen, J., Turler, M., Tuttlebee, M., Umana, G., Valenziano, L., Valiviita, J., Varis, J., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L.A., Wandelt, B.D., Watson, C., White, S.D.M., White, M., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Abstract: The European Space Agency’s Planck satellite was launched on 14 May 2009, and has been surveying the sky stably and continuously since 13 August 2009. Its performance is well in line with expectations, and it will continue to gather scientific data until the end of its cryogenic lifetime. We give an overview of the history of Planck in its first year of operations, and describe some of the key performance aspects of the satellite. This paper is part of a package submitted in conjunction with Planck’s Early Release Compact Source Catalogue, the first data product based on Planck to be released publicly. The package describes the scientific performance of the Planck payload, and presents results on a variety of astrophysical topics related to the sources included in the Catalogue, as well as selected topics on diffuse emission.
Published: 2011

22. Planck early results. II. The thermal performance of Planck

Author: Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A.J., Barreiro, R.B., Battaner, E., Benabed, K., Benoit, A., Bernard, J.-P., Bersanelli, M., Bhandari, P., Bhatia, R., Bock, J.J., Bonaldi, A., Bond, J.R., Borders, J., Borrill, J., Bouchet, F.R., Bowman, B., Bradshaw, T., Breelle, E., Bucher, M., Burigana, C., Butler, R.C., Cabella, P., Camus, P., Cantalupo, C.M., Cappellini, B., Cardoso, J.-F., Catalano, A., Cayon, L., Challinor, A., Chamballu, A., Chambelland, J.P., Charra, J., Charra, M., Chiang, L.-Y., Chiang, C., Christensen, P.R., Clements, D.L., Collaudin, B., Colombi, S., Couchot, F., Coulais, A., Crill, B.P., Crook, M., Cuttaia, F., Damasio, C., Danese, L., Davies, R.D., Davis, R.J., De Bernardis, P., de Gasperis, G., de Rosa, A., Delabrouille, J., Delouis, J.-M., Desert, F.-X., Dolag, K., Donzelli, S., Dore, O., Dorl, U., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T.A., Eriksen, H.K., Filliard, C., Finelli, F., Foley, S., Forni, O., Fosalba, P., Fourmond, J.-J., Frailis, M., Franceschi, E., Galeotta, S., Ganga, K., Gavila, E., Giard, M., Giardino, G., Giraud-Héraud, Y., Gonzalez-Nuevo, J., Gorski, K.M., Gratton, S., Gregorio, A., Grupposo, A., Guyot, G., Harrison, D., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Hoyland, R.J., Huffenberger, K.M., Israelsson, U., Jaffe, A.H., Jones, W.C., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T.S., Kneissl, R., Knox, L., Kurki-Suonio, H., Lagache, G., Lamarre, J.-M., Lami, P., Lasenby, A., Laureijs, R.J., Lavabre, A., Lawrence, C.R., Leach, S., Lee, R., Leonardi, R., Leroy, C., Lilje, P.B., Lopez-Caniego, M., Lubin, P.M., Macias-Perez, J.F., Maciaszek, T., MacTavish, C.J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., McGehee, P., Meinhold, P.R., Melchiorri, A., Melot, F., Mendes, L., Mennella, A., Miville-Deschenes, M.-A., Moneti, A., Montier, L., Mora, J., Morgante, G., Morisset, N., Mortlock, D., Munshi, D., Murphy, J.Anthony, Naselsky, P., Nash, A., Natoli, P., Netterfield, C.B., Novikov, D., Novikov, I., O'Dwyer, I.J., Osborne, S., Pajot, F., Pasian, F., Patanchon, G., Pearson, D., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Poutanen, T., Prezeau, G., Prina, M., Prunet, S., Rachen, J.P., Rebolo, R., Reinecke, M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rubino-Martin, J.A., Rusholme, B., Sandri, M., Santos, D., Savini, G., Schaefer, B.M., Scott, D., Seiffert, M.D., Shellard, P., Smoot, G.F., Starck, J.-L., Stassi, P., Stivoli, F., Stolyarov, V., Stompor, R., Sudiwala, R., Sygnet, J.-F., Tauber, J.A., Terenzi, L., Toffolatti, L., Tomasi, M., Torre, J.-P., Tristram, M., Tuovinen, J., Valenziano, L., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L.A., Wandelt, B.D., Watson, C., White, S.D.M., Wilkinson, A., Wilson, P., Yvon, D., Zacchei, A., Zhang, B., Zonca, A., Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A.J., Barreiro, R.B., Battaner, E., Benabed, K., Benoit, A., Bernard, J.-P., Bersanelli, M., Bhandari, P., Bhatia, R., Bock, J.J., Bonaldi, A., Bond, J.R., Borders, J., Borrill, J., Bouchet, F.R., Bowman, B., Bradshaw, T., Breelle, E., Bucher, M., Burigana, C., Butler, R.C., Cabella, P., Camus, P., Cantalupo, C.M., Cappellini, B., Cardoso, J.-F., Catalano, A., Cayon, L., Challinor, A., Chamballu, A., Chambelland, J.P., Charra, J., Charra, M., Chiang, L.-Y., Chiang, C., Christensen, P.R., Clements, D.L., Collaudin, B., Colombi, S., Couchot, F., Coulais, A., Crill, B.P., Crook, M., Cuttaia, F., Damasio, C., Danese, L., Davies, R.D., Davis, R.J., De Bernardis, P., de Gasperis, G., de Rosa, A., Delabrouille, J., Delouis, J.-M., Desert, F.-X., Dolag, K., Donzelli, S., Dore, O., Dorl, U., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T.A., Eriksen, H.K., Filliard, C., Finelli, F., Foley, S., Forni, O., Fosalba, P., Fourmond, J.-J., Frailis, M., Franceschi, E., Galeotta, S., Ganga, K., Gavila, E., Giard, M., Giardino, G., Giraud-Héraud, Y., Gonzalez-Nuevo, J., Gorski, K.M., Gratton, S., Gregorio, A., Grupposo, A., Guyot, G., Harrison, D., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Hoyland, R.J., Huffenberger, K.M., Israelsson, U., Jaffe, A.H., Jones, W.C., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T.S., Kneissl, R., Knox, L., Kurki-Suonio, H., Lagache, G., Lamarre, J.-M., Lami, P., Lasenby, A., Laureijs, R.J., Lavabre, A., Lawrence, C.R., Leach, S., Lee, R., Leonardi, R., Leroy, C., Lilje, P.B., Lopez-Caniego, M., Lubin, P.M., Macias-Perez, J.F., Maciaszek, T., MacTavish, C.J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., McGehee, P., Meinhold, P.R., Melchiorri, A., Melot, F., Mendes, L., Mennella, A., Miville-Deschenes, M.-A., Moneti, A., Montier, L., Mora, J., Morgante, G., Morisset, N., Mortlock, D., Munshi, D., Murphy, J.Anthony, Naselsky, P., Nash, A., Natoli, P., Netterfield, C.B., Novikov, D., Novikov, I., O'Dwyer, I.J., Osborne, S., Pajot, F., Pasian, F., Patanchon, G., Pearson, D., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Poutanen, T., Prezeau, G., Prina, M., Prunet, S., Rachen, J.P., Rebolo, R., Reinecke, M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rubino-Martin, J.A., Rusholme, B., Sandri, M., Santos, D., Savini, G., Schaefer, B.M., Scott, D., Seiffert, M.D., Shellard, P., Smoot, G.F., Starck, J.-L., Stassi, P., Stivoli, F., Stolyarov, V., Stompor, R., Sudiwala, R., Sygnet, J.-F., Tauber, J.A., Terenzi, L., Toffolatti, L., Tomasi, M., Torre, J.-P., Tristram, M., Tuovinen, J., Valenziano, L., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L.A., Wandelt, B.D., Watson, C., White, S.D.M., Wilkinson, A., Wilson, P., Yvon, D., Zacchei, A., Zhang, B., and Zonca, A.
Abstract: The performance of the Planck instruments in space is enabled by their low operating temperatures, 20 K for LFI and 0.1 K for HFI, achieved through a combination of passive radiative cooling and three active mechanical coolers. The scientific requirement for very broad frequency coverage led to two detector technologies with widely different temperature and cooling needs. Active coolers could satisfy these needs; a helium cryostat, as used by previous cryogenic space missions (IRAS, COBE, ISO, Spitzer, AKARI), could not. Radiative cooling is provided by three V-groove radiators and a large telescope baffle. The active coolers are a hydrogen sorption cooler (<20 K), a 4He Joule-Thomson cooler (4.7 K), and a 3He-4He dilution cooler (1.4 K and 0.1 K). The flight system was at ambient temperature at launch and cooled in space to operating conditions. The HFI bolometer plate reached 93 mK on 3 July 2009, 50 days after launch. The solar panel always faces the Sun, shadowing the rest of Planck, and operates at a mean temperature of 384 K. At the other end of the spacecraft, the telescope baffle operates at 42.3 K and the telescope primary mirror operates at 35.9 K. The temperatures of key parts of the instruments are stabilized by both active and passive methods. Temperature fluctuations are driven by changes in the distance from the Sun, sorption cooler cycling and fluctuations in gas-liquid flow, and fluctuations in cosmic ray flux on the dilution and bolometer plates. These fluctuations do not compromise the science data.
Published: 2011

23. Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance

Author: Hfi Core Team, P, Ade, P, Aghanim, N, Ansari, R, Arnaud, M, Ashdown, M, Aumont, J, Banday, A, Bartelmann, M, Bartlett, J, Battaner, E, Benabed, K, Benoit, A, Bernard, J, Bersanelli, M, Bhatia, R, Bock, J, Bond, J, Borrill, J, Bouchet, F, Boulanger, F, Bradshaw, T, Breelle, E, Bucher, M, Camus, P, Cardoso, J, Catalano, A, Challinor, A, Chamballu, A, Charra, J, Charra, M, Chary, R, Chiang, C, Church, S, Clements, D, Colombi, S, Couchot, F, Coulais, A, Cressiot, C, Crill, B, Crook, M, De Bernardis, P, Delabrouille, J, Delouis, J, Desert, F, Dolag, K, Dole, H, Dore, O, Douspis, M, Efstathiou, G, Eng, P, Filliard, C, Forni, O, Fosalba, P, Fourmond, J, Ganga, K, Giard, M, Girard, D, Giraud-Heraud, Y, Gispert, R, Gorski, K, Gratton, S, Griffin, M, Guyot, G, Haissinski, J, Harrison, D, Helou, G, Henrot-Versille, S, Hernandez-Monteagudo, C, Hildebrandt, S, Hills, R, Hivon, E, Hobson, M, Holmes, W, Huffenberger, K, Jaffe, A, Jones, W, Kaplan, J, Kneissl, R, Knox, L, Lagache, G, Lamarre, J, Lami, P, Lange, A, Lasenby, A, Lavabre, A, Lawrence, C, Leriche, B, Leroy, C, Longval, Y, Macias-Perez, J, Maciaszek, T, Mactavish, C, Maffei, B, Mandolesi, N, Mann, R, Mansoux, B, Masi, S, Matsumura, T, Mcgehee, P, Melin, J, Mercier, C, Miville-Deschenes, M, Moneti, A, Montier, L, Mortlock, D, Murphy, A, Nati, F, Netterfield, C, Norgaard-Nielsen, H, Nørgaard-Nielsen, H, North, C, Noviello, F, Novikov, D, Osborne, S, Paine, C, Pajot, F, Patanchon, G, Peacocke, T, Pearson, T, Perdereau, O, Perotto, L, Piacentini, F, Piat, M, Plaszczynski, S, Pointecouteau, E, Pons, R, Ponthieu, N, Prezeau, G, Prunet, S, Puget, J, Reach, W, Renault, C, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rowan-Robinson, M, Rusholme, B, Santos, D, Savini, G, Schaefer, B, Shellard, P, Spencer, L, Starck, J, Stassi, P, Stolyarov, V, Stompor, R, Sudiwala, R, Sunyaev, R, Sygnet, J, Tauber, J, Thum, C, Torre, J, Touze, F, Tristram, M, Van Leeuwen, F, Vibert, L, Vibert, D, Wade, L, Wandelt, B, White, S, Wiesemeyer, H, Woodcraft, A, Yurchenko, V, Yvon, D, Zacchei, A, Planck Hfi Core Team, P.A.R. Ade, N. Aghanim, R. Ansari, M. Arnaud, M. Ashdown, J. Aumont, A.J. Banday, M. Bartelmann, J.G. Bartlett, E. Battaner, K. Benabed, A. Benoit, J.P. Bernard, M. Bersanelli, R. Bhatia, J.J. Bock, J.R. Bond, J. Borrill, F.R. Bouchet, F. Boulanger, T. Bradshaw, E. Breelle, M. Bucher, P. Camus, J.F. Cardoso, A. Catalano, A. Challinor, A. Chamballu, J. Charra, M. Charra, R.R. Chary, C. Chiang, S. Church, D.L. Clements, S. Colombi, F. Couchot, A. Coulais, C. Cressiot, B.P. Crill, M. Crook, Paolo De Bernardis, J. Delabrouille, J.M. Delouis, F.X. Desert, K. Dolag, H. Dole, O. Dore, M. Douspis, G. Efstathiou, P. Eng, C. Filliard, O. Forni, P. Fosalba, J.J. Fourmond, K. Ganga, M. Giard, D. Girard, Y. Giraud-Heraud, R. Gispert, K.M. Gorski, S. Gratton, M. Griffin, G. Guyot, J. Haissinski, D. Harrison, G. Helou, S. Henrot-Versille, C. Hernandez-Monteagudo, S.R. Hildebrandt, R. Hills, E. Hivon, M. Hobson, W.A. Holmes, K.M. Huffenberger, A.H. Jaffe, W.C. Jones, J. Kaplan, R. Kneissl, L. Knox, G. Lagache, J.M. Lamarre, P. Lami, A.E. Lange, A. Lasenby, A. Lavabre, C.R. Lawrence, B. Leriche, C. Leroy, Y. Longval, J.F. Macias-Perez, T. Maciaszek, C.J. Mactavish, B. Maffei, N. Mandolesi, R. Mann, B. Mansoux, Silvia Masi, T. Matsumura, P. Mcgehee, J.B. Melin, C. Mercier, M.A. Miville-Deschenes, A. Moneti, L. Montier, D. Mortlock, A. Murphy, Federico Nati, C.B. Netterfield, H.U. Norgaard-Nielsen, H.U. Nørgaard-Nielsen, C. North, F. Noviello, D. Novikov, S. Osborne, C. Paine, F. Pajot, G. Patanchon, T. Peacocke, T.J. Pearson, O. Perdereau, L. Perotto, Francesco Piacentini, M. Piat, S. Plaszczynski, E. Pointecouteau, R. Pons, N. Ponthieu, G. Prezeau, S. Prunet, J.L. Puget, W.T. Reach, C. Renault, I. Ristorcelli, G. Rocha, C. Rosset, G. Roudier, M. Rowan-Robinson, B. Rusholme, D. Santos, Giorgio Savini, B.M. Schaefer, P. Shellard, L. Spencer, J.L. Starck, P. Stassi, V. Stolyarov, R. Stompor, R. Sudiwala, R. Sunyaev, J.F. Sygnet, J.A. Tauber, C. Thum, J.P. Torre, F. Touze, M. Tristram, F. Van Leeuwen, L. Vibert, D. Vibert, L.A. Wade, B.D. Wandelt, S.D.M. White, H. Wiesemeyer, A. Woodcraft, V. Yurchenko, D. Yvon, A. Zacchei, Hfi Core Team, P, Ade, P, Aghanim, N, Ansari, R, Arnaud, M, Ashdown, M, Aumont, J, Banday, A, Bartelmann, M, Bartlett, J, Battaner, E, Benabed, K, Benoit, A, Bernard, J, Bersanelli, M, Bhatia, R, Bock, J, Bond, J, Borrill, J, Bouchet, F, Boulanger, F, Bradshaw, T, Breelle, E, Bucher, M, Camus, P, Cardoso, J, Catalano, A, Challinor, A, Chamballu, A, Charra, J, Charra, M, Chary, R, Chiang, C, Church, S, Clements, D, Colombi, S, Couchot, F, Coulais, A, Cressiot, C, Crill, B, Crook, M, De Bernardis, P, Delabrouille, J, Delouis, J, Desert, F, Dolag, K, Dole, H, Dore, O, Douspis, M, Efstathiou, G, Eng, P, Filliard, C, Forni, O, Fosalba, P, Fourmond, J, Ganga, K, Giard, M, Girard, D, Giraud-Heraud, Y, Gispert, R, Gorski, K, Gratton, S, Griffin, M, Guyot, G, Haissinski, J, Harrison, D, Helou, G, Henrot-Versille, S, Hernandez-Monteagudo, C, Hildebrandt, S, Hills, R, Hivon, E, Hobson, M, Holmes, W, Huffenberger, K, Jaffe, A, Jones, W, Kaplan, J, Kneissl, R, Knox, L, Lagache, G, Lamarre, J, Lami, P, Lange, A, Lasenby, A, Lavabre, A, Lawrence, C, Leriche, B, Leroy, C, Longval, Y, Macias-Perez, J, Maciaszek, T, Mactavish, C, Maffei, B, Mandolesi, N, Mann, R, Mansoux, B, Masi, S, Matsumura, T, Mcgehee, P, Melin, J, Mercier, C, Miville-Deschenes, M, Moneti, A, Montier, L, Mortlock, D, Murphy, A, Nati, F, Netterfield, C, Norgaard-Nielsen, H, Nørgaard-Nielsen, H, North, C, Noviello, F, Novikov, D, Osborne, S, Paine, C, Pajot, F, Patanchon, G, Peacocke, T, Pearson, T, Perdereau, O, Perotto, L, Piacentini, F, Piat, M, Plaszczynski, S, Pointecouteau, E, Pons, R, Ponthieu, N, Prezeau, G, Prunet, S, Puget, J, Reach, W, Renault, C, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rowan-Robinson, M, Rusholme, B, Santos, D, Savini, G, Schaefer, B, Shellard, P, Spencer, L, Starck, J, Stassi, P, Stolyarov, V, Stompor, R, Sudiwala, R, Sunyaev, R, Sygnet, J, Tauber, J, Thum, C, Torre, J, Touze, F, Tristram, M, Van Leeuwen, F, Vibert, L, Vibert, D, Wade, L, Wandelt, B, White, S, Wiesemeyer, H, Woodcraft, A, Yurchenko, V, Yvon, D, Zacchei, A, Planck Hfi Core Team, P.A.R. Ade, N. Aghanim, R. Ansari, M. Arnaud, M. Ashdown, J. Aumont, A.J. Banday, M. Bartelmann, J.G. Bartlett, E. Battaner, K. Benabed, A. Benoit, J.P. Bernard, M. Bersanelli, R. Bhatia, J.J. Bock, J.R. Bond, J. Borrill, F.R. Bouchet, F. Boulanger, T. Bradshaw, E. Breelle, M. Bucher, P. Camus, J.F. Cardoso, A. Catalano, A. Challinor, A. Chamballu, J. Charra, M. Charra, R.R. Chary, C. Chiang, S. Church, D.L. Clements, S. Colombi, F. Couchot, A. Coulais, C. Cressiot, B.P. Crill, M. Crook, Paolo De Bernardis, J. Delabrouille, J.M. Delouis, F.X. Desert, K. Dolag, H. Dole, O. Dore, M. Douspis, G. Efstathiou, P. Eng, C. Filliard, O. Forni, P. Fosalba, J.J. Fourmond, K. Ganga, M. Giard, D. Girard, Y. Giraud-Heraud, R. Gispert, K.M. Gorski, S. Gratton, M. Griffin, G. Guyot, J. Haissinski, D. Harrison, G. Helou, S. Henrot-Versille, C. Hernandez-Monteagudo, S.R. Hildebrandt, R. Hills, E. Hivon, M. Hobson, W.A. Holmes, K.M. Huffenberger, A.H. Jaffe, W.C. Jones, J. Kaplan, R. Kneissl, L. Knox, G. Lagache, J.M. Lamarre, P. Lami, A.E. Lange, A. Lasenby, A. Lavabre, C.R. Lawrence, B. Leriche, C. Leroy, Y. Longval, J.F. Macias-Perez, T. Maciaszek, C.J. Mactavish, B. Maffei, N. Mandolesi, R. Mann, B. Mansoux, Silvia Masi, T. Matsumura, P. Mcgehee, J.B. Melin, C. Mercier, M.A. Miville-Deschenes, A. Moneti, L. Montier, D. Mortlock, A. Murphy, Federico Nati, C.B. Netterfield, H.U. Norgaard-Nielsen, H.U. Nørgaard-Nielsen, C. North, F. Noviello, D. Novikov, S. Osborne, C. Paine, F. Pajot, G. Patanchon, T. Peacocke, T.J. Pearson, O. Perdereau, L. Perotto, Francesco Piacentini, M. Piat, S. Plaszczynski, E. Pointecouteau, R. Pons, N. Ponthieu, G. Prezeau, S. Prunet, J.L. Puget, W.T. Reach, C. Renault, I. Ristorcelli, G. Rocha, C. Rosset, G. Roudier, M. Rowan-Robinson, B. Rusholme, D. Santos, Giorgio Savini, B.M. Schaefer, P. Shellard, L. Spencer, J.L. Starck, P. Stassi, V. Stolyarov, R. Stompor, R. Sudiwala, R. Sunyaev, J.F. Sygnet, J.A. Tauber, C. Thum, J.P. Torre, F. Touze, M. Tristram, F. Van Leeuwen, L. Vibert, D. Vibert, L.A. Wade, B.D. Wandelt, S.D.M. White, H. Wiesemeyer, A. Woodcraft, V. Yurchenko, D. Yvon, and A. Zacchei
Abstract: The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the cosmic microwave background and Galactic foregrounds in six ~30% bands centered at 100, 143, 217, 353, 545, and 857 GHz at an angular resolution of 10′ (100 GHz), 7′ (143 GHz), and 5′ (217 GHz and higher). HFI has been operating flawlessly since launch on 14 May 2009, with the bolometers reaching 100 mK the first week of July. The settings of the readout electronics, including bolometer bias currents, that optimize HFI's noise performance on orbit are nearly the same as the ones chosen during ground testing. Observations of Mars, Jupiter, and Saturn have confirmed that the optical beams and the time responses of the detection chains are in good agreement with the predictions of physical optics modeling and pre-launch measurements. The Detectors suffer from a high flux of cosmic rays due to historically low levels of solar activity. As a result of the redundancy of Planck's observation strategy, theremoval of a few percent of data contaminated by glitches does not significantly affect the instrumental sensitivity. The cosmic ray flux represents a significant and variable heat load on the sub-Kelvin stage. Temporal variation and the inhomogeneous distribution of the flux results in thermal fluctuations that are a probable source of low frequency noise. The removal of systematic effects in the time ordered data provides a signal with an average noise equivalent power that is 70% of the goal in the 0.6-2.5 Hz range. This is slightly higher than was achieved during the pre-launch characterization but better than predicted in the early phases of the project. The improvement over the goal is a result of the low level of instrumental background loading achieved by the optical and thermal design of the HFI.
Published: 2011

24. Planck Early Results: The thermal performance of Planck

Author: Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoit, A., Bernard, J. P., Bersanelli, M., Bhandari, P., Bhatia, R., Bock, J. J., Bonaldi, A., Bond, J. R., Borders, J., Borrill, J., Bouchet, F. R., Bowman, B., Bradshaw, T., Breelle, E., Bucher, M., Burigana, C., Butler, R. C., Cabella, P., Camus, P., Cantalupo, C. M., Cappellini, B., Cardoso, J. F., Catalano, A., Cayon, L., Challinor, A., Chamballu, A., Chambelland, J. P., Charra, J., Charra, M., Chiang, L. Y, Chiang, C., Christensen, P. R., Clements, D. L., Collaudin, B., Colombi, S., Couchot, F., Coulais, A., Crill, B. P., Crook, M., Cuttaia, F., Damasio, C., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Gasperis, G., de Rosa, A., Delabrouille, J., Delouis, J. M., Desert, F. -X., Doerl, U., Dolag, K., Donzelli, S., Dore, O., Douspis, M., Dupac, X., Efstathiou, G., Enslin, T. A., Eriksen, H. K., Finelli, F., Foley, S., Forni, O., Fosalba, P., Fourmond, J. J., Frailis, M., Franceschi, E., Galeotta, S., Ganga, K., Gavila, E., Giard, M., Giardino, G., Giraud-Heraud, Y., Gonzalez-Nuevo, J., Gorski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Guyot, G., Harrison, D., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Hoyland, R. J., Huffenberger, K. M., Israelsson, U., Jaffe, A. H., Jones, W. C., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knox, L., Kurki-Suonio, H., Lagache, G., Lamarre, J. M., Lami, P., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leonardi, R., Leroy, C., Lilje, P. B., Lopez-Caniego, M., Lubin, P. M., Macias-Perez, J. F., Maciaszek, T., MacTavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., McGehee, P., Meinhold, P. R., Melchiorri, A., Melot, F., Mendes, L., Mennella, A., Miville-Deschenes, M. -A., Moneti, A., Montier, L., Mora, J., Morgante, G., Morisset, N., Mortlock, D., Munshi, D., Murphy, A., Naselsky, P., Nash, A., Natoli, P., Netterfield, C. B., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Pajot, F., Pasian, F., Patanchon, G., Pearson, D., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Poutanen, T., Prezeau, G., Prina, M., Prunet, S., Puget, J. L., Rachen, J. P., Rebolo, R., Reinecke, M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rubiino-Martin, J. A., Rusholme, B., Sandri, M., Santos, D., Schaefer, B. M., Scott, D., Seiffert, M. D., Shellard, P., Smoot, G. F., Starck, J. -L., Stassi, P., Stivoli, F., Stolyarov, V., Stompor, R., Sudiwala, R., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Torre, J. -P., Tristram, M., Tuovinen, J., Valenziano, L., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, C., White, S. D. M., Wilkinson, A., Wilson, P., Yvon, D., Zacchei, A., Zhang, B., Zonca, A., Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoit, A., Bernard, J. P., Bersanelli, M., Bhandari, P., Bhatia, R., Bock, J. J., Bonaldi, A., Bond, J. R., Borders, J., Borrill, J., Bouchet, F. R., Bowman, B., Bradshaw, T., Breelle, E., Bucher, M., Burigana, C., Butler, R. C., Cabella, P., Camus, P., Cantalupo, C. M., Cappellini, B., Cardoso, J. F., Catalano, A., Cayon, L., Challinor, A., Chamballu, A., Chambelland, J. P., Charra, J., Charra, M., Chiang, L. Y, Chiang, C., Christensen, P. R., Clements, D. L., Collaudin, B., Colombi, S., Couchot, F., Coulais, A., Crill, B. P., Crook, M., Cuttaia, F., Damasio, C., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Gasperis, G., de Rosa, A., Delabrouille, J., Delouis, J. M., Desert, F. -X., Doerl, U., Dolag, K., Donzelli, S., Dore, O., Douspis, M., Dupac, X., Efstathiou, G., Enslin, T. A., Eriksen, H. K., Finelli, F., Foley, S., Forni, O., Fosalba, P., Fourmond, J. J., Frailis, M., Franceschi, E., Galeotta, S., Ganga, K., Gavila, E., Giard, M., Giardino, G., Giraud-Heraud, Y., Gonzalez-Nuevo, J., Gorski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Guyot, G., Harrison, D., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Hoyland, R. J., Huffenberger, K. M., Israelsson, U., Jaffe, A. H., Jones, W. C., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knox, L., Kurki-Suonio, H., Lagache, G., Lamarre, J. M., Lami, P., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leonardi, R., Leroy, C., Lilje, P. B., Lopez-Caniego, M., Lubin, P. M., Macias-Perez, J. F., Maciaszek, T., MacTavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., McGehee, P., Meinhold, P. R., Melchiorri, A., Melot, F., Mendes, L., Mennella, A., Miville-Deschenes, M. -A., Moneti, A., Montier, L., Mora, J., Morgante, G., Morisset, N., Mortlock, D., Munshi, D., Murphy, A., Naselsky, P., Nash, A., Natoli, P., Netterfield, C. B., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Pajot, F., Pasian, F., Patanchon, G., Pearson, D., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Poutanen, T., Prezeau, G., Prina, M., Prunet, S., Puget, J. L., Rachen, J. P., Rebolo, R., Reinecke, M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Rubiino-Martin, J. A., Rusholme, B., Sandri, M., Santos, D., Schaefer, B. M., Scott, D., Seiffert, M. D., Shellard, P., Smoot, G. F., Starck, J. -L., Stassi, P., Stivoli, F., Stolyarov, V., Stompor, R., Sudiwala, R., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Torre, J. -P., Tristram, M., Tuovinen, J., Valenziano, L., Vibert, L., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, C., White, S. D. M., Wilkinson, A., Wilson, P., Yvon, D., Zacchei, A., Zhang, B., and Zonca, A.
Abstract: The performance of the Planck instruments in space is enabled by their low operating temperatures, 20K for LFI and 0.1K for HFI, achieved through a combination of passive radiative cooling and three active mechanical coolers. Active coolers were chosen to minimize straylight on the detectors and to maximize lifetime. The scientific requirement for very broad frequency led to two detector technologies with widely dierent temperature and cooling needs. This made use of a helium cryostat, as used by previous cryogenic space missions (IRAS, COBE, ISO, SPITZER, AKARI), infeasible. Radiative cooling is provided by three V-groove radiators and a large telescope bae. The active coolers are a hydrogen sorption cooler (<20 K), a 4He Joule-Thomson cooler (4.7 K), and a 3He-4He dilution cooler (1.4K and 0.1 K). The flight system was at ambient temperature at launch and cooled in space to operating conditions. The bolometer plate of the High Frequency Instrument reached 93mK on 3 July 2009, 50 days after launch. The solar panel always faces the Sun, shadowing the rest of Planck, and operates at a mean temperature of 384 K. At the other end of the spacecraft, the telescope bae operates at 42.3K and the telescope primary mirror operates at 35.9 K. The temperatures of key parts of the instruments are stabilized by both active and passive methods. Temperature fluctuations are driven by changes in the distance from the Sun, sorption cooler cycling and fluctuations in gas-liquid flow, and fluctuations in cosmic ray flux on the dilution and bolometer plates. These fluctuations do not compromise the science data.
Published: 2011

25. Planck pre-launch status: the planck mission

Author: Universitat Politècnica de Catalunya. Departament de Teoria del Senyal i Comunicacions, Universitat Politècnica de Catalunya. RF&MW - Grup de Recerca de sistemes, dispositius i materials de RF i microones, Tauber, Jan A., Mandolesi, Nazzareno, Pujet, J.L., Banos, T., Bersanelli, Marco, Bouchet, R.C., Butler, Chris, Charra, J., Crone, Gerald, Dodsworth, John, Efstathiou, George, Gispert, Richard, Guyot, Guy, Gregorio, A., Juillet, J. J., Lamarre, J. M., Laureijs, R. J., Lawrence, C. R., Nørgaard-Nielsen, H. U., Passvogel, T., Reix, J. M., Texier, D., Pradell i Cara, Lluís, Vibert, L., Zacchei, A., Ade, P.A.R, Aghanim, N., Aja Abelán, Beatriz, Alippi, E., Aloy, L., Armand, P., Arnaud, M., Arondel, A., Arreola-Villanueva, A., Artal Latorre, Eduardo, Artina, E., Arts, A., Ashdown, M., Aumont, J., Azzaro, M., Bacchetta, A., Baccigalupi, C., Baker, M., Balasini, M., Balbi, A., Banday, A.J., Barbier, G., Barreiro Vilas, Rita Belén, Bartelmann, M., Battaglia, P., Battaner, E., Benabed, K., Beney, J. L., Beneyton, R., Bennett, K., Benoit, A., Bernard, J. P., Bhandari, P., Bhatia, R., Biggi, M., Biggins, R., Billig, G., Blanc, Y., Blavot, H., Bock, J. J., Bonaldi, A., Bond, R., Bonis, J., Borders, J., Borrill, J., Boschini, L., Boulanger, F., Bouvier, J., Bouzit, M., Bowman, R., Bréelle, E., Bradshaw, T., Braghin, M., Bremer, M., Brienza, D., Broszkiewicz, D., Burigana, C., Burkhalter, M., Cabella, P., Cafferty, T., Cairola, M., Caminade, S., Camus, P., Cantalupo, C. M., Cappellini, B., Cardoso, J. F., Carr, R., Catalano, A., Cayón, L., Cesa, M., Chaigneau, M., Challinor, A., Universitat Politècnica de Catalunya. Departament de Teoria del Senyal i Comunicacions, Universitat Politècnica de Catalunya. RF&MW - Grup de Recerca de sistemes, dispositius i materials de RF i microones, Tauber, Jan A., Mandolesi, Nazzareno, Pujet, J.L., Banos, T., Bersanelli, Marco, Bouchet, R.C., Butler, Chris, Charra, J., Crone, Gerald, Dodsworth, John, Efstathiou, George, Gispert, Richard, Guyot, Guy, Gregorio, A., Juillet, J. J., Lamarre, J. M., Laureijs, R. J., Lawrence, C. R., Nørgaard-Nielsen, H. U., Passvogel, T., Reix, J. M., Texier, D., Pradell i Cara, Lluís, Vibert, L., Zacchei, A., Ade, P.A.R, Aghanim, N., Aja Abelán, Beatriz, Alippi, E., Aloy, L., Armand, P., Arnaud, M., Arondel, A., Arreola-Villanueva, A., Artal Latorre, Eduardo, Artina, E., Arts, A., Ashdown, M., Aumont, J., Azzaro, M., Bacchetta, A., Baccigalupi, C., Baker, M., Balasini, M., Balbi, A., Banday, A.J., Barbier, G., Barreiro Vilas, Rita Belén, Bartelmann, M., Battaglia, P., Battaner, E., Benabed, K., Beney, J. L., Beneyton, R., Bennett, K., Benoit, A., Bernard, J. P., Bhandari, P., Bhatia, R., Biggi, M., Biggins, R., Billig, G., Blanc, Y., Blavot, H., Bock, J. J., Bonaldi, A., Bond, R., Bonis, J., Borders, J., Borrill, J., Boschini, L., Boulanger, F., Bouvier, J., Bouzit, M., Bowman, R., Bréelle, E., Bradshaw, T., Braghin, M., Bremer, M., Brienza, D., Broszkiewicz, D., Burigana, C., Burkhalter, M., Cabella, P., Cafferty, T., Cairola, M., Caminade, S., Camus, P., Cantalupo, C. M., Cappellini, B., Cardoso, J. F., Carr, R., Catalano, A., Cayón, L., Cesa, M., Chaigneau, M., and Challinor, A.
Abstract: The European Space Agency's Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies of the CMB over the whole sky, with unprecedented sensitivity ( ~ 2 × 10-6) and angular resolution (~5 arcmin). Planck will provide a major source of information relevant to many fundamental cosmological problems and will test current theories of the early evolution of the Universe and the origin of structure. It will also address a wide range of areas of astrophysical research related to the Milky Way as well as external galaxies and clusters of galaxies. The ability of Planck to measure polarization across a wide frequency range (30-350 GHz), with high precision and accuracy, and over the whole sky, will provide unique insight, not only into specific cosmological questions, but also into the properties of the interstellar medium. This paper is part of a series which describes the technical capabilities of the Planck scientific payload. It is based on the knowledge gathered during the on-ground calibration campaigns of the major subsystems, principally its telescope and its two scientific instruments, and of tests at fully integrated satellite level. It represents the best estimate before launch of the technical performance that the satellite and its payload will achieve in flight. In this paper, we summarise the main elements of the payload performance, which is described in detail in the accompanying papers. In addition, we describe the satellite performance elements which are most relevant for science, and provide an overview of the plans for scientific operations and data analysis., Peer Reviewed, Postprint (published version)
Published: 2010

26. Planck pre-launch status: The Planck mission

Author: Tauber, J. A., Mandoles, N., Puget, J.-L., Banos, T., Bersanelli, M., Bouchet, F. R., Butler, R. C., Charra, J., Crone, G., Dodsworth, J., Efstathiou, G., Gispert, R., Guyot, G., Gregorio, A., Juillet, J. J., Lamarre, J.-M., Laureijs, R. J., Lawrence, C. R., Nørgaard-Nielsen, Hans Ulrik, Passvogel, T., Reix, J. M., Texier, D., Vilbert, L., Zacchei, A., Ade, P. A. R., Aghanim, N., Aja, B., Alippi, E., Aloy, L., Armand, P., Arnaud, M., Arondel, A., Arreola-Villanueva, A., Artal, E., Artina, E., Arts, A., Ashdown, M., Aumont, J., Azzaro, M., Bacchetta, A., Baccigalupi, C., Baker, M., Balasini, M., Balbi, A., Banday, A. J., Barbier, G., Barreiro, R. B., Bartelmann, M., Battaglia, P., Battaner, E., Benabed, K., Beney, J.-L., Beneyton, R., Bennett, K., Benoit, A., Bernard, J.-P., Bhandari, P., Bhatia, R., Biggi, M., Biggins, R., Billig, G., Blanc, Y., Blavot, H., Bock, J. J., Bonaldi, A., Bond, R., Bonis, J., Borders, J., Borrill, J., Boschini, L., Boulanger, F., Bouvier, J., Bouzit, M., Bowman, R., Bréelle, E., Bradshaw, T., Braghin, M., Bremer, M., Brienza, D., Broszkiewicz, D., Burigana, C., Burkhalter, M., Cabella, P., Cafferty, T., Cairola, M., Caminade, S., Camus, P., Cantalupo, C. M., Cappellini, B., Cardoso, J.-F., Carr, R., Catalono, A., Caýon, L., Cesa, M., Chaigneau, M., Challinor, A., Chamballu, A., Chambelland, J. P., Charra, M., Chiang, L.-Y., Chlewicki, G., Christensen, P. R., Church, S., Ciancietta, E., Cibrario, M., Cizeron, R., Clements, D., Collaudin, B., Colley, J.-M., Colombi, S., Colombo, A., Colombo, F., Corre, O., Couchot, F., Cougrand, B., Coulais, A., Couzin, P., Crane, B., Crill, B., Crook, M., Crumb, D., cuttala, F., Döri, U., da Silva, P., Daddato, R., Damasio, C., Danese, L., d'Aquino, G., D'Arcangelo, O., Dassas, K., Davies, R. D., Davies, W., Davis, R. J., De Bernardis, P., de Chambure, D., de Gasperis, G., De la Fuente, M. L., De Paco, P., De Rosa, A., De Troia, G., De Zotti, G., Dehamme, M., Delabrouille, J., Delouis, J.-M., Désert, F.-X., di Girolamo, G., Dickinson, C., Doelling, E., Dolag, K., Domken, I., Douspis, M., Doyle, D., Du, S., Dubruel, D., Dufour, C., Dumesnil, C., Dupac, X., Duret, P., Eder, C., Elfving, A., Enßlin, T. A., Eng, P., English, K., Eriksen, H. K., Estaria, P., Falvella, M. C., Ferrari, F., Finelli, F., Fishman, A., Fogliani, S., Foley, S., Fonseca, A., Forma, G., Forni, O., Fosalba, P., Fourmond, J.-J., Frallis, M., Franceschet, C., Franceschi, E., François, S., Frerking, M., Gómez-Reñasco, M. F., Gorski, K. M., Gaier, T. C., Galeotta, S., Ganga, K., García Lázaro, J., Garnica, A., Gaspard, M., Gavila, E., Giard, m., Giardino, G., Glenger, G., Giraud-Heraud, Y., Glorian, J.-M., Griffin, M., Gruppuso, A., Guglieimi, L., Guichon, D., Guillaume, B., Guillouet, P., Haissinski, J., Hansen, F. K., Hardy, J., Harrison, D., Hazell, A., Hechler, M., Heckenauer, V., Heinzer, D., Hell, R., Henrot-Versillé, S., Hernándes-Monteagudo, C., Herranz, D., Herreros, J. M., Hervier, V., Heske, A., Heurtel, A., Hildebrandt, S. R., Hills, R., Hivon, E., Hobson, M., Hollert, D., Holmes, W., Hornstrup, Allan, Hovest, W., Hoyland, R. J., Huey, G., Huffenberger, K. M., Hughes, N., Israelsson, U., Jackson, B., Jaffe, A., Jaffe, T. R., Jagemann, T., Jessen, Niels Christian, Jewell, J., Jones, W., Juvela, M., Kaplan, J., Karlmann, P., Keck, F., Kelhänen, E., King, M., Kisner, T. S., Kletzkine, P., Kneissi, R., Knoche, J., Knox, L., Koch, T., Krassenburg, M., Kurki-Suonio, H., Lähteenmäki, A., Lagache, G., Lagorio, E., Lami, P., Lande, J., Lange, A., Langlet, F., Lapini, R., Lapolla, M., Lasenby, A., Le Jeune, M., Leahy, J. P., Lefebvre, M., Legrand, F., Le Meur, G., Leonardi, R., Leriche, B., Leroy, C., Leutenegger, P., Levin, S. M., Lilje, P. B., Lindensmith, C., Linden-Vørnle, Michael, Loc, A., Longval, Y., Lubin, P. M., Luchik, T., Luthold, I., Macias-Perez, J. F., Maciaszek, T., MacTavish, C., Madden, S., Maffei, B., Magneville, C., Maino, D., Mambretti, A., Mansoux, B., Marchioro, D., Maris, M., Marliani, F., Marrucho, J.-C., Marti-Canales, J., Martinez-Gonzalez, E., Martin-Polegre, A., Martin, P., Marty, C., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., McDonald, A., McGrath, P., Mediavilla, A., Meinhold, P. R., Mélin, J.-B., Melot, F., Mendes, L., Mennella, A., Mervier, C., Meslier, L., Miccolis, M., Miville-Deschenes, M.-A., Moneti, A., Montet, D., Montier, L., Mora, J., Morgante, G., Morigi, G., Morinaud, G., Morisset, N., Mortlock, D., Mottet, S., Mulder, J., Munshi, D., Murphy, A., Murphy, P., Musi, P., Narbonne, J., Naselsky, P., Nash, A., Nati, F., Natoli, P., Netterfield, B., Newell, J., Nexon, M., Nicolas, C., Hansen, P. H., Ninane, N., Noviello, F., Novikov, D., Novikov, I., O´Dwyer, I. J., Oldeman, P., Olivier, P., Ouchet, L., Oxborrow, Carol Anne, Pérez-Cuevas, L., Pagan, L., Paine, C., Pajot, F., Paladini, R., Pancher, F., Panh, J., Parks, G., Parnaudeau, P., Patridge, B., Parvin, B., Pascual, J. P., Pasian, F., Pearson, D. P., Pearson, T., Pecora, M., Perdereau, O., Perotto, L., Perrotta, F., Placentini, F., Piat, M., Pierpaoli, E., Piersanti, O., Plaige, E., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poulleau, G., Poutanen, T., Prézeau, G., Pradell, L., Prina, M., Prunet, S., Rachen, J. P., Rambaud, D., Rame, F., Rasmussen, I., Rautakoski, J., Reach, W. T., Rebolo, R., Reinecke, M., Reiter, J., Renault, C., Ricciardi, S., Rideau, P., Riller, T., Ristorcelli, I., Riti, J. B., Tauber, J. A., Mandoles, N., Puget, J.-L., Banos, T., Bersanelli, M., Bouchet, F. R., Butler, R. C., Charra, J., Crone, G., Dodsworth, J., Efstathiou, G., Gispert, R., Guyot, G., Gregorio, A., Juillet, J. J., Lamarre, J.-M., Laureijs, R. J., Lawrence, C. R., Nørgaard-Nielsen, Hans Ulrik, Passvogel, T., Reix, J. M., Texier, D., Vilbert, L., Zacchei, A., Ade, P. A. R., Aghanim, N., Aja, B., Alippi, E., Aloy, L., Armand, P., Arnaud, M., Arondel, A., Arreola-Villanueva, A., Artal, E., Artina, E., Arts, A., Ashdown, M., Aumont, J., Azzaro, M., Bacchetta, A., Baccigalupi, C., Baker, M., Balasini, M., Balbi, A., Banday, A. J., Barbier, G., Barreiro, R. B., Bartelmann, M., Battaglia, P., Battaner, E., Benabed, K., Beney, J.-L., Beneyton, R., Bennett, K., Benoit, A., Bernard, J.-P., Bhandari, P., Bhatia, R., Biggi, M., Biggins, R., Billig, G., Blanc, Y., Blavot, H., Bock, J. J., Bonaldi, A., Bond, R., Bonis, J., Borders, J., Borrill, J., Boschini, L., Boulanger, F., Bouvier, J., Bouzit, M., Bowman, R., Bréelle, E., Bradshaw, T., Braghin, M., Bremer, M., Brienza, D., Broszkiewicz, D., Burigana, C., Burkhalter, M., Cabella, P., Cafferty, T., Cairola, M., Caminade, S., Camus, P., Cantalupo, C. M., Cappellini, B., Cardoso, J.-F., Carr, R., Catalono, A., Caýon, L., Cesa, M., Chaigneau, M., Challinor, A., Chamballu, A., Chambelland, J. P., Charra, M., Chiang, L.-Y., Chlewicki, G., Christensen, P. R., Church, S., Ciancietta, E., Cibrario, M., Cizeron, R., Clements, D., Collaudin, B., Colley, J.-M., Colombi, S., Colombo, A., Colombo, F., Corre, O., Couchot, F., Cougrand, B., Coulais, A., Couzin, P., Crane, B., Crill, B., Crook, M., Crumb, D., cuttala, F., Döri, U., da Silva, P., Daddato, R., Damasio, C., Danese, L., d'Aquino, G., D'Arcangelo, O., Dassas, K., Davies, R. D., Davies, W., Davis, R. J., De Bernardis, P., de Chambure, D., de Gasperis, G., De la Fuente, M. L., De Paco, P., De Rosa, A., De Troia, G., De Zotti, G., Dehamme, M., Delabrouille, J., Delouis, J.-M., Désert, F.-X., di Girolamo, G., Dickinson, C., Doelling, E., Dolag, K., Domken, I., Douspis, M., Doyle, D., Du, S., Dubruel, D., Dufour, C., Dumesnil, C., Dupac, X., Duret, P., Eder, C., Elfving, A., Enßlin, T. A., Eng, P., English, K., Eriksen, H. K., Estaria, P., Falvella, M. C., Ferrari, F., Finelli, F., Fishman, A., Fogliani, S., Foley, S., Fonseca, A., Forma, G., Forni, O., Fosalba, P., Fourmond, J.-J., Frallis, M., Franceschet, C., Franceschi, E., François, S., Frerking, M., Gómez-Reñasco, M. F., Gorski, K. M., Gaier, T. C., Galeotta, S., Ganga, K., García Lázaro, J., Garnica, A., Gaspard, M., Gavila, E., Giard, m., Giardino, G., Glenger, G., Giraud-Heraud, Y., Glorian, J.-M., Griffin, M., Gruppuso, A., Guglieimi, L., Guichon, D., Guillaume, B., Guillouet, P., Haissinski, J., Hansen, F. K., Hardy, J., Harrison, D., Hazell, A., Hechler, M., Heckenauer, V., Heinzer, D., Hell, R., Henrot-Versillé, S., Hernándes-Monteagudo, C., Herranz, D., Herreros, J. M., Hervier, V., Heske, A., Heurtel, A., Hildebrandt, S. R., Hills, R., Hivon, E., Hobson, M., Hollert, D., Holmes, W., Hornstrup, Allan, Hovest, W., Hoyland, R. J., Huey, G., Huffenberger, K. M., Hughes, N., Israelsson, U., Jackson, B., Jaffe, A., Jaffe, T. R., Jagemann, T., Jessen, Niels Christian, Jewell, J., Jones, W., Juvela, M., Kaplan, J., Karlmann, P., Keck, F., Kelhänen, E., King, M., Kisner, T. S., Kletzkine, P., Kneissi, R., Knoche, J., Knox, L., Koch, T., Krassenburg, M., Kurki-Suonio, H., Lähteenmäki, A., Lagache, G., Lagorio, E., Lami, P., Lande, J., Lange, A., Langlet, F., Lapini, R., Lapolla, M., Lasenby, A., Le Jeune, M., Leahy, J. P., Lefebvre, M., Legrand, F., Le Meur, G., Leonardi, R., Leriche, B., Leroy, C., Leutenegger, P., Levin, S. M., Lilje, P. B., Lindensmith, C., Linden-Vørnle, Michael, Loc, A., Longval, Y., Lubin, P. M., Luchik, T., Luthold, I., Macias-Perez, J. F., Maciaszek, T., MacTavish, C., Madden, S., Maffei, B., Magneville, C., Maino, D., Mambretti, A., Mansoux, B., Marchioro, D., Maris, M., Marliani, F., Marrucho, J.-C., Marti-Canales, J., Martinez-Gonzalez, E., Martin-Polegre, A., Martin, P., Marty, C., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., McDonald, A., McGrath, P., Mediavilla, A., Meinhold, P. R., Mélin, J.-B., Melot, F., Mendes, L., Mennella, A., Mervier, C., Meslier, L., Miccolis, M., Miville-Deschenes, M.-A., Moneti, A., Montet, D., Montier, L., Mora, J., Morgante, G., Morigi, G., Morinaud, G., Morisset, N., Mortlock, D., Mottet, S., Mulder, J., Munshi, D., Murphy, A., Murphy, P., Musi, P., Narbonne, J., Naselsky, P., Nash, A., Nati, F., Natoli, P., Netterfield, B., Newell, J., Nexon, M., Nicolas, C., Hansen, P. H., Ninane, N., Noviello, F., Novikov, D., Novikov, I., O´Dwyer, I. J., Oldeman, P., Olivier, P., Ouchet, L., Oxborrow, Carol Anne, Pérez-Cuevas, L., Pagan, L., Paine, C., Pajot, F., Paladini, R., Pancher, F., Panh, J., Parks, G., Parnaudeau, P., Patridge, B., Parvin, B., Pascual, J. P., Pasian, F., Pearson, D. P., Pearson, T., Pecora, M., Perdereau, O., Perotto, L., Perrotta, F., Placentini, F., Piat, M., Pierpaoli, E., Piersanti, O., Plaige, E., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poulleau, G., Poutanen, T., Prézeau, G., Pradell, L., Prina, M., Prunet, S., Rachen, J. P., Rambaud, D., Rame, F., Rasmussen, I., Rautakoski, J., Reach, W. T., Rebolo, R., Reinecke, M., Reiter, J., Renault, C., Ricciardi, S., Rideau, P., Riller, T., Ristorcelli, I., and Riti, J. B.
Abstract: The European Space Agency's Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies of the CMB over the whole sky, with unprecedented sensitivity ( ~ 2 × 10-6) and angular resolution (~5 arcmin). Planck will provide a major source of information relevant to many fundamental cosmological problems and will test current theories of the early evolution of the Universe and the origin of structure. It will also address a wide range of areas of astrophysical research related to the Milky Way as well as external galaxies and clusters of galaxies. The ability of Planck to measure polarization across a wide frequency range (30-350 GHz), with high precision and accuracy, and over the whole sky, will provide unique insight, not only into specific cosmological questions, but also into the properties of the interstellar medium. This paper is part of a series which describes the technical capabilities of the Planck scientific payload. It is based on the knowledge gathered during the on-ground calibration campaigns of the major subsystems, principally its telescope and its two scientific instruments, and of tests at fully integrated satellite level. It represents the best estimate before launch of the technical performance that the satellite and its payload will achieve in flight. In this paper, we summarise the main elements of the payload performance, which is described in detail in the accompanying papers. In addition, we describe the satellite performance elements which are most relevant for science, and provide an overview of the plans for scientific operations and data analysis.
Published: 2010

27. The Planck High Frequency Instrument, a third generation CMB experiment, and a full sky submillimeter survey

Author: Lamarre, J.-M., Puget, J.-L., Bouchet, F.R., Ade, P.A.R., Benoit, A., Bernard, J.-P., Bock, J.J., De Bernardis, P., Charra, J., Couchot, F., Delabrouille, J., Efstathiou, G., Giard, M., Guyot, G., Lange, A.E., Maffei, B., Murphy, J.Anthony, Pajot, F., Piat, M., Ristorcelli, I., Santos, D., Sudiwala, R., Sygnet, J.-F., Torre, J.-P., Yurchenko, V., Yvon, D., Lamarre, J.-M., Puget, J.-L., Bouchet, F.R., Ade, P.A.R., Benoit, A., Bernard, J.-P., Bock, J.J., De Bernardis, P., Charra, J., Couchot, F., Delabrouille, J., Efstathiou, G., Giard, M., Guyot, G., Lange, A.E., Maffei, B., Murphy, J.Anthony, Pajot, F., Piat, M., Ristorcelli, I., Santos, D., Sudiwala, R., Sygnet, J.-F., Torre, J.-P., Yurchenko, V., and Yvon, D.
Abstract: The High Frequency Instrument (HFI) of Planck is the most sensitive CMB experiment ever planned. Statistical fluctuations (photon noise) of the CMB itself will be the major limitation to the sensitivity of the CMB channels. Higher frequency channels will measure galactic foregrounds. Together with the Low Frequency Instrument, this will make a unique tool to measure the full sky and to separate the various components of its spectrum. Measurement of the polarization of these various components will give a new picture of the CMB. In addition, HFI will provide the scientific community with new full sky maps of intensity and polarization at six frequencies, with unprecedented angular resolution and sensitivity. This paper describes the logics that prevailed to define the HFI and the performances expected from this instrument. It details several features of the HFI design that has not been published up to now.
Published: 2003

28. Planckpre-launch status: ThePlanckmission

Author: Tauber, J. A., primary, Mandolesi, N., additional, Puget, J.-L., additional, Banos, T., additional, Bersanelli, M., additional, Bouchet, F. R., additional, Butler, R. C., additional, Charra, J., additional, Crone, G., additional, Dodsworth, J., additional, Efstathiou, G., additional, Gispert, R., additional, Guyot, G., additional, Gregorio, A., additional, Juillet, J. J., additional, Lamarre, J.-M., additional, Laureijs, R. J., additional, Lawrence, C. R., additional, Nørgaard-Nielsen, H. U., additional, Passvogel, T., additional, Reix, J. M., additional, Texier, D., additional, Vibert, L., additional, Zacchei, A., additional, Ade, P. A. R., additional, Aghanim, N., additional, Aja, B., additional, Alippi, E., additional, Aloy, L., additional, Armand, P., additional, Arnaud, M., additional, Arondel, A., additional, Arreola-Villanueva, A., additional, Artal, E., additional, Artina, E., additional, Arts, A., additional, Ashdown, M., additional, Aumont, J., additional, Azzaro, M., additional, Bacchetta, A., additional, Baccigalupi, C., additional, Baker, M., additional, Balasini, M., additional, Balbi, A., additional, Banday, A. J., additional, Barbier, G., additional, Barreiro, R. B., additional, Bartelmann, M., additional, Battaglia, P., additional, Battaner, E., additional, Benabed, K., additional, Beney, J.-L., additional, Beneyton, R., additional, Bennett, K., additional, Benoit, A., additional, Bernard, J.-P., additional, Bhandari, P., additional, Bhatia, R., additional, Biggi, M., additional, Biggins, R., additional, Billig, G., additional, Blanc, Y., additional, Blavot, H., additional, Bock, J. J., additional, Bonaldi, A., additional, Bond, R., additional, Bonis, J., additional, Borders, J., additional, Borrill, J., additional, Boschini, L., additional, Boulanger, F., additional, Bouvier, J., additional, Bouzit, M., additional, Bowman, R., additional, Bréelle, E., additional, Bradshaw, T., additional, Braghin, M., additional, Bremer, M., additional, Brienza, D., additional, Broszkiewicz, D., additional, Burigana, C., additional, Burkhalter, M., additional, Cabella, P., additional, Cafferty, T., additional, Cairola, M., additional, Caminade, S., additional, Camus, P., additional, Cantalupo, C. M., additional, Cappellini, B., additional, Cardoso, J.-F., additional, Carr, R., additional, Catalano, A., additional, Cayón, L., additional, Cesa, M., additional, Chaigneau, M., additional, Challinor, A., additional, Chamballu, A., additional, Chambelland, J. P., additional, Charra, M., additional, Chiang, L.-Y., additional, Chlewicki, G., additional, Christensen, P. R., additional, Church, S., additional, Ciancietta, E., additional, Cibrario, M., additional, Cizeron, R., additional, Clements, D., additional, Collaudin, B., additional, Colley, J.-M., additional, Colombi, S., additional, Colombo, A., additional, Colombo, F., additional, Corre, O., additional, Couchot, F., additional, Cougrand, B., additional, Coulais, A., additional, Couzin, P., additional, Crane, B., additional, Crill, B., additional, Crook, M., additional, Crumb, D., additional, Cuttaia, F., additional, Dörl, U., additional, da Silva, P., additional, Daddato, R., additional, Damasio, C., additional, Danese, L., additional, d'Aquino, G., additional, D'Arcangelo, O., additional, Dassas, K., additional, Davies, R. D., additional, Davies, W., additional, Davis, R. J., additional, De Bernardis, P., additional, de Chambure, D., additional, de Gasperis, G., additional, De la Fuente, M. L., additional, De Paco, P., additional, De Rosa, A., additional, De Troia, G., additional, De Zotti, G., additional, Dehamme, M., additional, Delabrouille, J., additional, Delouis, J.-M., additional, Désert, F.-X., additional, di Girolamo, G., additional, Dickinson, C., additional, Doelling, E., additional, Dolag, K., additional, Domken, I., additional, Douspis, M., additional, Doyle, D., additional, Du, S., additional, Dubruel, D., additional, Dufour, C., additional, Dumesnil, C., additional, Dupac, X., additional, Duret, P., additional, Eder, C., additional, Elfving, A., additional, Enßlin, T. A., additional, Eng, P., additional, English, K., additional, Eriksen, H. K., additional, Estaria, P., additional, Falvella, M. C., additional, Ferrari, F., additional, Finelli, F., additional, Fishman, A., additional, Fogliani, S., additional, Foley, S., additional, Fonseca, A., additional, Forma, G., additional, Forni, O., additional, Fosalba, P., additional, Fourmond, J.-J., additional, Frailis, M., additional, Franceschet, C., additional, Franceschi, E., additional, François, S., additional, Frerking, M., additional, Gómez-Reñasco, M. F., additional, Górski, K. M., additional, Gaier, T. C., additional, Galeotta, S., additional, Ganga, K., additional, García Lázaro, J., additional, Garnica, A., additional, Gaspard, M., additional, Gavila, E., additional, Giard, M., additional, Giardino, G., additional, Gienger, G., additional, Giraud-Heraud, Y., additional, Glorian, J.-M., additional, Griffin, M., additional, Gruppuso, A., additional, Guglielmi, L., additional, Guichon, D., additional, Guillaume, B., additional, Guillouet, P., additional, Haissinski, J., additional, Hansen, F. K., additional, Hardy, J., additional, Harrison, D., additional, Hazell, A., additional, Hechler, M., additional, Heckenauer, V., additional, Heinzer, D., additional, Hell, R., additional, Henrot-Versillé, S., additional, Hernández-Monteagudo, C., additional, Herranz, D., additional, Herreros, J. M., additional, Hervier, V., additional, Heske, A., additional, Heurtel, A., additional, Hildebrandt, S. R., additional, Hills, R., additional, Hivon, E., additional, Hobson, M., additional, Hollert, D., additional, Holmes, W., additional, Hornstrup, A., additional, Hovest, W., additional, Hoyland, R. J., additional, Huey, G., additional, Huffenberger, K. M., additional, Hughes, N., additional, Israelsson, U., additional, Jackson, B., additional, Jaffe, A., additional, Jaffe, T. R., additional, Jagemann, T., additional, Jessen, N. C., additional, Jewell, J., additional, Jones, W., additional, Juvela, M., additional, Kaplan, J., additional, Karlman, P., additional, Keck, F., additional, Keihänen, E., additional, King, M., additional, Kisner, T. S., additional, Kletzkine, P., additional, Kneissl, R., additional, Knoche, J., additional, Knox, L., additional, Koch, T., additional, Krassenburg, M., additional, Kurki-Suonio, H., additional, Lähteenmäki, A., additional, Lagache, G., additional, Lagorio, E., additional, Lami, P., additional, Lande, J., additional, Lange, A., additional, Langlet, F., additional, Lapini, R., additional, Lapolla, M., additional, Lasenby, A., additional, Le Jeune, M., additional, Leahy, J. P., additional, Lefebvre, M., additional, Legrand, F., additional, Le Meur, G., additional, Leonardi, R., additional, Leriche, B., additional, Leroy, C., additional, Leutenegger, P., additional, Levin, S. M., additional, Lilje, P. B., additional, Lindensmith, C., additional, Linden-Vørnle, M., additional, Loc, A., additional, Longval, Y., additional, Lubin, P. M., additional, Luchik, T., additional, Luthold, I., additional, Macias-Perez, J. F., additional, Maciaszek, T., additional, MacTavish, C., additional, Madden, S., additional, Maffei, B., additional, Magneville, C., additional, Maino, D., additional, Mambretti, A., additional, Mansoux, B., additional, Marchioro, D., additional, Maris, M., additional, Marliani, F., additional, Marrucho, J.-C., additional, Martí-Canales, J., additional, Martínez-González, E., additional, Martín-Polegre, A., additional, Martin, P., additional, Marty, C., additional, Marty, W., additional, Masi, S., additional, Massardi, M., additional, Matarrese, S., additional, Matthai, F., additional, Mazzotta, P., additional, McDonald, A., additional, McGrath, P., additional, Mediavilla, A., additional, Meinhold, P. R., additional, Mélin, J.-B., additional, Melot, F., additional, Mendes, L., additional, Mennella, A., additional, Mervier, C., additional, Meslier, L., additional, Miccolis, M., additional, Miville-Deschenes, M.-A., additional, Moneti, A., additional, Montet, D., additional, Montier, L., additional, Mora, J., additional, Morgante, G., additional, Morigi, G., additional, Morinaud, G., additional, Morisset, N., additional, Mortlock, D., additional, Mottet, S., additional, Mulder, J., additional, Munshi, D., additional, Murphy, A., additional, Murphy, P., additional, Musi, P., additional, Narbonne, J., additional, Naselsky, P., additional, Nash, A., additional, Nati, F., additional, Natoli, P., additional, Netterfield, B., additional, Newell, J., additional, Nexon, M., additional, Nicolas, C., additional, Nielsen, P. H., additional, Ninane, N., additional, Noviello, F., additional, Novikov, D., additional, Novikov, I., additional, O'Dwyer, I. J., additional, Oldeman, P., additional, Olivier, P., additional, Ouchet, L., additional, Oxborrow, C. A., additional, Pérez-Cuevas, L., additional, Pagan, L., additional, Paine, C., additional, Pajot, F., additional, Paladini, R., additional, Pancher, F., additional, Panh, J., additional, Parks, G., additional, Parnaudeau, P., additional, Partridge, B., additional, Parvin, B., additional, Pascual, J. P., additional, Pasian, F., additional, Pearson, D. P., additional, Pearson, T., additional, Pecora, M., additional, Perdereau, O., additional, Perotto, L., additional, Perrotta, F., additional, Piacentini, F., additional, Piat, M., additional, Pierpaoli, E., additional, Piersanti, O., additional, Plaige, E., additional, Plaszczynski, S., additional, Platania, P., additional, Pointecouteau, E., additional, Polenta, G., additional, Ponthieu, N., additional, Popa, L., additional, Poulleau, G., additional, Poutanen, T., additional, Prézeau, G., additional, Pradell, L., additional, Prina, M., additional, Prunet, S., additional, Rachen, J. P., additional, Rambaud, D., additional, Rame, F., additional, Rasmussen, I., additional, Rautakoski, J., additional, Reach, W. T., additional, Rebolo, R., additional, Reinecke, M., additional, Reiter, J., additional, Renault, C., additional, Ricciardi, S., additional, Rideau, P., additional, Riller, T., additional, Ristorcelli, I., additional, Riti, J. B., additional, Rocha, G., additional, Roche, Y., additional, Pons, R., additional, Rohlfs, R., additional, Romero, D., additional, Roose, S., additional, Rosset, C., additional, Rouberol, S., additional, Rowan-Robinson, M., additional, Rubiño-Martín, J. A., additional, Rusconi, P., additional, Rusholme, B., additional, Salama, M., additional, Salerno, E., additional, Sandri, M., additional, Santos, D., additional, Sanz, J. L., additional, Sauter, L., additional, Sauvage, F., additional, Savini, G., additional, Schmelzel, M., additional, Schnorhk, A., additional, Schwarz, W., additional, Scott, D., additional, Seiffert, M. D., additional, Shellard, P., additional, Shih, C., additional, Sias, M., additional, Silk, J. I., additional, Silvestri, R., additional, Sippel, R., additional, Smoot, G. F., additional, Starck, J.-L., additional, Stassi, P., additional, Sternberg, J., additional, Stivoli, F., additional, Stolyarov, V., additional, Stompor, R., additional, Stringhetti, L., additional, Strommen, D., additional, Stute, T., additional, Sudiwala, R., additional, Sugimura, R., additional, Sunyaev, R., additional, Sygnet, J.-F., additional, Türler, M., additional, Taddei, E., additional, Tallon, J., additional, Tamiatto, C., additional, Taurigna, M., additional, Taylor, D., additional, Terenzi, L., additional, Thuerey, S., additional, Tillis, J., additional, Tofani, G., additional, Toffolatti, L., additional, Tommasi, E., additional, Tomasi, M., additional, Tonazzini, E., additional, Torre, J.-P., additional, Tosti, S., additional, Touze, F., additional, Tristram, M., additional, Tuovinen, J., additional, Tuttlebee, M., additional, Umana, G., additional, Valenziano, L., additional, Vallée, D., additional, van der Vlis, M., additional, Van Leeuwen, F., additional, Vanel, J.-C., additional, Van-Tent, B., additional, Varis, J., additional, Vassallo, E., additional, Vescovi, C., additional, Vezzu, F., additional, Vibert, D., additional, Vielva, P., additional, Vierra, J., additional, Villa, F., additional, Vittorio, N., additional, Vuerli, C., additional, Wade, L. A., additional, Walker, A. R., additional, Wandelt, B. D., additional, Watson, C., additional, Werner, D., additional, White, M., additional, White, S. D. M., additional, Wilkinson, A., additional, Wilson, P., additional, Woodcraft, A., additional, Yoffo, B., additional, Yun, M., additional, Yurchenko, V., additional, Yvon, D., additional, Zhang, B., additional, Zimmermann, O., additional, Zonca, A., additional, and Zorita, D., additional
Published: 2010
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29. Planckpre-launch status: HFI ground calibration

Author: Pajot, F., primary, Ade, P. A. R., additional, Beney, J.-L., additional, Bréelle, E., additional, Broszkiewicz, D., additional, Camus, P., additional, Carabétian, C., additional, Catalano, A., additional, Chardin, A., additional, Charra, M., additional, Charra, J., additional, Cizeron, R., additional, Couchot, F., additional, Coulais, A., additional, Crill, B. P., additional, Dassas, K., additional, Daubin, J., additional, de Bernardis, P., additional, de Marcillac, P., additional, Delouis, J.-M., additional, Désert, F.-X., additional, Duret, P., additional, Eng, P., additional, Evesque, C., additional, Fourmond, J.-J., additional, François, S., additional, Giard, M., additional, Giraud-Héraud, Y., additional, Guglielmi, L., additional, Guyot, G., additional, Haissinski, J., additional, Henrot-Versillé, S., additional, Hervier, V., additional, Holmes, W., additional, Jones, W. C., additional, Lamarre, J.-M., additional, Lami, P., additional, Lange, A. E., additional, Lefebvre, M., additional, Leriche, B., additional, Leroy, C., additional, Macias-Perez, J., additional, Maciaszek, T., additional, Maffei, B., additional, Mahendran, A., additional, Mansoux, B., additional, Marty, C., additional, Masi, S., additional, Mercier, C., additional, Miville-Deschenes, M.-A., additional, Montier, L., additional, Nicolas, C., additional, Noviello, F., additional, Perdereau, O., additional, Piacentini, F., additional, Piat, M., additional, Plaszczynski, S., additional, Pointecouteau, E., additional, Pons, R., additional, Ponthieu, N., additional, Puget, J.-L., additional, Rambaud, D., additional, Renault, C., additional, Renault, J.-C., additional, Rioux, C., additional, Ristorcelli, I., additional, Rosset, C., additional, Savini, G., additional, Sudiwala, R., additional, Torre, J.-P., additional, Tristram, M., additional, Vallée, D., additional, Veneziani, M., additional, and Yvon, D., additional
Published: 2010
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30. Planckpre-launch status: The HFI instrument, from specification to actual performance

Author: Lamarre, J.-M., primary, Puget, J.-L., additional, Ade, P. A. R., additional, Bouchet, F., additional, Guyot, G., additional, Lange, A. E., additional, Pajot, F., additional, Arondel, A., additional, Benabed, K., additional, Beney, J.-L., additional, Benoît, A., additional, Bernard, J.-Ph., additional, Bhatia, R., additional, Blanc, Y., additional, Bock, J. J., additional, Bréelle, E., additional, Bradshaw, T. W., additional, Camus, P., additional, Catalano, A., additional, Charra, J., additional, Charra, M., additional, Church, S. E., additional, Couchot, F., additional, Coulais, A., additional, Crill, B. P., additional, Crook, M. R., additional, Dassas, K., additional, de Bernardis, P., additional, Delabrouille, J., additional, de Marcillac, P., additional, Delouis, J.-M., additional, Désert, F.-X., additional, Dumesnil, C., additional, Dupac, X., additional, Efstathiou, G., additional, Eng, P., additional, Evesque, C., additional, Fourmond, J.-J., additional, Ganga, K., additional, Giard, M., additional, Gispert, R., additional, Guglielmi, L., additional, Haissinski, J., additional, Henrot-Versillé, S., additional, Hivon, E., additional, Holmes, W. A., additional, Jones, W. C., additional, Koch, T. C., additional, Lagardère, H., additional, Lami, P., additional, Landé, J., additional, Leriche, B., additional, Leroy, C., additional, Longval, Y., additional, Macías-Pérez, J. F., additional, Maciaszek, T., additional, Maffei, B., additional, Mansoux, B., additional, Marty, C., additional, Masi, S., additional, Mercier, C., additional, Miville-Deschênes, M.-A., additional, Moneti, A., additional, Montier, L., additional, Murphy, J. A., additional, Narbonne, J., additional, Nexon, M., additional, Paine, C. G., additional, Pahn, J., additional, Perdereau, O., additional, Piacentini, F., additional, Piat, M., additional, Plaszczynski, S., additional, Pointecouteau, E., additional, Pons, R., additional, Ponthieu, N., additional, Prunet, S., additional, Rambaud, D., additional, Recouvreur, G., additional, Renault, C., additional, Ristorcelli, I., additional, Rosset, C., additional, Santos, D., additional, Savini, G., additional, Serra, G., additional, Stassi, P., additional, Sudiwala, R. V., additional, Sygnet, J.-F., additional, Tauber, J. A., additional, Torre, J.-P., additional, Tristram, M., additional, Vibert, L., additional, Woodcraft, A., additional, Yurchenko, V., additional, and Yvon, D., additional
Published: 2010
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31. The High Frequency Instrument of Planck: Design and Performances

Author: Lamarre, J.-M., Ade, P.A.R., Benoit, A., De Bernardis, P., Bock, J.J., Bouchet, F.R., Bradshaw, T., Charra, J., Church, S., Couchot, F., Delabrouille, J., Efstathiou, G., Giard, M., Giraud-Héraud, Y., Gispert, R., Griffin, M., Lange, A.E., Murphy, J.Anthony, Pajot, F., Puget, J.-L., Ristorcelli, I., Lamarre, J.-M., Ade, P.A.R., Benoit, A., De Bernardis, P., Bock, J.J., Bouchet, F.R., Bradshaw, T., Charra, J., Church, S., Couchot, F., Delabrouille, J., Efstathiou, G., Giard, M., Giraud-Héraud, Y., Gispert, R., Griffin, M., Lange, A.E., Murphy, J.Anthony, Pajot, F., Puget, J.-L., and Ristorcelli, I.
Abstract: The abstract is included in the text.
Published: 2000

32. Global solar Doppler velocity determination with the GOLF/SoHO instrument

Author: García, R. A., primary, Turck-Chièze, S., additional, Boumier, P., additional, Robillot, J. M., additional, Bertello, L., additional, Charra, J., additional, Dzitko, H., additional, Gabriel, A. H., additional, Jiménez-Reyes, S. J., additional, Pallé, P. L., additional, Renaud, C., additional, Roca Cortés, T., additional, and Ulrich, R. K., additional
Published: 2005
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33. The Planck High Frequency Instrument, a third generation CMB experiment, and a full sky submillimeter survey

Author: Lamarre, J.M, primary, Puget, J.L, additional, Bouchet, F, additional, Ade, P.A.R, additional, Benoit, A, additional, Bernard, J.P, additional, Bock, J, additional, De Bernardis, P, additional, Charra, J, additional, Couchot, F, additional, Delabrouille, J, additional, Efstathiou, G, additional, Giard, M, additional, Guyot, G, additional, Lange, A, additional, Maffei, B, additional, Murphy, A, additional, Pajot, F, additional, Piat, M, additional, Ristorcelli, I, additional, Santos, D, additional, Sudiwala, R, additional, Sygnet, J.F, additional, Torre, J.P, additional, Yurchenko, V, additional, and Yvon, D, additional
Published: 2003
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34. A search for solar $\vec{g}$ modes in the GOLF data

Author: Gabriel, A. H., primary, Baudin, F., additional, Boumier, P., additional, García, R. A., additional, Turck-Chièze, S., additional, Appourchaux, T., additional, Bertello, L., additional, Berthomieu, G., additional, Charra, J., additional, Gough, D. O., additional, Pallé, P. L., additional, Provost, J., additional, Renaud, C., additional, Robillot, J.-M., additional, Roca Cortés, T., additional, Thiery, S., additional, and Ulrich, R. K., additional
Published: 2002
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35. A search for solar $\vec{g}$modes in the GOLF data

Author: Gabriel, A. H., Baudin, F., Boumier, P., García, R. A., Turck-Chièze, S., Appourchaux, T., Bertello, L., Berthomieu, G., Charra, J., Gough, D. O., Pallé, P. L., Provost, J., Renaud, C., Robillot, J.-M., Roca Cortés, T., Thiery, S., Ulrich, R. K., Gabriel, A. H., Baudin, F., Boumier, P., García, R. A., Turck-Chièze, S., Appourchaux, T., Bertello, L., Berthomieu, G., Charra, J., Gough, D. O., Pallé, P. L., Provost, J., Renaud, C., Robillot, J.-M., Roca Cortés, T., Thiery, S., and Ulrich, R. K.
Abstract: With over 5 years of GOLF data having some 90% continuity, a new attempt has been made to search for possible solar gmodes. Statistical methods are used, based on the minimum of assumptions regarding the solar physics; namely that mode line-widths are small compared with the inverse of the observing time, and that modes are sought in the frequency interval 150 to 400 μHz. A number of simulations are carried out in order to understand the expected behaviour of a system consisting principally of a solar noise continuum overlaid with some weak sharp resonances. The method adopted is based on the FFT analysis of a time series with zero-padding by a factor of 5. One prominent resonance at 284.666 μHz coincides with a previous tentative assignment as one member of an $n=1$, $l=1$, p-mode multiplet. Components of two multiplets, previously tentatively identified as possible g-mode candidates from the GOLF data in 1998, continue to be found, although their statistical significance is shown to be insufficient, within the present assumption regarding the nature of the signal. An upper limit to the amplitude of any gmode present is calculated using two different statistical approaches, according to either the assumed absence (H0 hypothesis) or the assumed presence (H1 hypothesis) of a signal. The former yields a slightly lower limit of around 6 mm/s.
Published: 2002
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36. Global Oscillations at Low Frequency from the SOHO mission (GOLF)

Author: Gabriel, A. H., primary, Grec, G., additional, Charra, J., additional, Robillot, J. -M., additional, Roca Cortés, T., additional, Turck-Chièze, S., additional, Bocchia, R., additional, Boumier, P., additional, Cantin, M., additional, Cespédes, E., additional, Cougrand, B., additional, Crétolle, J., additional, Damé, L., additional, Decaudin, M., additional, Delache, P., additional, Denis, N., additional, Duc, R., additional, Dzitko, H., additional, Fossat, E., additional, Fourmond, J. -J., additional, García, R. A., additional, Gough, D., additional, Grivel, C., additional, Herreros, J. M., additional, Lagardère, H., additional, Moalic, J. -P., additional, Pallé, P. L., additional, Pétrou, N., additional, Sanchez, M., additional, Ulrich, R., additional, and van der Raay, H. B., additional
Published: 1995
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37. The High Frequency Instrument of Planck: Design and Performances.

Author: Lamarre, J.M., Ade, P.A.R., Benoit, A., de Bernardis, P., Bock, J., Bouchet, F., Bradshaw, T., Charra, J., Church, S., Couchot, F., Delabrouille, J., Efstathiou, G., Giard, M., Giraud-Heraud, Y., Gispert, R., Griffin, M., Lange, A., Murphy, A., and Pajot, F.
Subjects: ASTRONOMICAL instruments, COSMIC background radiation
Abstract: Deals with the design and performances of the Planck High Frequency Instrument (HFI) of the European Space Authority. Importance of the planck cosmic microwave background measurements for cosmologists; Architecture of the Planck HFI.
Published: 1998

38. Performance and Early Results from the Golf Instrument Flown on the Soho Mission.

Author: Gabriel, A., Charra, J., Grec, G., Robillot, J.-M., Roca Cortés, T., Turck-Chièze, S., Ulrich, R., Basu, S., Baudin, F., Bertello, L., Boumier, P., Charra, M., Christensen-Dalsgaard, J., Decaudin, M., Dzitko, H., Foglizzo, T., Fossat, E., García, R., Herreros, J., and Lazrek, M.
Abstract: GOLF in-flight commissioning and calibration was carried out during the first four months, most of which represented the cruise phase of SOHO towards its final L1 orbit. The initial performance of GOLF is shown to be within the design specification, for the entire instrument as well as for the separate sub-systems. Malfunctioning of the polarising mechanisms after 3 to 4 months operation has led to the adoption of an unplanned operating sequence in which these mechanisms are no longer used. This mode, which measures only the blue wing of the solar sodium lines, detracts little from the detection and frequency measurements of global oscillations, but does make more difficult the absolute velocity calibration, which is currently of the order of 20%. Data continuity in the new mode is extremely high and the instrument is producing exceptionally noise-free p-mode spectra. The data set is particularly well suited to the study of effects due to the excitation mechanism of the modes, leading to temporal variations in their amplitudes. The g modes have not yet been detected in this limited data set. In the present mode of operation, there are no indications of any degradation which would limit the use of GOLF for up to 6 years or more. [ABSTRACT FROM AUTHOR]
Published: 1997
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39. A 30-cm objective grating for far-UV astronomy: theoretical study and laboratory tests

Author: Prangé, Renée, Duban, Michel, Vidal-Madjar, Alfred, Barnstedt, Jürgen, Parisot, D., Decaudin, M., Crussaire, J. P., Laurent, C., Labèque, A., Ancourt, G., Flamand, J., Grewing, M., Hoekstra, R., Thévenon, A., Bargot, G., Barthélémy, M., Canovas, F., Charra, J., Hallier, C., Lagardère, H., Levanti, G., Michaud, G., and Poncet, H.
Abstract: We have performed theoretical determination and experimental calibrations of an objective grating designed for high resolution spectroscopy of astronomical faint sources in the EUV and far-UV wavelength ranges (500–1400 Å). First through theoretical calculations we show the feasibility of the concept with an aspheric shape for the grating blank and determine its geometrical parameters. A grating of this large size has been manufactured and tested, associated with a photon counting detector, in a vacuum environment. Finally we demonstrate that a resolving power of 3 × 10^4, a total equivalent effective area of ~5–10 cm^2 can be achieved, together with a very low scattered light level (10^−4–10^−5 of the peak value).
Published: 1989

40. Actual Status and Early Results from GOLF Experiment on-board SOHO

Author: Roca Cortes, T., Gabriel, A. H., Charra, J., Grec, G., Ulrich, R. K., Turck-Chieze, S., Robillot, J. M., Boumier, P., Regulo, C., Baudin, F., Lazrek, M., Garcia, R. A., Palle, P. L., and Golf, Team

41. Stability Study of the GOLF Blue Wing Working Cycle

Author: Robillot, J. M., Turck-Chieze, S., Garcia, R. A., Boumier, P., Charra, J., Ulrich, R. K., Gabriel, A., Grec, G., and Roca Cortes, T.

42. Sensitivity of the GOLF signal to combined solar velocity and intensity variations

Author: Ulrich, R. K., García, R. A., Robillot, J. -M, Turck-Chièze, S., Luca Bertello, Charra, J., Dzitko, H., Gabriel, A. H., and Roca Cortés, T.

43. The integrated magnetic field of the Sun as seen by GOLF on board SOHO

Author: Rafael A. García, Boumier, P., Charra, J., Foglizzo, T., Gabriel, A. H., Grec, G., Régulo, C., Robillot, J. M., Turck-Chièze, S., and Ulrich, R. K.

44. Infrared sounding of comet Halley from Vega 1

Author: Combes, M., primary, Moroz, V. I., additional, Crifo, J. F., additional, Lamarre, J. M., additional, Charra, J., additional, Sanko, N. F., additional, Soufflot, A., additional, Bibring, J. P., additional, Cazes, S., additional, Coron, N., additional, Crovisier, J., additional, Emerich, C., additional, Encrenaz, T., additional, Gispert, R., additional, Grigoryev, A. V., additional, Guyot, G., additional, Krasnopolsky, V. A., additional, Nikolsky, Yu. V., additional, and Rocard, F., additional
Published: 1986
Full Text: View/download PDF

45. The instrument IKS and its calibration

Author: Cazes, S., primary, Charra, J., additional, Coron, N., additional, Cougrand, B., additional, Crifo, J.-F., additional, Crovisier, J., additional, Emerich, C., additional, Gispert, R., additional, Gondet, B., additional, Guyot, G., additional, Harduin, D., additional, Lamarre, J.-M., additional, Levanti, G., additional, Maurel, C., additional, Parisot, D., additional, Rocard, F., additional, Salvetat, P., additional, Soufflot, A., additional, Bibring, J.-P., additional, Combes, M., additional, and Encrenaz, T., additional
Published: 1984
Full Text: View/download PDF

46. Calibrated full disk solar H I Lyman-alpha and Lyman-beta profiles

Author: Lemaire, P., primary, Charra, J., additional, Jouchoux, A., additional, Vidal-Madjar, A., additional, Artzner, G. E., additional, Vial, J. C., additional, Bonnet, R. M., additional, and Skumanich, A., additional
Published: 1978
Full Text: View/download PDF

47. Conclusion

Author: Nicoud, Marilyn, Histoire, Archéologie et Littératures des mondes chrétiens et musulmans médiévaux (CIHAM), École normale supérieure - Lyon (ENS Lyon)-Université Lumière - Lyon 2 (UL2)-École des hautes études en sciences sociales (EHESS)-Université Jean Moulin - Lyon 3 (UJML), Université de Lyon-Université de Lyon-Avignon Université (AU)-Centre National de la Recherche Scientifique (CNRS), V. Giacomotto-Charra, J. Vons, and École normale supérieure de Lyon (ENS de Lyon)-Université Lumière - Lyon 2 (UL2)-École des hautes études en sciences sociales (EHESS)-Université Jean Moulin - Lyon 3 (UJML)
Subjects: [SHS.HISPHILSO]Humanities and Social Sciences/History, Philosophy and Sociology of Sciences, [SHS.LITT]Humanities and Social Sciences/Literature, [SHS.HIST]Humanities and Social Sciences/History, ComputingMilieux_MISCELLANEOUS
Abstract: International audience
Published: 2017

48. Un aspect de la réception du De Generatione : la définition des éléments dans la physique vulgarisée du XVIe siècle

Author: Giacomotto-Charra, Violaine, Textes, littératures, écritures et modèles (TELEM), Université Bordeaux Montaigne, and V. Giacomotto-Charra, J. Ducos
Subjects: ComputingMilieux_MISCELLANEOUS, [SHS]Humanities and Social Sciences
Abstract: International audience
Published: 2011

49. « Lire Aristote au Moyen Age et à la Renaissance : enjeux et problématique », avec J. Ducos

Author: Giacomotto-Charra, Violaine, Textes, littératures, écritures et modèles (TELEM), Université Bordeaux Montaigne, and V. Giacomotto-Charra, J. Ducos
Subjects: ComputingMilieux_MISCELLANEOUS, [SHS]Humanities and Social Sciences
Abstract: International audience
Published: 2011

50. Planck pre-launch status: The Planck mission

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Boschini18, F. Boulanger3, J. Bouvier28, M. Bouzit3, R. Bowman12, E. Bréelle38, T. Bradshaw39, M. Braghin7, M. Bremer1, D. Brienza40, D. Broszkiewicz38, C. Burigana2, M. Burkhalter41, P. Cabella25, T. Cafferty12, M. Cairola23, S. Caminade3, P. Camus42, C. M. Cantalupo43, B. Cappellini5, J.-F. Cardoso38, R. Carr14, A. Catalano38, L. Cayón44, M. Cesa23, M. Chaigneau3, A. Challinor9, A. Chamballu45, J. P. Chambelland4, M. Charra3, L.-Y. Chiang46, G. Chlewicki23, P. R. Christensen47, S. Church48, E. Ciancietta23, M. Cibrario23, R. Cizeron32, D. Clements45, B. Collaudin4, J.-M. Colley38, 6, S. Colombi6, A. Colombo7, F. Colombo18, O. Corre4, F. Couchot32, B. Cougrand3, A. Coulais11, P. Couzin4, B. Crane3, B. Crill12, M. Crook39, D. Crumb12, F. Cuttaia2, U. Dörl26, P. da Silva6, R. Daddato7, C. Damasio7, L. Danese24, G. d'Aquino7, O. D'Arcangelo49, K. Dassas3, R. D. Davies50, W. Davies41, R. J. Davis50, P. De Bernardis40, D. de Chambure7, G. de Gasperis25, M. L. De la Fuente17, P. 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Beney, J, Bernard, J, Bock, J, Bréelle, E, Cantalupo, C, Cardoso, J, Cayón, L, Chambelland, J, Chiang, L, Christensen, P, Colley, J, Dörl, U, D'Aquino, G, D'Arcangelo, O, Davies, R, Davis, R, DE LA FUENTE, M, Delouis, J, Désert, F, Enlin, T, Eriksen, H, Falvella, M, Fourmond, J, Frailis, M, Franceschet, C, Franceschi, E, François, S, Frerking, M, GÓMEZ REÑASCO, M, Górski, K, Gaier, T, Galeotta, S, Ganga, K, GARCÍA LÁZARO, J, Garnica, A, Gaspard, M, Gavila, E, Giard, M, Giardino, G, Gienger, G, GIRAUD HERAUD, Y, Glorian, J, Griffin, M, Gruppuso, A, Guglielmi, L, Guichon, D, Guillaume, B, Guillouet, P, Haissinski, J, Hansen, F, Hardy, J, Harrison, D, Hazell, A, Hechler, M, Heckenauer, V, Heinzer, D, Hell, R, HENROT VERSILLÉ, S, HERNÁNDEZ MONTEAGUDO, C, Herranz, D, Herreros, J, Hervier, V, Heske, A, Heurtel, A, Hildebrandt, S, Hills, R, Hivon, E, Hobson, M, Hollert, D, Holmes, W, Hornstrup, A, Hovest, W, Hoyland, R, Huey, G, Huffenberger, K, Hughes, N, Israelsson, U, Jackson, B, Jaffe, A, Jaffe, T, Jagemann, T, Jessen, N, Jewell, J, Jones, W, Juvela, M, Kaplan, J, Karlman, P, Keck, F, Keihänen, E, King, M, Kisner, T, Kletzkine, P, Kneissl, R, Knoche, J, Knox, L, Koch, T, Krassenburg, M, KURKI SUONIO, H, Lähteenmäki, A, Lagache, G, Lagorio, E, Lami, P, Lande, J, Lange, A, Langlet, F, Lapini, R, Lapolla, M, Lasenby, A, LE JEUNE, M, Leahy, J, Lefebvre, M, Legrand, F, LE MEUR, G, Leonardi, R, Leriche, B, Leroy, C, Leutenegger, P, Levin, S, Lilje, P, Lindensmith, C, LINDEN VØRNLE, M, Loc, A, Longval, Y, Lubin, P, Luchik, T, Luthold, I, MACIAS PEREZ, J, Maciaszek, T, Mactavish, C, Madden, S, Maffei, B, Magneville, C, Maino, D, Mambretti, A, Mansoux, B, Marchioro, D, Maris, M, Marliani, F, Marrucho, J, MARTÍ CANALES, J, MARTÍNEZ GONZÁLEZ, E, MARTÍN POLEGRE, A, Martin, P, Marty, C, Marty, W, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, Mcdonald, A, Mcgrath, P, Mediavilla, A, Meinhold, P, Mélin, J, Melot, F, Mendes, L, Mennella, A, Mervier, C, Meslier, L, Miccolis, M, MIVILLE DESCHENES, M, Moneti, A, Montet, D, Montier, L, Mora, J, Morgante, G, Morigi, G, Morinaud, G, Morisset, N, Mortlock, D, Mottet, S, Mulder, J, Munshi, D, Murphy, A, Murphy, P, Musi, P, Narbonne, J, Naselsky, P, Nash, A, Nati, F, Natoli, P, Netterfield, B, Newell, J, Nexon, M, Nicolas, C, Nielsen, P, Ninane, N, Noviello, F, Novikov, D, Novikov, I, O'Dwyer, I, Oldeman, P, Olivier, P, Ouchet, L, Oxborrow, C, PÉREZ CUEVAS, L, Pagan, L, Paine, C, Pajot, F, Paladini, R, Pancher, F, Panh, J, Parks, G, Parnaudeau, P, Partridge, B, Parvin, B, Pascual, J, Pasian, F, Pearson, D, Pearson, T, Pecora, M, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Piersanti, O, Plaige, E, Plaszczynski, S, Platania, P, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poulleau, G, Poutanen, T, Prézeau, G, Pradell, L, Prina, M, Prunet, S, Rachen, J, Rambaud, D, Rame, F, Rasmussen, I, Rautakoski, J, Reach, W, Rebolo, R, Reinecke, M, Reiter, J, Renault, C, Ricciardi, S, Rideau, P, Riller, T, Ristorcelli, I, Riti, J, Rocha, G, Roche, Y, Pons, R, Rohlfs, R, Romero, D, Roose, S, Rosset, C, Rouberol, S, ROWAN ROBINSON, M, RUBIÑO MARTÍN, J, Rusconi, P, Rusholme, B, Salama, M, Salerno, E, Sandri, M, Santos, D, Sanz, J, Sauter, L, Sauvage, F, Savini, G, Schmelzel, M, Schnorhk, A, Schwarz, W, Scott, D, Seiffert, M, Shellard, P, Shih, C, Sias, M, Silk, J, Silvestri, R, Sippel, R, Smoot, G, Starck, J, Stassi, P, Sternberg, J, Stivoli, F, Stolyarov, V, Stompor, R, Stringhetti, L, Strommen, D, Stute, T, Sudiwala, R, Sugimura, R, Sunyaev, R, Sygnet, J, Türler, M, Taddei, E, Tallon, J, Tamiatto, C, Taurigna, M, Taylor, D, Terenzi, L, Thuerey, S, Tillis, J, Tofani, G, Toffolatti, L, Tommasi, E, Tomasi, M, Tonazzini, E, Torre, J, Tosti, S, Touze, F, Tristram, M, Tuovinen, J, Tuttlebee, M, Umana, G, Valenziano, L, Vallée, D, VAN DER VLIS, M, VAN LEEUWEN, F, Vanel, J, VAN TENT, B, Varis, J, Vassallo, E, Vescovi, C, Vezzu, F, Vibert, D, Vielva, P, Vierra, J, Villa, F, Vittorio, N, Vuerli, C, Wade, L, Walker, A, Wandelt, B, Watson, C, Werner, D, White, M, White, S, Wilkinson, A, Wilson, P, Woodcraft, A, Yoffo, B, Yun, M, Yurchenko, V, Yvon, D, Zhang, B, Zimmermann, O, Zonca, A, Zorita, D, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Department of Physics, Helsinki Institute of Physics, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), École normale supérieure - Paris (ENS Paris), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), and Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics, general [Submillimeter], 7. Clean energy, 01 natural sciences, DESIGN, Aeronautics, CMB physics, SPACE, Space vehicles: instruments, Instrumentation: detectors, 010303 astronomy & astrophysics, detectors [Instrumentation], QB, CALIBRATION, Physics, Planck ESA mission, general [Radio continuum], Astrophysics::Instrumentation and Methods for Astrophysics, space vehicles: instrument, MICROWAVE BACKGROUND ANISOTROPY, instrumentation: polarimeter, HIGH-FREQUENCY INSTRUMENT, cosmic microwave background, Submillimeter: general, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Cosmic microwawe background, education, Astrophysics::Cosmology and Extragalactic Astrophysics, instrumentation: detector, Instrumentation: polarimeters, Cosmic microwave background, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], instruments [Space vehicles], Radio continuum: general, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, polarimeters [Instrumentation], 010308 nuclear & particles physics, Astronomy and Astrophysics, Space vehicles, PERFORMANCE, 115 Astronomy, Space science, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], space vehicles: instruments, instrumentation: detectors, instrumentation: polarimeters, submillimeter: general, radio continuum: general, CMB EXPERIMENTS, 13. Climate action, Space and Planetary Science, Astronautics, Aeronàutica i espai::Astronàutica [Àrees temàtiques de la UPC], Instruments, Astronàutica
Abstract: 22 páginas, 16 figuras, 6 tablas.-- Planck Science Team: et al., The European Space Agency's Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies of the CMB over the whole sky, with unprecedented sensitivity ( ~ 2 × 10-6) and angular resolution (~5 arcmin). Planck will provide a major source of information relevant to many fundamental cosmological problems and will test current theories of the early evolution of the Universe and the origin of structure. It will also address a wide range of areas of astrophysical research related to the Milky Way as well as external galaxies and clusters of galaxies. The ability of Planck to measure polarization across a wide frequency range (30-350 GHz), with high precision and accuracy, and over the whole sky, will provide unique insight, not only into specific cosmological questions, but also into the properties of the interstellar medium. This paper is part of a series which describes the technical capabilities of the Planck scientific payload. It is based on the knowledge gathered during the on-ground calibration campaigns of the major subsystems, principally its telescope and its two scientific instruments, and of tests at fully integrated satellite level. It represents the best estimate before launch of the technical performance that the satellite and its payload will achieve in flight. In this paper, we summarise the main elements of the payload performance, which is described in detail in the accompanying papers. In addition, we describe the satellite performance elements which are most relevant for science, and provide an overview of the plans for scientific operations and data analysis.
Published: 2010

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