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1. The large scale polarization explorer (LSPE) for CMB measurements: performance forecast

Author: The LSPE collaboration, Addamo, G., Ade, P. A. R., Baccigalupi, C., Baldini, A. M., Battaglia, P. M., Battistelli, E. S., Baù, A., de Bernardis, P., Bersanelli, M., Biasotti, M., Boscaleri, A., Caccianiga, B., Caprioli, S., Cavaliere, F., Cei, F., Cleary, K. A., Columbro, F., Coppi, G., Coppolecchia, A., Cuttaia, F., D'Alessandro, G., De Gasperis, G., De Petris, M., Fafone, V., Farsian, F., Barusso, L. Ferrari, Fontanelli, F., Franceschet, C., Gaier, T. C., Galli, L., Gatti, F., Genova-Santos, R., Gerbino, M., Gervasi, M., Ghigna, T., Grosso, D., Gruppuso, A., Gualtieri, R., Incardona, F., Jones, M. E., Kangaslahti, P., Krachmalnicoff, N., Lamagna, L., Lattanzi, M., López-Caraballo, C. H., Lumia, M., Mainini, R., Maino, D., Mandelli, S., Maris, M., Masi, S., Matarrese, S., May, A., Mele, L., Mena, P., Mennella, A., Molina, R., Molinari, D., Morgante, G., Natale, U., Nati, F., Natoli, P., Pagano, L., Paiella, A., Panico, F., Paonessa, F., Paradiso, S., Passerini, A., Perez-de-Taoro, M., Peverini, O. A., Piacentini, F., Piccirillo, L., Pisano, G., Poletti, D., Presta, G., Realini, S., Reyes, N., Rubino-Martin, J. A., Sandri, M., Sartor, S., Pezzotta, F., Polenta, G., Rocchi, A., Schillaci, A., Signorelli, G., Siri, B., Soria, M., Spinella, F., Tapia, V., Tartari, A., Taylor, A. C., Terenzi, L., Tomasi, M., Tommasi, E., Tucker, C., Vaccaro, D., Vigano, D. M., Villa, F., Virone, G., Vittorio, N., Volpe, A., Watkins, R. E. J., Zacchei, A., and Zannoni, M.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: [Abridged] The measurement of the polarization of the Cosmic Microwave Background radiation is one of the current frontiers in cosmology. In particular, the detection of the primordial B-modes, could reveal the presence of gravitational waves in the early Universe. The detection of such component is at the moment the most promising technique to probe the inflationary theory describing the very early evolution of the Universe. We present the updated performance forecast of the Large Scale Polarization Explorer (LSPE), a program dedicated to the measurement of the CMB polarization. LSPE is composed of two instruments: Strip, a radiometer-based telescope on the ground in Tenerife, and SWIPE (Short-Wavelength Instrument for the Polarization Explorer) a bolometer-based instrument designed to fly on a winter arctic stratospheric long-duration balloon. The program is among the few dedicated to observation of the Northern Hemisphere, while most of the international effort is focused into ground-based observation in the Southern Hemisphere. Measurements are currently scheduled in Winter 2021/22 for SWIPE, with a flight duration up to 15 days, and in Summer 2021 with two years observations for Strip. We describe the main features of the two instruments, identifying the most critical aspects of the design, in terms of impact into performance forecast. We estimate the expected sensitivity of each instrument and propagate their combined observing power to the sensitivity to cosmological parameters, including the effect of scanning strategy, component separation, residual foregrounds and partial sky coverage. We also set requirements on the control of the most critical systematic effects and describe techniques to mitigate their impact. LSPE can reach a sensitivity in tensor-to-scalar ratio of $\sigma_r<0.01$, and improve constrains on other cosmological parameters., Comment: Submitted to JCAP. Abstract abridged for arXiv submission
Published: 2020
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2. Progress report on the Large Scale Polarization Explorer

Author: Lamagna, L., Addamo, G., Ade, P. A. R., Baccigalupi, C., Baldini, A. M., Battaglia, P. M., Battistelli, E., Baù, A., Bersanelli, M., Biasotti, M., Boragno, C., Boscaleri, A., Caccianiga, B., Caprioli, S., Cavaliere, F., Cei, F., Cleary, K. A., Columbro, F., Coppi, G., Coppolecchia, A., Corsini, D., Cuttaia, F., D'Alessandro, G., de Bernardis, P., De Gasperis, G., De Petris, M., Del Torto, F., Fafone, V., Farooqui, Z., Farsian, F., Fontanelli, F., Franceschet, C., Gaier, T. C., Gatti, F., Genova-Santos, R., Gervasi, M., Ghigna, T., Grassi, M., Grosso, D., Gualtieri, R., Incardona, F., Jones, M., Kangaslahti, P., Krachmalnicoff, N., Mainini, R., Maino, D., Mandelli, S., Maris, M., Masi, S., Matarrese, S., May, A., Mena, P., Mennella, A., Molina, R., Molinari, D., Morgante, G., Nati, F., Natoli, P., Pagano, L., Paiella, A., Paonessa, F., Passerini, A., Perez-de-Taoro, M., Peverini, O. A., Pezzotta, F., Piacentini, F., Piccirillo, L., Pisano, G., Polastri, L., Polenta, G., Poletti, D., Presta, G., Realini, S., Reyes, N., Rocchi, A., Rubiño-Martin, J. A., Sandri, M., Sartor, S., Schillaci, A., Signorelli, G., Siri, B., Soria, M., Spinella, F., Tapia, V., Tartari, A., Taylor, A., Terenzi, L., Tomasi, M., Tommasi, E., Tucker, C., Vaccaro, D., Vigano, D. M., Villa, F., Virone, G., Vittorio, N., Volpe, A., Watkins, B., Zacchei, A., and Zannoni, M.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Large Scale Polarization Explorer (LSPE) is a cosmology program for the measurement of large scale curl-like features (B-modes) in the polarization of the Cosmic Microwave Background. Its goal is to constrain the background of inflationary gravity waves traveling through the universe at the time of matter-radiation decoupling. The two instruments of LSPE are meant to synergically operate by covering a large portion of the northern microwave sky. LSPE/STRIP is a coherent array of receivers planned to be operated from the Teide Observatory in Tenerife, for the control and characterization of the low-frequency polarized signals of galactic origin; LSPE/SWIPE is a balloon-borne bolometric polarimeter based on 330 large throughput multi-moded detectors, designed to measure the CMB polarization at 150 GHz and to monitor the polarized emission by galactic dust above 200 GHz. The combined performance and the expected level of systematics mitigation will allow LSPE to constrain primordial B-modes down to a tensor/scalar ratio of $10^{-2}$. We here report the status of the STRIP pre-commissioning phase and the progress in the characterization of the key subsystems of the SWIPE payload (namely the cryogenic polarization modulation unit and the multi-moded TES pixels) prior to receiver integration., Comment: 8 pages, 5 figures, Accepted for publication in Journal of Low Temperature Physics
Published: 2020
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3. The STRIP instrument of the Large Scale Polarization Explorer: microwave eyes to map the Galactic polarized foregrounds

Author: Franceschet, C., Realini, S., Mennella, A., Addamo, G., Baù, A., Battaglia, P. M., Bersanelli, M., Caccianiga, B., Caprioli, S., Cavaliere, F., Cleary, K. A., Cuttaia, F., Del Torto, F., Fafone, V., Farooqui, Z., Santos, R. T. Génova, Gaier, T. C., Gervasi, M., Ghigna, T., Incardona, F., Iovenitti, S., Jones, M., Kangaslahti, P., Mainini, R., Maino, D., Maris, M., Mena, P., Molina, R., Morgante, G., Passerini, A., Perez-de-Taoro, M., Peverini, O. A., Pezzotta, F., Pincella, C., Reyes, N., Rocchi, A., Rubiño-Martín, J. A., Sandri, M., Sartor, S., Soria, M., Tapia, V., Terenzi, L., Tomasi, M., Tommasi, E., Viganó, D. M., Villa, F., Virone, G., Volpe, A., Watkins, B., Zacchei, A., and Zannoni, M.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: In this paper we discuss the latest developments of the STRIP instrument of the "Large Scale Polarization Explorer" (LSPE) experiment. LSPE is a novel project that combines ground-based (STRIP) and balloon-borne (SWIPE) polarization measurements of the microwave sky on large angular scales to attempt a detection of the "B-modes" of the Cosmic Microwave Background polarization. STRIP will observe approximately 25% of the Northern sky from the "Observatorio del Teide" in Tenerife, using an array of forty-nine coherent polarimeters at 43 GHz, coupled to a 1.5 m fully rotating crossed-Dragone telescope. A second frequency channel with six-elements at 95 GHz will be exploited as an atmospheric monitor. At present, most of the hardware of the STRIP instrument has been developed and tested at sub-system level. System-level characterization, starting in July 2018, will lead STRIP to be shipped and installed at the observation site within the end of the year. The on-site verification and calibration of the whole instrument will prepare STRIP for a 2-years campaign for the observation of the CMB polarization., Comment: 17 pages, 15 figures, proceedings of the SPIE Astronomical Telescopes + Instrumentation conference "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX", on June 15th, 2018, Austin (TX)
Published: 2018
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4. Planck 2013 results. XVI. Cosmological parameters

Author: Planck Collaboration, Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cappellini, B., Cardoso, J. -F., Catalano, A., Challinor, A., Chamballu, A., Chary, R. -R., Chen, X., Chiang, H. C., Chiang, L. -Y, Christensen, P. R., Church, S., Clements, D. L., Colombi, S., Colombo, L. P. L., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Delouis, J. -M., Désert, F. -X., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Gaier, T. C., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Haissinski, J., Hamann, J., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hou, Z., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., León-Tavares, J., Lesgourgues, J., Lewis, A., Liguori, M., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maffei, B., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Melin, J. -B., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Oxborrow, C. A., Paci, F., Pagano, L., Pajot, F., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Pearson, T. J., Peiris, H. V., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rowan-Robinson, M., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Savini, G., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Wehus, I. K., White, M., White, S. D. M., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra. The Planck spectra at high multipoles are extremely well described by the standard spatially-flat six-parameter LCDM cosmology. In this model Planck data determine the cosmological parameters to high precision. We find a low value of the Hubble constant, H0=67.3+/-1.2 km/s/Mpc and a high value of the matter density parameter, Omega_m=0.315+/-0.017 (+/-1 sigma errors) in excellent agreement with constraints from baryon acoustic oscillation (BAO) surveys. Including curvature, we find that the Universe is consistent with spatial flatness to percent-level precision using Planck CMB data alone. We present results from an analysis of extensions to the standard cosmology, using astrophysical data sets in addition to Planck and high-resolution CMB data. None of these models are favoured significantly over standard LCDM. The deviation of the scalar spectral index from unity is insensitive to the addition of tensor modes and to changes in the matter content of the Universe. We find a 95% upper limit of r<0.11 on the tensor-to-scalar ratio. There is no evidence for additional neutrino-like relativistic particles. Using BAO and CMB data, we find N_eff=3.30+/-0.27 for the effective number of relativistic degrees of freedom, and an upper limit of 0.23 eV for the summed neutrino mass. Our results are in excellent agreement with big bang nucleosynthesis and the standard value of N_eff=3.046. We find no evidence for dynamical dark energy. Despite the success of the standard LCDM model, this cosmology does not provide a good fit to the CMB power spectrum at low multipoles, as noted previously by the WMAP team. While not of decisive significance, this is an anomaly in an otherwise self-consistent analysis of the Planck temperature data., Comment: 69 pages. Matches version to appear in Astronomy & Astrophysics
Published: 2013
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5. Planck 2013 results. XV. CMB power spectra and likelihood

Author: Planck collaboration, Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Battaner, E., Benabed, K., Benoit, A., Benoit-Levy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Catalano, A., Challinor, A., Chamballu, A., Chiang, L. -Y, Chiang, H. C., Christensen, P. R., Church, S., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Delouis, J. -M., Desert, F. -X., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Dore, O., Douspis, M., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Ensslin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Gaier, T. C., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giardino, G., Giraud-Heraud, Y., Gjerlow, E., Gonzalez-Nuevo, J., Gorski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Hansen, F. K., Hanson, D., 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., Huffenberger, K. M., Hurier, G., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Keihanen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lawrence, C. R., Jeune, M. Le, Leach, S., Leahy, J. P., Leonardi, R., Leon-Tavares, J., Lesgourgues, J., Liguori, M., Lilje, P. B., Lindholm, V., Linden-Vornle, M., Lopez-Caniego, M., Lubin, P. M., Macias-Perez, J. F., Maffei, B., Maino, D., Mandolesi, N., Marinucci, D., Maris, M., Marshall, D. J., Martin, P. G., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschenes, M. -A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Nati, F., Natoli, P., Netterfield, C. B., Norgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I. J., Orieux, F., Osborne, S., Oxborrow, C. A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Paykari, P., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prezeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rahlin, A., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Riller, T., Ringeval, C., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rowan-Robinson, M., Rubino-Martin, J. A., Rusholme, B., Sandri, M., Sanselme, L., Santos, D., Savini, G., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sudiwala, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Turler, M., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Wehus, I. K., White, M., White, S. D. M., Yvon, D., Zacchei, A., and Zonca, A.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the Planck likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations. We use this likelihood to derive the Planck CMB power spectrum over three decades in l, covering 2 <= l <= 2500. The main source of error at l <= 1500 is cosmic variance. Uncertainties in small-scale foreground modelling and instrumental noise dominate the error budget at higher l's. For l < 50, our likelihood exploits all Planck frequency channels from 30 to 353 GHz through a physically motivated Bayesian component separation technique. At l >= 50, we employ a correlated Gaussian likelihood approximation based on angular cross-spectra derived from the 100, 143 and 217 GHz channels. We validate our likelihood through an extensive suite of consistency tests, and assess the impact of residual foreground and instrumental uncertainties on cosmological parameters. We find good internal agreement among the high-l cross-spectra with residuals of a few uK^2 at l <= 1000. We compare our results with foreground-cleaned CMB maps, and with cross-spectra derived from the 70 GHz Planck map, and find broad agreement in terms of spectrum residuals and cosmological parameters. The best-fit LCDM cosmology is in excellent agreement with preliminary Planck polarisation spectra. The standard LCDM cosmology is well constrained by Planck by l <= 1500. For example, we report a 5.4 sigma deviation from n_s /= 1. Considering various extensions beyond the standard model, we find no indication of significant departures from the LCDM framework. Finally, we report a tension between the best-fit LCDM model and the low-l spectrum in the form of a power deficit of 5-10% at l <~ 40, significant at 2.5-3 sigma. We do not elaborate further on its cosmological implications, but note that this is our most puzzling finding in an otherwise remarkably consistent dataset. (Abridged), Comment: This paper is one of a set associated with the 2013 release of data from the Planck mission. 62 pages, 64 figures, 12 tables
Published: 2013
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6. Planck 2013 results. I. Overview of products and scientific results

Author: Planck Collaboration, Ade, P. A. R., Aghanim, N., Alves, M. I. R., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Aussel, H., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Barrena, R., Bartelmann, M., Bartlett, J. G., Bartolo, N., Basak, S., Battaner, E., Battye, R., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bertincourt, B., Bethermin, M., Bielewicz, P., Bikmaev, I., Blanchard, A., Bobin, J., Bock, J. J., Böhringer, H., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bourdin, H., Bowyer, J. W., Bridges, M., Brown, M. L., Bucher, M., Burenin, R., Burigana, C., Butler, R. C., Calabrese, E., Cappellini, B., Cardoso, J. -F., Carr, R., Carvalho, P., Casale, M., Castex, G., Catalano, A., Challinor, A., Chamballu, A., Chary, R. -R., Chen, X., Chiang, H. C., Chiang, L. -Y, Chon, G., Christensen, P. R., Churazov, E., Church, S., Clemens, M., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Comis, B., Couchot, F., Coulais, A., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Da Silva, A., Dahle, H., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Déchelette, T., Delabrouille, J., Delouis, J. -M., Démoclès, J., Désert, F. -X., Dick, J., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Fabre, O., Falgarone, E., Falvella, M. C., Fantaye, Y., Fergusson, J., Filliard, C., Finelli, F., Flores-Cacho, I., Foley, S., Forni, O., Fosalba, P., Frailis, M., Fraisse, A. A., Franceschi, E., Freschi, M., Fromenteau, S., Frommert, M., Gaier, T. C., Galeotta, S., Gallegos, J., Galli, S., Gandolfo, B., Ganga, K., Gauthier, C., Génova-Santos, R. T., Ghosh, T., Giard, M., Giardino, G., Gilfanov, M., Girard, D., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Haissinski, J., Hamann, J., Hansen, F. K., Hansen, M., Hanson, D., Harrison, D. L., Heavens, A., Helou, G., Hempel, A., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Ho, S., Hobson, M., Holmes, W. A., Hornstrup, A., Hou, Z., Hovest, W., Huey, G., Huffenberger, K. M., Hurier, G., Ilić, S., Jaffe, A. H., Jaffe, T. R., Jasche, J., Jewell, J., Jones, W. C., Juvela, M., Kalberla, P., Kangaslahti, P., Keihänen, E., Kerp, J., Keskitalo, R., Khamitov, I., Kiiveri, K., Kim, J., Kisner, T. S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lacasa, F., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Langer, M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lavabre, A., Lawrence, C. R., Jeune, M. Le, Leach, S., Leahy, J. P., Leonardi, R., León-Tavares, J., Leroy, C., Lesgourgues, J., Lewis, A., Li, C., Liddle, A., Liguori, M., Lilje, P. B., Linden-Vørnle, M., Lindholm, V., López-Caniego, M., Lowe, S., Lubin, P. M., Macías-Pérez, J. F., MacTavish, C. J., Maffei, B., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marcos-Caballero, A., Marinucci, D., Maris, M., Marleau, F., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Matsumura, T., Matthai, F., Maurin, L., Mazzotta, P., McDonald, A., McEwen, J. D., McGehee, P., Mei, S., Meinhold, P. R., Melchiorri, A., Melin, J. -B., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Mikkelsen, K., Millea, M., Miniscalco, R., Mitra, S., Miville-Deschênes, M. -A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Morisset, N., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Negrello, M., Nesvadba, N. P. H., Netterfield, C. B., Nørgaard-Nielsen, H. U., North, C., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I. J., Orieux, F., Osborne, S., O'Sullivan, C., Oxborrow, C. A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Pandolfi, S., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Paykari, P., Pearson, D., Pearson, T. J., Peel, M., Peiris, H. V., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pogosyan, D., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Pullen, A. R., Rachen, J. P., Racine, B., Rahlin, A., Räth, C., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Riazuelo, A., Ricciardi, S., Riller, T., Ringeval, C., Ristorcelli, I., Robbers, G., Rocha, G., Roman, M., Rosset, C., Rossetti, M., Roudier, G., Rowan-Robinson, M., Rubiño-Martín, J. A., Ruiz-Granados, B., Rusholme, B., Salerno, E., Sandri, M., Sanselme, L., Santos, D., Savelainen, M., Savini, G., Schaefer, B. M., Schiavon, F., Scott, D., Seiffert, M. D., Serra, P., Shellard, E. P. S., Smith, K., Smoot, G. F., Souradeep, T., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sureau, F., Sutter, P., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Taylor, D., Terenzi, L., Texier, D., Toffolatti, L., Tomasi, M., Torre, J. -P., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Tuttlebee, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vibert, L., Viel, M., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, C., Watson, R., Wehus, I. K., Welikala, N., Weller, J., White, M., White, S. D. M., Wilkinson, A., Winkel, B., Xia, J. -Q., Yvon, D., Zacchei, A., Zibin, J. P., and Zonca, A.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The ESA's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. This paper gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the CMB and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the SZ effect. The likelihood code used to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter LCDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25 sigma. Planck finds no evidence for non-Gaussianity in the CMB. Planck's results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluctuations derived from CMB data and that derived from SZ data. The Planck and WMAP power spectra are offset from each other by an average level of about 2% around the first acoustic peak.
Published: 2013
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7. Planck 2013 results. IV. Low Frequency Instrument beams and window functions

Author: Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, L. -Y, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud-Héraud, Y., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden-Vørnle, M., Lindholm, V., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Zacchei, A., and Zonca, A.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: This paper presents the characterization of the in-flight beams, the beam window functions and the associated uncertainties for the Planck Low Frequency Instrument (LFI). Knowledge of the beam profiles is necessary for determining the transfer function to go from the observed to the actual sky anisotropy power spectrum. The main beam distortions affect the beam window function, complicating the reconstruction of the anisotropy power spectrum at high multipoles, whereas the sidelobes affect the low and intermediate multipoles. The in-flight assessment of the LFI main beams relies on the measurements performed during Jupiter observations. By stacking the data from multiple Jupiter transits, the main beam profiles are measured down to -20 dB at 30 and 44 GHz, and down to -25 dB at 70 GHz. The main beam solid angles are determined to better than 0.2% at each LFI frequency band. The Planck pre-launch optical model is conveniently tuned to characterize the main beams independently of any noise effects. This approach provides an optical model whose beams fully reproduce the measurements in the main beam region, but also allows a description of the beams at power levels lower than can be achieved by the Jupiter measurements themselves. The agreement between the simulated beams and the measured beams is better than 1% at each LFI frequency band. The simulated beams are used for the computation of the window functions for the effective beams. The error budget for the window functions is estimated from both main beam and sidelobe contributions, and accounts for the radiometer bandshapes. The total uncertainties in the effective beam window functions are: 2% and 1.2% at 30 and 44 GHz, respectively (at $\ell \approx 600$), and 0.7% at 70 GHz (at $\ell \approx 1000$).
Published: 2013
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8. Planck 2013 results. III. LFI systematic uncertainties

Author: Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, L. -Y, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dick, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Lindholm, V., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. We also present an overall budget of known systematic effect uncertainties, which are dominated sidelobe straylight pick-up and imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave background (CMB) fluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipole range $\ell<20$, most notably at 30 GHz, and is likely caused by residual Galactic straylight contamination. Current analysis aims to further reduce the level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibration uncertainties., Comment: Accepted for publication by A&A
Published: 2013
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9. Planck 2013 results. II. Low Frequency Instrument data processing

Author: Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cappellini, B., Cardoso, J. -F., Catalano, A., Chamballu, A., Chen, X., Chiang, L. -Y, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden-Vørnle, M., Lindholm, V., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Morisset, N., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Robbers, G., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Salerno, E., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wehus, I. K., White, S. D. M., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5 months of operations at 30, 44 and 70 GHz. In particular, we discuss the various steps involved in reducing the data, starting from telemetry packets through to the production of cleaned, calibrated timelines and calibrated frequency maps. Data are continuously calibrated using the modulation induced on the mean temperature of the cosmic microwave background radiation by the proper motion of the spacecraft. Sky signals other than the dipole are removed by an iterative procedure based on simultaneous fitting of calibration parameters and sky maps. Noise properties are estimated from time-ordered data after the sky signal has been removed, using a generalized least square map-making algorithm. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices, required to compute statistical uncertainties on LFI and Planck products, are also produced. Main beams are estimated down to the -20 dB level using Jupiter transits, which are also used for the geometrical calibration of the focal plane.
Published: 2013
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10. Planck 2013 results. V. LFI calibration

Author: Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cappellini, B., Cardoso, J. -F., Catalano, A., Chamballu, A., Chen, X., Chiang, L. -Y, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the Orbital Dipole plus the Solar Dipole, caused respectively by the motion of the Planck spacecraft with respect to the Sun and by motion of the Solar System with respect to the CMB rest frame. The latter provides a signal of a few mK with the same spectrum as the CMB anisotropies and is visible throughout the mission. In this data release we rely on the characterization of the Solar Dipole as measured by WMAP. We also present preliminary results (at 44GHz only) on the study of the Orbital Dipole, which agree with the WMAP value of the Solar System speed within our uncertainties. We compute the calibration constant for each radiometer roughly once per hour, in order to keep track of changes in the detectors' gain. Since non-idealities in the optical response of the beams proved to be important, we implemented a fast convolution algorithm which considers the full beam response in estimating the signal generated by the dipole. Moreover, in order to further reduce the impact of residual systematics due to sidelobes, we estimated time variations in the calibration constant of the 30GHz radiometers (the ones with the largest sidelobes) using the signal of a reference load. We have estimated the calibration accuracy in two ways: we have run a set of simulations to assess the impact of statistical errors and systematic effects in the instrument and in the calibration procedure, and we have performed a number of consistency checks on the data and on the brightness temperature of Jupiter. Calibration errors for this data release are expected to be about 0.6% at 44 and 70 GHz, and 0.8% at 30 GHz. (Abriged.), Comment: 29 pages, 23 figures, 12 tables, 1 appendix - New version submitted to A&A
Published: 2013
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11. Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance

Author: Mennella, A., Bersanelli, M., Butler, R. C., Curto, A., Cuttaia, F., Davis, R. J., Dick, J., Frailis, M., Galeotta, S., Gregorio, A., Kurki-Suonio, H., Lawrence, C. R., Leach, S., Leahy, J. P., Lowe, S., Maino, D., Mandolesi, N., Maris, M., Martínez-González, E., Meinhold, P. R., Morgante, G., Pearson, D., Perrotta, F., Polenta, G., Poutanen, T., Sandri, M., Seiffert, M. D., Suur-Uski, A. -S., Tavagnacco, D., Terenzi, L., Tomasi, M., Valiviita, J., Villa, F., Watson, R., Wilkinson, A., Zacchei, A., Zonca, A., Aja, B., Artal, E., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., Battaglia, P., Bennett, K., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F. R., Burigana, C., Cabella, P., Cappellini, B., Chen, X., Colombo, L., Cruz, M., Danese, L., D'Arcangelo, O., Davies, R. D., de Gasperis, G., de Rosa, A., de Zotti, G., Dickinson, C., Diego, J. M., Donzelli, S., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Foley, S., Franceschet, C., Franceschi, E., Gaier, T. C., Génova-Santos, R. T., George, D., Gómez, F., González-Nuevo, J., Górski, K. M., Gruppuso, A., Hansen, F. K., Herranz, D., Herreros, J. M., Hoyland, R. J., Hughes, N., Jewell, J., Jukkala, P., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kilpia, V. -H., Kisner, T. S., Knoche, J., Knox, L., Laaninen, M., Lähteenmäki, A., Lamarre, J. -M., Leonardi, R., León-Tavares, J., Leutenegger, P., Lilje, P. B., López-Caniego, M., Lubin, P. M., Malaspina, M., Marinucci, D., Massardi, M., Matarrese, S., Matthai, F., Melchiorri, A., Mendes, L., Miccolis, M., Migliaccio, M., Mitra, S., Moss, A., Natoli, P., Nesti, R., Nørgaard-Nielsen, H. U., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Pettorino, V., Pietrobon, D., Pospieszalski, M., Prézeau, G., Prina, M., Procopio, P., Puget, J. -L., Quercellini, C., Rachen, J. P., Rebolo, R., Reinecke, M., Ricciardi, S., Robbers, G., Rocha, G., Roddis, N., Rubiño-Martín, J. A., Savelainen, M., Scott, D., Silvestri, R., Simonetto, A., Sjoman, P., Smoot, G. F., Sozzi, C., Stringhetti, L., Tauber, J. A., Tofani, G., Toffolatti, L., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Varis, J., Vielva, P., Vittorio, N., Wade, L. A., Watson, C., White, S. D. M., and Winder, F.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit operation is presented. We describe the main optical parameters and discuss photometric calibration, white noise sensitivity, and noise properties. A preliminary evaluation of the impact of the main systematic effects is presented. For each of the performance parameters, we outline the methods used to obtain them from the flight data and provide a comparison with pre-launch ground assessments, which are essentially confirmed in flight., Comment: Published version
Published: 2011
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12. Planck Early Results. V. The Low Frequency Instrument data processing

Author: Zacchei, A., Maino, D., Baccigalupi, C., Bersanelli, M., Bonaldi, A., Bonavera, L., Burigana, C., Butler, R. C., Cuttaia, F., de Zotti, G., Dick, J., Frailis, M., Galeotta, S., González-Nuevo, J., Górski, K. M., Gregorio, A., Keihänen, E., Keskitalo, R., Knoche, J., Kurki-Suonio, H., Lawrence, C. R., Leach, S., Leahy, J. P., López-Caniego, M., Mandolesi, N., Maris, M., Matthai, F., Meinhold, P. R., Mennella, A., Morgante, G., Morisset, N., Natoli, P., Pasian, F., Perrotta, F., Polenta, G., Poutanen, T., Reinecke, M., Ricciardi, S., Rohlfs, R., Sandri, M., Suur-Uski, A. -S., Tauber, J. A., Tavagnacco, D., Terenzi, L., Tomasi, M., Valiviita, J., Villa, F., Zonca, A., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., Bedini, L., Bennett, K., Binko, P., Borrill, J., Bouchet, F. R., Bremer, M., Cabella, P., Cappellini, B., Chen, X., Colombo, L., Cruz, M., Curto, A., Danese, L., Davies, R. D., Davis, R. J., de Gasperis, G., de Rosa, A., de Troia, G., Dickinson, C., Diego, J. M., Donzelli, S., Dörl, U., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Franceschi, E., Gaier, T. C., Gasparo, F., Génova-Santos, R. T., Giardino, G., Gómez, F., Gruppuso, A., Hansen, F. K., Hell, R., Herranz, D., Hovest, W., Huynh, M., Jewell, J., Juvela, M., Kisner, T. S., Knox, L., Lähteenmäki, A., Lamarre, J. -M., Leonardi, R., León-Tavares, J., Lilje, P. B., Lubin, P. M., Maggio, G., Marinucci, D., Martínez-González, E., Massardi, M., Matarrese, S., Meharga, M. T., Melchiorri, A., Migliaccio, M., Mitra, S., Moss, A., Nørgaard-Nielsen, H. U., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pearson, D., Pettorino, V., Pietrobon, D., Prézeau, G., Procopio, P., Puget, J. -L., Quercellini, C., Rachen, J. P., Rebolo, R., Robbers, G., Rocha, G., Rubiño-Martín, J. A., Salerno, E., Savelainen, M., Scott, D., Seiffert, M. D., Silk, J. I., Smoot, G. F., Sternberg, J., Stivoli, F., Stompor, R., Tofani, G., Toffolatti, L., Tuovinen, J., Türler, M., Umana, G., Vielva, P., Vittorio, N., Vuerli, C., Wade, L. A., Watson, R., White, S. D. M., and Wilkinson, A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discuss the steps involved in reducing the data from telemetry packets to cleaned, calibrated, time-ordered data (TOD) and frequency maps. Data are continuously calibrated using the modulation of the temperature of the cosmic microwave background radiation induced by the motion of the spacecraft. Noise properties are estimated from TOD from which the sky signal has been removed using a generalized least square map-making algorithm. Measured 1/f noise knee-frequencies range from 100mHz at 30GHz to a few tens of mHz at 70GHz. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices required to compute statistical uncertainties on LFI and Planck products are also produced. Main beams are estimated down to the approx -10dB level using Jupiter transits, which are also used for geometrical calibration of the focal plane., Comment: A&A Volume 536, December 2011 Planck early results
Published: 2011
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13. 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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14. Progress Report on the Large-Scale Polarization Explorer

Author: Lamagna, L, Addamo, G, Ade, P, Baccigalupi, C, Baldini, A, Battaglia, P, Battistelli, E, Baù, A, Bersanelli, M, Biasotti, M, Boragno, C, Boscaleri, A, Caccianiga, B, Caprioli, S, Cavaliere, F, Cei, F, Cleary, K, Columbro, F, Coppi, G, Coppolecchia, A, Corsini, D, Cuttaia, F, D’Alessandro, G, de Bernardis, P, De Gasperis, G, De Petris, M, Torto, F, Fafone, V, Farooqui, Z, Farsian, F, Fontanelli, F, Franceschet, C, Gaier, T, Gatti, F, Genova-Santos, R, Gervasi, M, Ghigna, T, Grassi, M, Grosso, D, Incardona, F, Jones, M, Kangaslahti, P, Krachmalnicoff, N, Mainini, R, Maino, D, Mandelli, S, Maris, M, Masi, S, Matarrese, S, May, A, Mena, P, Mennella, A, Molina, R, Molinari, D, Morgante, G, Nati, F, Natoli, P, Pagano, L, Paiella, A, Paonessa, F, Passerini, A, Perez-de-Taoro, M, Peverini, O, Pezzotta, F, Piacentini, F, Piccirillo, L, Pisano, G, Polastri, L, Polenta, G, Poletti, D, Presta, G, Realini, S, Reyes, N, Rocchi, A, Rubino-Martin, J, Sandri, M, Sartor, S, Schillaci, A, Signorelli, G, Soria, M, Spinella, F, Tapia, V, Tartari, A, Taylor, A, Terenzi, L, Tomasi, M, Tommasi, E, Tucker, C, Vaccaro, D, Vigano, D, Villa, F, Virone, G, Vittorio, N, Volpe, A, Watkins, B, Zacchei, A, Zannoni, M, Lamagna, L., Addamo, G., Ade, P. A. R., Baccigalupi, C., Baldini, A. M., Battaglia, P. M., Battistelli, E., Baù, A., Bersanelli, M., Biasotti, M., Boragno, C., Boscaleri, A., Caccianiga, B., Caprioli, S., Cavaliere, F., Cei, F., Cleary, K. A., Columbro, F., Coppi, G., Coppolecchia, A., Corsini, D., Cuttaia, F., D’Alessandro, G., de Bernardis, P., De Gasperis, G., De Petris, M., Torto, F. Del, Fafone, V., Farooqui, Z., Farsian, F., Fontanelli, F., Franceschet, C., Gaier, T. C., Gatti, F., Genova-Santos, R., Gervasi, M., Ghigna, T., Grassi, M., Grosso, D., Incardona, F., Jones, M., Kangaslahti, P., Krachmalnicoff, N., Mainini, R., Maino, D., Mandelli, S., Maris, M., Masi, S., Matarrese, S., May, A., Mena, P., Mennella, A., Molina, R., Molinari, D., Morgante, G., Nati, F., Natoli, P., Pagano, L., Paiella, A., Paonessa, F., Passerini, A., Perez-de-Taoro, M., Peverini, O. A., Pezzotta, F., Piacentini, F., Piccirillo, L., Pisano, G., Polastri, L., Polenta, G., Poletti, D., Presta, G., Realini, S., Reyes, N., Rocchi, A., Rubino-Martin, J. A., Sandri, M., Sartor, S., Schillaci, A., Signorelli, G., Soria, M., Spinella, F., Tapia, V., Tartari, A., Taylor, A., Terenzi, L., Tomasi, M., Tommasi, E., Tucker, C., Vaccaro, D., Vigano, D. M., Villa, F., Virone, G., Vittorio, N., Volpe, A., Watkins, B., Zacchei, A., Zannoni, M., Lamagna, L, Addamo, G, Ade, P, Baccigalupi, C, Baldini, A, Battaglia, P, Battistelli, E, Baù, A, Bersanelli, M, Biasotti, M, Boragno, C, Boscaleri, A, Caccianiga, B, Caprioli, S, Cavaliere, F, Cei, F, Cleary, K, Columbro, F, Coppi, G, Coppolecchia, A, Corsini, D, Cuttaia, F, D’Alessandro, G, de Bernardis, P, De Gasperis, G, De Petris, M, Torto, F, Fafone, V, Farooqui, Z, Farsian, F, Fontanelli, F, Franceschet, C, Gaier, T, Gatti, F, Genova-Santos, R, Gervasi, M, Ghigna, T, Grassi, M, Grosso, D, Incardona, F, Jones, M, Kangaslahti, P, Krachmalnicoff, N, Mainini, R, Maino, D, Mandelli, S, Maris, M, Masi, S, Matarrese, S, May, A, Mena, P, Mennella, A, Molina, R, Molinari, D, Morgante, G, Nati, F, Natoli, P, Pagano, L, Paiella, A, Paonessa, F, Passerini, A, Perez-de-Taoro, M, Peverini, O, Pezzotta, F, Piacentini, F, Piccirillo, L, Pisano, G, Polastri, L, Polenta, G, Poletti, D, Presta, G, Realini, S, Reyes, N, Rocchi, A, Rubino-Martin, J, Sandri, M, Sartor, S, Schillaci, A, Signorelli, G, Soria, M, Spinella, F, Tapia, V, Tartari, A, Taylor, A, Terenzi, L, Tomasi, M, Tommasi, E, Tucker, C, Vaccaro, D, Vigano, D, Villa, F, Virone, G, Vittorio, N, Volpe, A, Watkins, B, Zacchei, A, Zannoni, M, Lamagna, L., Addamo, G., Ade, P. A. R., Baccigalupi, C., Baldini, A. M., Battaglia, P. M., Battistelli, E., Baù, A., Bersanelli, M., Biasotti, M., Boragno, C., Boscaleri, A., Caccianiga, B., Caprioli, S., Cavaliere, F., Cei, F., Cleary, K. A., Columbro, F., Coppi, G., Coppolecchia, A., Corsini, D., Cuttaia, F., D’Alessandro, G., de Bernardis, P., De Gasperis, G., De Petris, M., Torto, F. Del, Fafone, V., Farooqui, Z., Farsian, F., Fontanelli, F., Franceschet, C., Gaier, T. C., Gatti, F., Genova-Santos, R., Gervasi, M., Ghigna, T., Grassi, M., Grosso, D., Incardona, F., Jones, M., Kangaslahti, P., Krachmalnicoff, N., Mainini, R., Maino, D., Mandelli, S., Maris, M., Masi, S., Matarrese, S., May, A., Mena, P., Mennella, A., Molina, R., Molinari, D., Morgante, G., Nati, F., Natoli, P., Pagano, L., Paiella, A., Paonessa, F., Passerini, A., Perez-de-Taoro, M., Peverini, O. A., Pezzotta, F., Piacentini, F., Piccirillo, L., Pisano, G., Polastri, L., Polenta, G., Poletti, D., Presta, G., Realini, S., Reyes, N., Rocchi, A., Rubino-Martin, J. A., Sandri, M., Sartor, S., Schillaci, A., Signorelli, G., Soria, M., Spinella, F., Tapia, V., Tartari, A., Taylor, A., Terenzi, L., Tomasi, M., Tommasi, E., Tucker, C., Vaccaro, D., Vigano, D. M., Villa, F., Virone, G., Vittorio, N., Volpe, A., Watkins, B., Zacchei, A., and Zannoni, M.
Abstract: The large-scale polarization explorer (LSPE) is a cosmology program for the measurement of large-scale curl-like features (B-modes) in the polarization of the cosmic microwave background. Its goal is to constrain the background of inflationary gravity waves traveling through the universe at the time of matter-radiation decoupling. The two instruments of LSPE are meant to synergically operate by covering a large portion of the northern microwave sky. LSPE/STRIP is a coherent array of receivers planned to be operated from the Teide Observatory in Tenerife, for the control and characterization of the low-frequency polarized signals of galactic origin; LSPE/SWIPE is a balloon-borne bolometric polarimeter based on 330 large throughput multi-moded detectors, designed to measure the CMB polarization at 150 GHz and to monitor the polarized emission by galactic dust above 200 GHz. The combined performance and the expected level of systematics mitigation will allow LSPE to constrain primordial B-modes down to a tensor/scalar ratio of 10^−2. We here report the status of the STRIP pre-commissioning phase and the progress in the characterization of the key subsystems of the SWIPE payload (namely the cryogenic polarization modulation unit and the multi-moded TES pixels) prior to receiver integration.
Published: 2020

15. Progress Report on the Large-Scale Polarization Explorer

Author: Lamagna, L., primary, Addamo, G., additional, Ade, P. A. R., additional, Baccigalupi, C., additional, Baldini, A. M., additional, Battaglia, P. M., additional, Battistelli, E., additional, Baù, A., additional, Bersanelli, M., additional, Biasotti, M., additional, Boragno, C., additional, Boscaleri, A., additional, Caccianiga, B., additional, Caprioli, S., additional, Cavaliere, F., additional, Cei, F., additional, Cleary, K. A., additional, Columbro, F., additional, Coppi, G., additional, Coppolecchia, A., additional, Corsini, D., additional, Cuttaia, F., additional, D’Alessandro, G., additional, de Bernardis, P., additional, De Gasperis, G., additional, De Petris, M., additional, Torto, F. Del, additional, Fafone, V., additional, Farooqui, Z., additional, Farsian, F., additional, Fontanelli, F., additional, Franceschet, C., additional, Gaier, T. C., additional, Gatti, F., additional, Genova-Santos, R., additional, Gervasi, M., additional, Ghigna, T., additional, Grassi, M., additional, Grosso, D., additional, Incardona, F., additional, Jones, M., additional, Kangaslahti, P., additional, Krachmalnicoff, N., additional, Mainini, R., additional, Maino, D., additional, Mandelli, S., additional, Maris, M., additional, Masi, S., additional, Matarrese, S., additional, May, A., additional, Mena, P., additional, Mennella, A., additional, Molina, R., additional, Molinari, D., additional, Morgante, G., additional, Nati, F., additional, Natoli, P., additional, Pagano, L., additional, Paiella, A., additional, Paonessa, F., additional, Passerini, A., additional, Perez-de-Taoro, M., additional, Peverini, O. A., additional, Pezzotta, F., additional, Piacentini, F., additional, Piccirillo, L., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Poletti, D., additional, Presta, G., additional, Realini, S., additional, Reyes, N., additional, Rocchi, A., additional, Rubino-Martin, J. A., additional, Sandri, M., additional, Sartor, S., additional, Schillaci, A., additional, Signorelli, G., additional, Soria, M., additional, Spinella, F., additional, Tapia, V., additional, Tartari, A., additional, Taylor, A., additional, Terenzi, L., additional, Tomasi, M., additional, Tommasi, E., additional, Tucker, C., additional, Vaccaro, D., additional, Vigano, D. M., additional, Villa, F., additional, Virone, G., additional, Vittorio, N., additional, Volpe, A., additional, Watkins, B., additional, Zacchei, A., additional, and Zannoni, M., additional
Published: 2020
Full Text: View/download PDF

16. Geo-STAR : a geostationary microwave sounder for the future.

Author: Lambrigtsen, Bjorn H, Brown, S. T, Dinardo, S. J, Gaier, T. C, Kangaslahti, P. P, and Tanner, A. B
Published: 2007

17. Initial results of the Geosynchronous Synthetic Thinned Array Radiometer (GeoSTAR)

Author: Tanner, Alan B, Wilson, W. J, Lambrigsten, B. H, Dinardo, S. J, Brown, S. T, Kangaslahti, P, Gaier, T. C, Ruf, C. S, Gross, S. M, Lim, B. H, Musko, S, and Rogacki, S
Published: 2006

18. THz Instrumentation for the Herschel Space Observatory's Heterodyne Instrument for Far Infrared

Author: Pearson, J. C, Mehdi, I, Ward, J. S, Maiwald, F, Ferber, R. R, Leduc, H. G, Schlecht, E. T, Gill, J. J, Hatch, W. A, Kawamura, J. H, Stern, J. A, Gaier, T. C, Samoska, L. A, Weinreb, S, Bumble, B, Pukala, D. M, Javadi, H. H, Finamore, B. P, Lin, R. H, Dengler, R. J, Velebir, J. R, Luong, E. M, Tsang, R, Peralta, A, and Wells, M
Subjects: Spacecraft Instrumentation And Astrionics
Abstract: The Heterodyne Instrument for Far Infrared (HIFI) on ESA's Herschel Space Observatory utilizes a variety of novel RF components in its five SIS receiver channels covering 480-1250 GHz and two HEB receiver channels covering 1410-1910 GHz. The local oscillator unit will be passively cooled while the focal plane unit is cooled by superfluid helium and cold helium vapors. HIFI employs W-band GaAs amplifiers, InP HEMT low noise IF amplifiers, fixed tuned broadband planar diode multipliers, high power W-bapd Isolators, and novel material systems in the SIS mixers. The National Aeronautics and Space Administration through the Jet Propulsion Laboratory is managing the development of the highest frequency (1119-1250 GHz) SIS mixers, the local oscillators oscillators for the three highest frequency receivers as well as W-band power amplifiers, high power W-band isolators, varactor diode devices for all high frequency multipliers and InP HEMT components for all the receiver channels intermediate frequency amplifiers. The NASA developed components represent a significant advancement in the available performance. This paper presents an update of the performance and the current state of development.
Published: 2004

19. Cryogenic W band power-combined amplifier designs for applications in the range of 71 to 106 GHz

Author: Ferber, R. R, Pearson, J. C, Gaier, T. C, Samoska, L. A, Swift, G, Yocom, P, and Liao, K. T
Published: 2003

20. W band MMIC power amplifier development for the Herschel HIFI Instrument

Author: Ferber, R. R, Pearson, J. C, Gaier, T. C, Samoska, L. A, Swift, G, Yocom, P, and Liao, K. T
Published: 2003

21. W band MMIC power amplifiers for the Herschel HIFI instrument

Author: Ferber, R. R, Gaier, T. C, Pearson, J. C, Samoska, L. A, Wells, M, and Campbell, A
Subjects: Electronics And Electrical Engineering
Abstract: This paper summarizes the development of W band amplifiers for the Local Oscillator (LO) chains for the Herschel HIFI (Heterodyne Instrument for Far Infrared) Instrument.
Published: 2003

22. W band power amplifier development for the Herschel HIFI instrument

Author: Ferber, R. R, Gaier, T. C, Pearson, J. C, Samoska, L. A, Wells, M, Swift, G, Yocom, P, and Chung, Y
Subjects: Instrumentation And Photography
Abstract: This paper summarizes the development of W Band amplifiers for the Local Oscilator chains for the Herschel HIFI Instrument.
Published: 2002

23. Coherent radiometers for cosmic microwve background polarization detection

Author: Gaier, T. C
Published: 2002

24. Degree-scale anisotropy in the cosmic microwave background: SP94 results

Author: Gundersen, J. O, Lim, M, Staren, J, Wuensche, C. A, Figueiredo, N, Gaier, T. C, Koch, T, Meinhold, P. R, Seiffert, M. D, and Cook, G
Subjects: Astrophysics
Abstract: We present results from two observations of the cosmic microwave background (CMB) performed from the South Pole during the 1993-1994 austral summer. Each observation employed a 3 deg peak-to-peak sinusoidal, single-difference chop and consisted of a 20 deg x 1 deg strip on the sky. The first observation used a receiver which operates in three channels between 38 and 45 GHz (Q-band) with a full width half maximum (FWHM) beam which varies from 1 deg to 1.15 deg. The second observation overlapped the first observation and used a receiver which operates in four channels between 26 and 36 GHz (Ka-band) with a FWHM beam which varies from 1.5 deg to 1.7 deg. Significant correlated structure is observed in all channels for each observation. The spectrum of the structure is consistent with a CMB spectrum and is formally inconsistent with diffuse synchrotron and free-free emission at the 5 sigma level. The amplitude of the structure is inconsistent with 20 K interstellar dust; however, the data do not discriminate against flat or inverted spectrum point sources. The root mean square amplitude (+/- 1 sigma) of the combined (Ka + Q) data is Delta T(sub rms) = 41.2(sup +15.5, sub -6.7) micro-K for an average window function which has a peak value of 0.97 at l = 68 and drops to e(exp -0.5) of the peak value at l = 36 and l = 106. A band power estimate of the CMB power spectrum, C(sub l), gives average value of (C(sub l)l(l + 1)/(2 pi))(sub B) = 1.77(sup +1.58, sub -0.54) x 10(exp -10).
Published: 1995
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25. Planck 2013 results

Author: Tauber, Jan, Aghanim, N., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cardoso, J. F., Catalano, A., Chamballu, A., Chiang, L. Y., Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Dick, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud Héraud, Y., Gjerløw, E., González Nuevo, J., Górski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot Versillé, S., Hernández Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden Vørnle, M., Lindholm, V., López Caniego, M., Lubin, P. M., Maciás Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubinõ Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur Uski, A. S., Sygnet, J. F., Tauber, J. A., Tavagnacco, Daniele, Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Universidad de Cantabria, Tauber, Jan, Aghanim, N., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cardoso, J. F., Catalano, A., Chamballu, A., Chiang, L. Y., Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Dick, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud Héraud, Y., Gjerløw, E., González Nuevo, J., Górski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot Versillé, S., Hernández Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden Vørnle, M., Lindholm, V., López Caniego, M., Lubin, P. M., Maciás Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubinõ Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur Uski, A. S., Sygnet, J. F., Tauber, J. A., Tavagnacco, Daniele, Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), 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), 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), 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), 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)-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), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, 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), PLANCK, University of Paris, University of Oxford, University of Paris Diderot, Kavli Institute for Cosmology, University of Salamanca, International School for Advanced Studies, Université de Toulouse, University of Granada, Pierre and Marie Curie University, California Institute of Technology, Istituto Nazionale Astrofisica - Italy, University of Manchester, University of Toronto, University of California Berkeley, Telecom ParisTech, Université Grenoble Alpes, Academia Sinica - Institute of Astronomy and Astrophysics, Niels Bohr Institute, University of Copenhagen, Stanford University, Sapienza University of Rome, Department of Radio Science and Engineering, Aalto-yliopisto, Aalto University, Department of Physics, Helsinki Institute of Physics, Hélium : du fondamental aux applications (NEEL - HELFA), 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), 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), École normale supérieure - Paris (ENS-PSL), 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)-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)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), 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), 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), 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)), 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 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), 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, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI)
Subjects: Calibration (statistics), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, Cosmic microwave background, data analysis, Astrophysics, cosmic background radiation, Residual, Cosmic background radiation, 7. Clean energy, 01 natural sciences, MAPS, Range (statistics), RADIOMETERS, 010303 astronomy & astrophysics, Cosmology: observations, Methods: data analysis, Physics, Astrophysics::Instrumentation and Methods for Astrophysics, Computer Science::Computers and Society, observations [cosmology], PLANCK, Physics::Space Physics, symbols, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], education, FOS: Physical sciences, observation [Cosmology], Computer Science::Digital Libraries, NO, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, Astronomy and Astrophysics, Space and Planetary Science, 0103 physical sciences, data analysis [methods], Planck, Spurious relationship, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010308 nuclear & particles physics, Spectral density, PERFORMANCE, Astronomy and Astrophysic, 115 Astronomy, Space science, Computational physics, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], data analysi [Methods], 13. Climate action, Multipole expansion, SKY, cosmology
Abstract: © 2014 ESO. We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-up and imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave background fluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipole range â.,> < 20, most notably at 30 GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reduce the level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibration uncertainties., The development of Planck has been supported by: 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 PRACE (EU).
Published: 2014

26. Planck 2013 results

Author: Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Beno��t, A., Benoit-L��vy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cappellini, B., Cardoso, J. -F., Catalano, A., Chamballu, A., Chen, X., Chiang, L. -Y, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Dor��, O., Douspis, M., Dupac, X., Efstathiou, G., En��lin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud-H��raud, Y., Gjerl��w, E., Gonz��lez-Nuevo, J., G��rski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versill��, S., Hern��ndez-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keih��nen, E., Keskitalo, R., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., L��hteenm��ki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden-V��rnle, M., L��pez-Caniego, M., Lubin, P. M., Mac��as-P��rez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Mart��nez-Gonz��lez, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., N��rgaard-Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Pr��zeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubi��o-Mart��n, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., T��rler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Universidad de Cantabria, Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), 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), 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), 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), 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, 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), PLANCK, Department of Physics, Helsinki Institute of Physics, Tauber, Jan, Aghanim, N., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M, Burigana, C., Butler, R. C., Cappellini, B., Cardoso, J. F., Catalano, A., Chamballu, A., Chen, X., Chiang, L. Y., Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud Héraud, Y., Gjerløw, E., González Nuevo, J., Górski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot Versillé, S., Hernández Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden Vørnle, M., López Caniego, M., Lubin, P. M., Maciás Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubinõ Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur Uski, A. S., Sygnet, J. F., Tauber, J. A., Tavagnacco, Daniele, Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Hélium : du fondamental aux applications (NEEL - HELFA), 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)-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), 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), École normale supérieure - Paris (ENS-PSL), 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)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), 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), Anne Lähteenmäki Group, Department of Electronics and Nanoengineering, Aalto-yliopisto, Aalto University, 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), 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 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), 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, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI)
Subjects: [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, Cosmic microwave background, data analysis, WMAP OBSERVATIONS, cosmic background radiation, Cosmic background radiation, Instrumentation: polarimeters, Methods: data analysis, 7. Clean energy, GHZ, data analysis [Methods], Physics, Detector, polarimeters, Astrophysics::Instrumentation and Methods for Astrophysics, instrumentation: polarimeters, CMB cold spot, Computer Science::Computers and Society, SKY MAPS, Brightness temperature, Physics::Space Physics, symbols, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, polarimeter [Instrumentation], Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astronomy and Astrophysics, Space and Planetary Science, education, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 114 Physical sciences, Computer Science::Digital Libraries, NO, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, Calibration, PRE-LAUNCH STATUS, Planck, Instrumentation and Methods for Astrophysics (astro-ph.IM), Radiometer, polarimeters [Instrumentation], Astronomy and Astrophysic, MICROWAVE-ANISOTROPY-PROBE, methods: data analysis, Computational physics, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], data analysi [Methods], Dipole
Abstract: We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the orbital dipole plus the solar dipole, caused respectively by the motion of the Planck spacecraft with respect to the Sun and by motion of the solar system with respect to the cosmic microwave background (CMB) rest frame. The latter provides a signal of a few mK with the same spectrum as the CMB anisotropies and is visible throughout the mission. In this data releasewe rely on the characterization of the solar dipole as measured by WMAP. We also present preliminary results (at 44 GHz only) on the study of the Orbital Dipole, which agree with the WMAP value of the solar system speed within our uncertainties. We compute the calibration constant for each radiometer roughly once per hour, in order to keep track of changes in the detectors' gain. Since non-idealities in the optical response of the beams proved to be important, we implemented a fast convolution algorithm which considers the full beam response in estimating the signal generated by the dipole. Moreover, in order to further reduce the impact of residual systematics due to sidelobes, we estimated time variations in the calibration constant of the 30 GHz radiometers (the ones with the largest sidelobes) using the signal of an internal reference load at 4 K instead of the CMB dipole. We have estimated the accuracy of the LFI calibration following two strategies: (1) we have run a set of simulations to assess the impact of statistical errors and systematic effects in the instrument and in the calibration procedure; and (2) we have performed a number of internal consistency checks on the data and on the brightness temperature of Jupiter. Errors in the calibration of this Planck/LFI data release are expected to be about 0.6% at 44 and 70 GHz, and 0.8% at 30 GHz. Both these preliminary results at low and high â.,> are consistent with WMAP results within uncertainties and comparison of power spectra indicates good consistency in the absolute calibration with HFI (0.3%) and a 1.4σ discrepancy with WMAP (0.9%)., The development of Planck has been supported by: 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 PRACE (EU).
Published: 2014

27. Planck 2013 results. IV. Low Frequency Instrument beams and window functions

Author: Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, Jacob, Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, Robb, Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, Lung-Yih, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, Rebecca, de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud-Héraud, Y., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, Steen, Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Lindholm, V., Linden-Vørnle, Michael, López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, Hans Ulrik, Novikov, D., Novikov, Igor Dmitrievich, O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, Frank, Vittorio, N., Wade, L. A., Wandelt, B. D., Zacchei, A., Zonca, A., Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, Jacob, Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, Robb, Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, Lung-Yih, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, Rebecca, de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud-Héraud, Y., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, Steen, Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Lindholm, V., Linden-Vørnle, Michael, López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, Hans Ulrik, Novikov, D., Novikov, Igor Dmitrievich, O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, Frank, Vittorio, N., Wade, L. A., Wandelt, B. D., Zacchei, A., and Zonca, A.
Abstract: This paper presents the characterization of the in-flight beams, the beam window functions and the associated errors for the Planck Low Frequency Instrument (LFI). Knowledge of the beam profiles is the key to determining their imprint on the transfer function from the observed to the actual sky anisotropy power spectrum. The main beam distortions affect the beam window function, complicating the reconstruction of the anisotropy power spectrum at high multipoles, whereas the sidelobes affect the low and intermediate multipoles. The in-flight assessment of the LFI main beams relied on the measurements performed during Jupiter observations. By stacking the data from Jupiter transits, the main beam profiles are measured down to -20 dB at 30 and 44 GHz, and down to -25 dB at 70 GHz. The main beam solid angles are determined to better than 0.2% at each LFI frequency band. To ensure a characterization of the main beam free from the radiometer noise, a dedicated tuning on the Planck pre-launch optical model is performed. This approach provides an optical model whose beams fully reproduce the measurements in the main beam region, but also allow us to describe the beams at power levels lower than can be reached by the Jupiter measurements themselves. The agreement between the simulated beams and the scanning beams is better than 1% at each LFI frequency band. The simulated beams are used for the computation of the window functions for the effective beams. The error budget in the window functions was estimated considering both main beam and sidelobe contributions, as well as taking into account the radiometer bandshapes. The total uncertainties in the effective beam window functions are: (at ell = 600) 2% and 1.2% at 30 and 44 GHz, respectively; and at ell = 1000, 0.7% at 70 GHz.
Published: 2014

28. Planck 2013 results. V. LFI calibration

Author: Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, Jacob, Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, Robb, Cappellini, B., Cardoso, J. -F., Catalano, A., Chamballu, A., Chen, X., Chiang, Lung-Yih, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, Rebecca, de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, Steen, Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden-Vørnle, Michael, López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, Hans Ulrik, Novikov, D., Novikov, Igor Dmitrievich, O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, Frank, Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Planck Collaboration, Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, Jacob, Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, Robb, Cappellini, B., Cardoso, J. -F., Catalano, A., Chamballu, A., Chen, X., Chiang, Lung-Yih, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, Rebecca, de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, Steen, Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden-Vørnle, Michael, López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, Hans Ulrik, Novikov, D., Novikov, Igor Dmitrievich, O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, Frank, Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Abstract: We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on the Solar Dipole, caused by motion of the Solar System with respect to the CMB rest frame, which provides a signal of a few mK with the same spectrum as the CMB anisotrophies and is visible throughout the mission. In this data release we rely on the characterization of the Solar Dipole as measured by WMAP. We also present preliminary results on the study of the Orbital Dipole, caused by the motion of the Planck spacecraft, which agree with the WMAP value of the Solar System speed to 0.2%. We compute the calibration constant for each radiometer roughly once per hour, in order to keep track of changes in the detectors' gain. Since non-idealities in the optical response of the beams proved to be important, we implemented a fast convolution algorithm which considers the full beam response in estimating the signal generated by the dipole. Moreover, in order to further reduce the impact of residual systematics due to sidelobes, we estimated time variations in the calibration constant of the 30 GHz radiometers (the ones with the most important sidelobes) using the signal of an internal reference load at 4 K instead of the CMB dipole. We estimated the accuracy of the LFI calibration following two strategies: (1) we have run a set of simulations to assess the impact of statistical errors and systematic effects in the instrument and in the calibration procedure, and (2) we have performed a number of internal consistency checks on the data. Errors in the calibration of this Planck/LFI data release are expected to be about 0.6% at 44 and 70 GHz, and 0.8% at 30 GHz.
Published: 2014

29. Sunyaev-Zeldovich Effect Science with the Cornell-Caltech Atacama Telescope

Author: GOLWALA SUNIL, R, Battistelli, Elia Stefano, Bean, R, Blain, A. W., Bock, J. J., Cooray, A, Dragovan, M, Gaier, T. C., Glenn, J, Halpern, M, Komatsu, E, Lange, A. E., Readhead, A. C. S., Torchinsky, S, and Myers, S. T.
Published: 2007

30. Planck 2013 results. II. The Low Frequency Instrument data processing

Author: Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, Jacob, Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, Robb, Cappellini, B., Cardoso, J. -F., Catalano, A., Chamballu, A., Chen, X., Chiang, Lung-Yih, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, Rebecca, de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, Steen, Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Lindholm, V., Linden-Vørnle, Michael, López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, Hans Ulrik, Novikov, D., Novikov, Igor Dmitrievich, O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Salerno, E., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, Frank, Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wehus, I. K., White, S. D. M., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, Jacob, Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, Robb, Cappellini, B., Cardoso, J. -F., Catalano, A., Chamballu, A., Chen, X., Chiang, Lung-Yih, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, Rebecca, de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, Steen, Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Lindholm, V., Linden-Vørnle, Michael, López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, Hans Ulrik, Novikov, D., Novikov, Igor Dmitrievich, O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Salerno, E., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, Frank, Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wehus, I. K., White, S. D. M., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Abstract: We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5 months of operations at 30, 44, and 70 GHz. In particular, we discuss the various steps involved in reducing the data, from telemetry packets through to the production of cleaned, calibrated timelines and calibrated frequency maps. Data are continuously calibrated using the modulation induced on the mean temperature of the cosmic microwave background radiation by the proper motion of the spacecraft. Sky signals other than the dipole are removed by an iterative procedure based on simultaneous fitting of calibration parameters and sky maps. Noise properties are estimated from time-ordered data after the sky signal has been removed, using a generalized least squares map-making algorithm. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices, required to compute statistical uncertainties on LFI and Planck products, are also produced. Main beams are estimated down to the approximate to-20 dB level using Jupiter transits, which are also used for the geometrical calibration of the focal plane.
Published: 2013

31. Planck 2013 results. III. LFI systematic uncertainties

Author: Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, Jacob, Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, Robb, Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, Lung-Yih, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, Rebecca, de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dick, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, Steen, Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Lindholm, V., Linden-Vørnle, Michael, López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, Hans Ulrik, Novikov, D., Novikov, Igor Dmitrievich, O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, Frank, Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, Jacob, Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, Robb, Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, Lung-Yih, Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, Rebecca, de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dick, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, Steen, Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, Allan, Hovest, W., Huffenberger, K. M., Jaffe, T. R., Jaffe, A. H., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Lindholm, V., Linden-Vørnle, Michael, López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard-Nielsen, Hans Ulrik, Novikov, D., Novikov, Igor Dmitrievich, O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, Frank, Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., and Zonca, A.
Abstract: We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the firstrelease of the Planck cosmological results.We give an overview of the main effects and of the tools and methods applied to assess residuals in mapsand power spectra.We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-upand imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave backgroundfluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipolerange ∫ < 20, most notably at 30GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reducethe level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibrationuncertainties.
Published: 2013

32. 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. 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, 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

33. 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

34. Planckearly results. III. First assessment of the Low Frequency Instrument in-flight performance

Author: Mennella, A., primary, Bersanelli, M., additional, Butler, R. C., additional, Curto, A., additional, Cuttaia, F., additional, Davis, R. J., additional, Dick, J., additional, Frailis, M., additional, Galeotta, S., additional, Gregorio, A., additional, Kurki-Suonio, H., additional, Lawrence, C. R., additional, Leach, S., additional, Leahy, J. P., additional, Lowe, S., additional, Maino, D., additional, Mandolesi, N., additional, Maris, M., additional, Martínez-González, E., additional, Meinhold, P. R., additional, Morgante, G., additional, Pearson, D., additional, Perrotta, F., additional, Polenta, G., additional, Poutanen, T., additional, Sandri, M., additional, Seiffert, M. D., additional, Suur-Uski, A.-S., additional, Tavagnacco, D., additional, Terenzi, L., additional, Tomasi, M., additional, Valiviita, J., additional, Villa, F., additional, Watson, R., additional, Wilkinson, A., additional, Zacchei, A., additional, Zonca, A., additional, Aja, B., additional, Artal, E., additional, Baccigalupi, C., additional, Banday, A. J., additional, Barreiro, R. B., additional, Bartlett, J. G., additional, Bartolo, N., additional, Battaglia, P., additional, Bennett, K., additional, Bonaldi, A., additional, Bonavera, L., additional, Borrill, J., additional, Bouchet, F. R., additional, Burigana, C., additional, Cabella, P., additional, Cappellini, B., additional, Chen, X., additional, Colombo, L., additional, Cruz, M., additional, Danese, L., additional, D’Arcangelo, O., additional, Davies, R. D., additional, de Gasperis, G., additional, de Rosa, A., additional, de Zotti, G., additional, Dickinson, C., additional, Diego, J. M., additional, Donzelli, S., additional, Efstathiou, G., additional, Enßlin, T. A., additional, Eriksen, H. K., additional, Falvella, M. C., additional, Finelli, F., additional, Foley, S., additional, Franceschet, C., additional, Franceschi, E., additional, Gaier, T. C., additional, Génova-Santos, R. T., additional, George, D., additional, Gómez, F., additional, González-Nuevo, J., additional, Górski, K. M., additional, Gruppuso, A., additional, Hansen, F. K., additional, Herranz, D., additional, Herreros, J. M., additional, Hoyland, R. J., additional, Hughes, N., additional, Jewell, J., additional, Jukkala, P., additional, Juvela, M., additional, Kangaslahti, P., additional, Keihänen, E., additional, Keskitalo, R., additional, Kilpia, V.-H., additional, Kisner, T. S., additional, Knoche, J., additional, Knox, L., additional, Laaninen, M., additional, Lähteenmäki, A., additional, Lamarre, J.-M., additional, Leonardi, R., additional, León-Tavares, J., additional, Leutenegger, P., additional, Lilje, P. B., additional, López-Caniego, M., additional, Lubin, P. M., additional, Malaspina, M., additional, Marinucci, D., additional, Massardi, M., additional, Matarrese, S., additional, Matthai, F., additional, Melchiorri, A., additional, Mendes, L., additional, Miccolis, M., additional, Migliaccio, M., additional, Mitra, S., additional, Moss, A., additional, Natoli, P., additional, Nesti, R., additional, Nørgaard-Nielsen, H. U., additional, Pagano, L., additional, Paladini, R., additional, Paoletti, D., additional, Partridge, B., additional, Pasian, F., additional, Pettorino, V., additional, Pietrobon, D., additional, Pospieszalski, M., additional, Prézeau, G., additional, Prina, M., additional, Procopio, P., additional, Puget, J.-L., additional, Quercellini, C., additional, Rachen, J. P., additional, Rebolo, R., additional, Reinecke, M., additional, Ricciardi, S., additional, Robbers, G., additional, Rocha, G., additional, Roddis, N., additional, Rubi no-Martín, J. A., additional, Savelainen, M., additional, Scott, D., additional, Silvestri, R., additional, Simonetto, A., additional, Sjoman, P., additional, Smoot, G. F., additional, Sozzi, C., additional, Stringhetti, L., additional, Tauber, J. A., additional, Tofani, G., additional, Toffolatti, L., additional, Tuovinen, J., additional, Türler, M., additional, Umana, G., additional, Valenziano, L., additional, Varis, J., additional, Vielva, P., additional, Vittorio, N., additional, Wade, L. A., additional, Watson, C., additional, White, S. D. M., additional, and Winder, F., additional
Published: 2011
Full Text: View/download PDF

35. Planckearly results. V. The Low Frequency Instrument data processing

Author: Zacchei, A., primary, Maino, D., additional, Baccigalupi, C., additional, Bersanelli, M., additional, Bonaldi, A., additional, Bonavera, L., additional, Burigana, C., additional, Butler, R. C., additional, Cuttaia, F., additional, de Zotti, G., additional, Dick, J., additional, Frailis, M., additional, Galeotta, S., additional, González-Nuevo, J., additional, Górski, K. M., additional, Gregorio, A., additional, Keihänen, E., additional, Keskitalo, R., additional, Knoche, J., additional, Kurki-Suonio, H., additional, Lawrence, C. R., additional, Leach, S., additional, Leahy, J. P., additional, López-Caniego, M., additional, Mandolesi, N., additional, Maris, M., additional, Matthai, F., additional, Meinhold, P. R., additional, Mennella, A., additional, Morgante, G., additional, Morisset, N., additional, Natoli, P., additional, Pasian, F., additional, Perrotta, F., additional, Polenta, G., additional, Poutanen, T., additional, Reinecke, M., additional, Ricciardi, S., additional, Rohlfs, R., additional, Sandri, M., additional, Suur-Uski, A.-S., additional, Tauber, J. A., additional, Tavagnacco, D., additional, Terenzi, L., additional, Tomasi, M., additional, Valiviita, J., additional, Villa, F., additional, Zonca, A., additional, Banday, A. J., additional, Barreiro, R. B., additional, Bartlett, J. G., additional, Bartolo, N., additional, Bedini, L., additional, Bennett, K., additional, Binko, P., additional, Borrill, J., additional, Bouchet, F. R., additional, Bremer, M., additional, Cabella, P., additional, Cappellini, B., additional, Chen, X., additional, Colombo, L., additional, Cruz, M., additional, Curto, A., additional, Danese, L., additional, Davies, R. D., additional, Davis, R. J., additional, de Gasperis, G., additional, de Rosa, A., additional, de Troia, G., additional, Dickinson, C., additional, Diego, J. M., additional, Donzelli, S., additional, Dörl, U., additional, Efstathiou, G., additional, Enßlin, T. A., additional, Eriksen, H. K., additional, Falvella, M. C., additional, Finelli, F., additional, Franceschi, E., additional, Gaier, T. C., additional, Gasparo, F., additional, Génova-Santos, R. T., additional, Giardino, G., additional, Gómez, F., additional, Gruppuso, A., additional, Hansen, F. K., additional, Hell, R., additional, Herranz, D., additional, Hovest, W., additional, Huynh, M., additional, Jewell, J., additional, Juvela, M., additional, Kisner, T. S., additional, Knox, L., additional, Lähteenmäki, A., additional, Lamarre, J.-M., additional, Leonardi, R., additional, León-Tavares, J., additional, Lilje, P. B., additional, Lubin, P. M., additional, Maggio, G., additional, Marinucci, D., additional, Martínez-González, E., additional, Massardi, M., additional, Matarrese, S., additional, Meharga, M. T., additional, Melchiorri, A., additional, Migliaccio, M., additional, Mitra, S., additional, Moss, A., additional, Nørgaard-Nielsen, H. U., additional, Pagano, L., additional, Paladini, R., additional, Paoletti, D., additional, Partridge, B., additional, Pearson, D., additional, Pettorino, V., additional, Pietrobon, D., additional, Prézeau, G., additional, Procopio, P., additional, Puget, J.-L., additional, Quercellini, C., additional, Rachen, J. P., additional, Rebolo, R., additional, Robbers, G., additional, Rocha, G., additional, Rubiño-Martín, J. A., additional, Salerno, E., additional, Savelainen, M., additional, Scott, D., additional, Seiffert, M. D., additional, Silk, J. I., additional, Smoot, G. F., additional, Sternberg, J., additional, Stivoli, F., additional, Stompor, R., additional, Tofani, G., additional, Toffolatti, L., additional, Tuovinen, J., additional, Türler, M., additional, Umana, G., additional, Vielva, P., additional, Vittorio, N., additional, Vuerli, C., additional, Wade, L. A., additional, Watson, R., additional, White, S. D. M., additional, and Wilkinson, A., additional
Published: 2011
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36. 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
Full Text: View/download PDF

37. GeoSTAR: a geostationary microwave sounder for the future

Author: Lambrigtsen, B. H., primary, Brown, S. T., additional, Dinardo, S. J., additional, Gaier, T. C., additional, Kangaslahti, P. P., additional, and Tanner, A. B., additional
Published: 2007
Full Text: View/download PDF

38. GeoSTAR: a microwave sounder for geostationary applications

Author: Lambrigtsen, B. H., primary, Brown, S. T., additional, Dinardo, S. J., additional, Gaier, T. C., additional, Kangaslahti, P. P., additional, Tanner, A. B., additional, Piepmeier, J. R., additional, Ruf, C. S., additional, Gross, S. M., additional, Musko, S., additional, and Rogacki, S., additional
Published: 2006
Full Text: View/download PDF

39. Anisotropy in the cosmic microwave background: present status-future directions

Author: Gundersen, J., Lim, M., Staren, J., Wuensche, Carlos Alexandre, Figueiredo, N., Childers, J., Levy, A., Gaier, T. C., Meinhold, P. R., Seiffert, M. D., Lubin, P. M., Gundersen, J., Lim, M., Staren, J., Wuensche, Carlos Alexandre, Figueiredo, N., Childers, J., Levy, A., Gaier, T. C., Meinhold, P. R., Seiffert, M. D., and Lubin, P. M.
Abstract: Measurments of the cosmic microwave background (CMB) stand as one of the experimental pillars of modern cosmology. In particular, anisotropy measurments of the CME have been shown to be very powerful tests of theories which attempt to explain the origin, evolution, matter content, and geometry of the Universe. When anisotropy measurements are combined with maps of the galaxy distribution, they can also be used to gain information about the origin of large scale structure in the Universe. Since the detection of anisotropy by the Cosmic Background Explorer (COBE) satellite,1l there has been a concerted effort to measure anisotropy at higher angular resolution with particular emphasis on medium/degree angular scales. In this talk, the scientific motivation behind these measurements is reviewed, a summary of the medium angular scale measurements is presented, and a description of some of the future experiments is given., Pages: 309-318
Published: 1995

40. CMB power spectra and likelihood

Author: Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Battaner, E., Benabed, K., Benoit, A., Benoit-Levy, A., Bemard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Catalano, A., Challinor, A., Chamballu, A., Chiang, H. C., Chiang, L. -Y, Christensen, P. R., Church, S., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., De Bemardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Delouis, J. -M., Desert, F. -X., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Dore, O., Douspis, M., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Ensslin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Gaier, T. C., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giardino, G., Giraud-Heraud, Y., Gjerlow, E., Gonzalez-Nuevo, J., Gorski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Hansen, F. K., Hanson, D., Harrison, D., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Homtrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Keihanen, E., Kesldtalo, R., Kiiveri, K., Kisner, T. S., Krieiss, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lawrence, C. R., Le Jeune, M., Leach, S., Leahy, J. P., Leonardi, R., Leon-Tavares, J., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden-Vornle, M., Lindholm, V., Lopez-Caniego, M., Lubin, P. M., Macias-Perez, J. F., Maffei, B., Maino, D., Mandolesi, N., Marinucci, D., Maris, M., Marshall, D. J., Martin, P. G., Martinez-Gonzalez, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschenes, M. -A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C. B., Norgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I. J., Orieux, F., Osborne, S., Oxborrow, C. A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Paykari, P., Perdereaun, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prezeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rahlin, A., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Riller, T., Ringeval, C., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rowan-Robinson, M., Rubino-Martin, J. A., Rusholme, B., Sandri, M., Sanselme, L., Santos, D., Savini, G., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Sudiwala, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Tuerler, M., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Wehus, I. K., White, M., White, S. D. M., Yvon, D., Zacchei, A., and Zonca, A.
Subjects: cosmology: observations, Astrophysics::Cosmology and Extragalactic Astrophysics, cosmic background radiation, cosmological parameters, methods: data analysis
Abstract: This paper presents the Planck 2013 likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations that accounts for all known relevant uncertainties, both instrumental and astrophysical in nature. We use this likelihood to derive our best estimate of the CMB angular power spectrum from Planck over three decades in multipole moment, t, covering 2 2500. The main source of uncertainty at S 1500 is cosmic variance. Uncertainties in small-scale foreground modelling and instrumental noise dominate the error budget at higher Es. For < 50, our likelihood exploits all Planck frequency channels from 30 to 353 GHz, separating the cosmological CMB signal from diffuse Galactic foregrounds through a physically motivated Bayesian component separation technique. At 50, we employ a correlated Gaussian likelihood approximation based on a fine-grained set of angular cross-spectra derived from multiple detector combinations between the 100, 143, and 217 GHz frequency channels, marginalising over power spectrum foreground templates. We validate our likelihood through an extensive suite of consistency tests, and assess the impact of residual foreground and instrumental uncertainties on the final cosmological parameters. We find good internal agreement among the high- cross-spectra with residuals below a few fiK2 at S 1000, in agreement with estimated calibration uncertainties. We compare our results with foreground-cleaned CMB maps derived from all Planck frequencies, as well as with cross-spectra derived from the 70 GHz Planck map, and find broad agreement in terms of spectrum residuals and cosmological parameters. We further show that the best-fit ACDM cosmology is in excellent agreement with preliminary Planck EE and T E polarisation spectra. We find that the standard ACDM cosmology is well constrained by Planck from the measurements at C 1500. One specific example is the spectral index of scalar perturbations, for which we report a 5.4o- deviation from scale invariance, ns = 1. Increasing the multipole range beyond = 1500 does not increase our accuracy for the ACDM parameters, but instead allows us to study extensions beyond the standard model. We find no indication of significant departures from the ACDM framework. Finally, we report a tension between the Planck best-fit ACDM model and the low- spectrum in the form of a power deficit of 5-10% at 40, with a statistical significance of 2.5-3o-. Without a theoretically motivated model for this power deficit, we do not elaborate further on its cosmological implications, but note that this is our most puzzling finding in an otherwise remarkably consistent data set.

41. LFI systematic uncertainties

Author: Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoit, A., Benoit-Levy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, L. -Y, Cristensen, P. R., Church, S., Olombi, S. C., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rose, A., De Zotti, G., Delabrouillei, J., Dick, J., Dickinson, C., Diego, J. M., Dole, H., Donzeli, S., Dore, O., Douspis, M., Dupac, X., Efstathiou, G., Ensslin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud-Heraud, Y., Gjerlow, E., Gonzalez-Nuevo, J., Gorski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kaneaslahti, P., Keihanen, E., Keskitalo, R., Kuveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J. -M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden-Vornle, M., Lindholm, V., Lopez-Caniego, M., Lubin, P. M., Macias-Perez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martinez-Gonzalez, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Mieliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Norgaard-Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, D., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, I., Poutanen, T., Pratt, G. W., Prezeau, G., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubino-Martin, J. A., Rusholme, B., Sandri, M., Salltos, D., Scott, D., Seitiert, M. A., Shellard, E. P. S., Spencer, L. D., Starck, J. -L., Stolyarov, V., Stompor, R., Stueau, F., Sutton, D., Sum-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Tavaenacco, D., Terenzi, L., Totfolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Turler, M., Umana, G., Valenziano, L., Vaiiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., and Planck Collaboration
Subjects: cosmology: observations, cosmic background radiation, methods: data analysis
Abstract: We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-up and imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave background fluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipole range l < 20, most notably at 30GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reduce the level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibration uncertainties.

42. Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance ⋆

Author: Mennella, A., Bersanelli, M., Butler, R. C., Curto, A., Cuttaia, F., Davis, R. J., Dick, J., Frailis, M., Galeotta, S., Gregorio, A., Kurki-Suonio, H., Lawrence, C. R., Leach, S., Leahy, J. P., Lowe, S., Maino, D., Mandolesi, N., Maris, M., Martínez-González, E., Meinhold, P. R., Morgante, G., Pearson, D., Perrotta, F., Polenta, G., Poutanen, T., Sandri, M., Seiffert, M. D., Suur-Uski, A.-S., Tavagnacco, D., Terenzi, L., Tomasi, M., Valiviita, J., Villa, F., Watson, R., Wilkinson, A., Zacchei, A., Zonca, A., Aja, B., Artal, E., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., Battaglia, P., Bennett, K., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F. R., Burigana, C., Cabella, P., Cappellini, B., Chen, X., Colombo, L., Cruz, M., Danese, L., D’Arcangelo, O., Davies, R. D., de Gasperis, G., de Rosa, A., de Zotti, G., Dickinson, C., Diego, J. M., Donzelli, S., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Foley, S., Franceschet, C., Franceschi, E., Gaier, T. C., Génova-Santos, R. T., George, D., Gómez, F., González-Nuevo, J., Górski, K. M., Gruppuso, A., Hansen, F. K., Herranz, D., Herreros, J. M., Hoyland, R. J., Hughes, N., Jewell, J., Jukkala, P., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kilpia, V.-H., Kisner, T. S., Knoche, J., Knox, L., Laaninen, M., Lähteenmäki, A., Lamarre, J.-M., Leonardi, R., León-Tavares, J., Leutenegger, P., Lilje, P. B., López-Caniego, M., Lubin, P. M., Malaspina, M., Marinucci, D., Massardi, M., Matarrese, S., Matthai, F., Melchiorri, A., Mendes, L., Miccolis, M., Migliaccio, M., Mitra, S., Moss, A., Natoli, P., Nesti, R., Nørgaard-Nielsen, H. U., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Pettorino, V., Pietrobon, D., Pospieszalski, M., Prézeau, G., Prina, M., Procopio, P., Puget, J.-L., Quercellini, C., Rachen, J. P., Rebolo, R., Reinecke, M., Ricciardi, S., Robbers, G., Rocha, G., Roddis, N., Rubi no-Martín, J. A., Savelainen, M., Scott, D., Silvestri, R., Simonetto, A., Sjoman, P., Smoot, G. F., Sozzi, C., Stringhetti, L., Tauber, J. A., Tofani, G., Toffolatti, L., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Varis, J., Vielva, P., Vittorio, N., Wade, L. A., Watson, C., White, S. D. M., and Winder, F.
Abstract: The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit operation is presented. We describe the main optical parameters and discuss photometric calibration, white noise sensitivity, and noise properties. A preliminary evaluation of the impact of the main systematic effects is presented. For each of the performance parameters, we outline the methods used to obtain them from the flight data and provide a comparison with pre-launch ground assessments, which are essentially confirmed in flight.
Published: 2011
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43. Planck 2013 results. XV. CMB power spectra and likelihood

Author: Tauber, J, Ade, P, Aghanim, N, Armitage Caplan, C, Arnaud, M, Ashdown, M, Atrio Barandela, F, Aumont, J, Baccigalupi, C, Banday, A, Barreiro, R, Bartlett, J, Battaner, E, Benabed, K, Benoit, A, Benoit Levy, A, Bernard, J, Bersanelli, M, Bielewicz, P, Bobin, J, Bock, J, Bonaldi, A, Bonavera, L, Bond, J, Borrill, J, Bouchet, F, Boulanger, F, Bridges, M, Bucher, M, Burigana, C, Butler, R, Calabrese, E, Cardoso, J, Catalano, A, Challinor, A, Chamballu, A, Chiang, H, Chiang, L, Christensen, P, Church, S, Clements, D, Colombi, S, Colombo, L, Combet, C, Couchot, F, Coulais, A, Crill, B, Curto, A, Cuttaia, F, Danese, L, Davies, R, Davis, R, De Bernardis, P, De Rosa, A, De Zotti, G, Delabrouille, J, Delouis, J, Desert, F, Dickinson, C, Diego, J, Dole, H, Donzelli, S, Dore, O, Douspis, M, Dunkley, J, Dupac, X, Efstathiou, G, Elsner, F, Ensslin, T, Eriksen, H, Finelli, F, Forni, O, Frailis, M, Fraisse, A, Franceschi, E, Gaier, T, Galeotta, S, Galli, S, Ganga, K, Giard, M, Giardino, G, Giraud Heraud, Y, Gjerlow, E, Gonzalez Nuevo, J, Gorski, K, Gratton, S, Gregorio, A, Gruppuso, A, Gudmundsson, J, Hansen, F, Hanson, D, Harrison, D, Helou, G, Henrot Versille, S, Hernandez Monteagudo, C, Herranz, D, Hildebrandt, S, Hivon, E, Hobson, M, Holmes, W, Hornstrup, A, Hovest, W, Huffenberger, K, Hurier, G, Jaffe, A, Jaffe, T, Jewell, J, Jones, W, Juvela, M, Keihanen, E, Keskitalo, R, Kiiveri, K, Kisner, T, Kneissl, R, Knoche, J, Knox, L, Kunz, M, Kurki Suonio, H, Lagache, G, Lahteenmaki, A, Lamarre, J, Lasenby, A, Lattanzi, M, Laureijs, R, Lawrence, C, Le Jeune, M, Leach, S, Leahy, J, Leonardi, R, Leon Tavares, J, Lesgourgues, J, Liguori, M, Lilje, P, Linden Vornle, M, Lindholm, V, Lopez Caniego, M, Lubin, P, Macias Perez, J, Maffei, B, Maino, D, Mandolesi, N, Marinucci, D, Maris, M, Marshall, D, Martin, P, Martinez Gonzalez, E, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, Meinhold, P, Melchiorri, A, Mendes, L, Menegoni, E, Mennella, A, Migliaccio, M, Millea, M, Mitra, S, Miville Deschenes, M, Molinari, D, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Moss, A, Munshi, D, Murphy, J, Naselsky, P, Nati, F, Natoli, P, Netterfield, C, Norgaard Nielsen, H, Noviello, F, Novikov, D, Novikov, I, O'Dwyer, I, Orieux, F, Osborne, S, Oxborrow, C, Paci, F, Pagano, L, Pajot, F, Paladini, R, Paoletti, D, Partridge, B, Pasian, F, Patanchon, G, Paykari, P, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, G, Prezeau, G, Prunet, S, Puget, J, Rachen, J, Rahlin, A, Rebolo, R, Reinecke, M, Remazeilles, M, Renault, C, Ricciardi, S, Riller, T, Ringeval, C, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rowan Robinson, M, Rubino Martin, J, Rusholme, B, Sandri, M, Sanselme, L, Santos, D, Savini, G, Scott, D, Seiffert, M, Shellard, E, Spencer, L, Starck, J, Stolyarov, V, Stompor, R, Sudiwala, R, Sureau, F, Sutton, D, Suur Uski, A, Sygnet, J, Tavagnacco, D, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Tuovinen, J, Turler, M, Valenziano, L, Valiviita, J, Van Tent, B, Varis, J, Vielva, P, Villa, F, Vittorio, N, Wade, L, Wandelt, B, Wehus, I, White, M, White, S, Yvon, D, Zacchei, A, Zonca, 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)-Centre National d’Études Spatiales [Paris] (CNES), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), 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), Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - 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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), 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), 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), Etablissement français du sang [Poitiers] (EFS), 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), Département de Physique des Particules (ex SPP) (DPP), 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 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 - 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CNRS), Centre National de la Recherche Scientifique (CNRS)-CentraleSupélec-Université Paris-Sud - Paris 11 (UP11), University of Geneva [Switzerland]-University of Geneva [Switzerland], Tauber, Jan, Ade, P. A. R., Aghanim, N., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Battaner, E., Benabed, K., Benoît, A., Benoit Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. F., Catalano, A., Challinor, A., Chamballu, A., Chiang, H. C., Chiang, L. Y., Christensen, P. R., Church, S., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Delouis, J. M., Désert, F. X., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Gaier, T. C., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giardino, G., Giraud Héraud, Y., Gjerløw, E., González Nuevo, J., Górski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Gudmundsson, J. E., Hansen, F. K., Hanson, D., Harrison, D., Helou, G., Henrot Versillé, S., Hernández Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lawrence, C. R., Le Jeune, M., Leach, S., Leahy, J. P., Leonardi, R., León Tavares, J., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden Vørnle, M., Lindholm, V., López Caniego, M., Lubin, P. M., Maciás Pérez, J. F., Maffei, B., Maino, D., Mandolesi, N., Marinucci, D., Maris, M., Marshall, D. J., Martin, P. G., Martínez González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville Deschênes, M. A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C. B., Nørgaard Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I. J., Orieux, F., Osborne, S., Oxborrow, C. A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Paykari, P., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. L., Rachen, J. P., Rahlin, A., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Riller, T., Ringeval, C., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rowan Robinson, M., Rubinõ Martín, J. A., Rusholme, B., Sandri, M., Sanselme, L., Santos, D., Savini, G., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. L., Stolyarov, V., Stompor, R., Sudiwala, R., Sureau, F., Sutton, D., Suur Uski, A. S., Sygnet, J. F., Tauber, J. A., Tavagnacco, Daniele, Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Wehus, I. K., White, M., White, S. D. M., Yvon, D., Zacchei, A., Zonca, A., Department of Physics, Helsinki Institute of Physics, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), 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), 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 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), 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), 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), Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-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 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), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Tauber, J, Ade, P, Aghanim, N, Armitage Caplan, C, Arnaud, M, Ashdown, M, Atrio Barandela, F, Aumont, J, Baccigalupi, C, Banday, A, Barreiro, R, Bartlett, J, Battaner, E, Benabed, K, Benoît, A, Benoit Lévy, A, Bernard, J, Bersanelli, M, Bielewicz, P, Bobin, J, Bock, J, Bonaldi, A, Bonavera, L, Bond, J, Borrill, J, Bouchet, F, Boulanger, F, Bridges, M, Bucher, M, Burigana, C, Butler, R, Calabrese, E, Cardoso, J, Catalano, A, Challinor, A, Chamballu, A, Chiang, H, Chiang, L, Christensen, P, Church, S, Clements, D, Colombi, S, Colombo, L, Combet, C, Couchot, F, Coulais, A, Crill, B, Curto, A, Cuttaia, F, Danese, L, Davies, R, Davis, R, DE BERNARDIS, P, De Rosa, A, De Zotti, G, Delabrouille, J, Delouis, J, Désert, F, Dickinson, C, Diego, J, Dole, H, Donzelli, S, Doré, O, Douspis, M, Dunkley, J, Dupac, X, Efstathiou, G, Elsner, F, Enßlin, T, Eriksen, H, Finelli, F, Forni, O, Frailis, M, Fraisse, A, Franceschi, E, Gaier, T, Galeotta, S, Galli, S, Ganga, K, Giard, M, Giardino, G, Giraud Héraud, Y, Gjerløw, E, González Nuevo, J, Górski, K, Gratton, S, Gregorio, A, Gruppuso, A, Gudmundsson, J, Hansen, F, Hanson, D, Harrison, D, Helou, G, Henrot Versillé, S, Hernández Monteagudo, C, Herranz, D, Hildebrandt, S, Hivon, E, Hobson, M, Holmes, W, Hornstrup, A, Hovest, W, Huffenberger, K, Hurier, G, Jaffe, A, Jaffe, T, Jewell, J, Jones, W, Juvela, M, Keihänen, E, Keskitalo, R, Kiiveri, K, Kisner, T, Kneissl, R, Knoche, J, Knox, L, Kunz, M, Kurki Suonio, H, Lagache, G, Lähteenmäki, A, Lamarre, J, Lasenby, A, Lattanzi, M, Laureijs, R, Lawrence, C, Le Jeune, M, Leach, S, Leahy, J, Leonardi, R, León Tavares, J, Lesgourgues, J, Liguori, M, Lilje, P, Linden Vørnle, M, Lindholm, V, López Caniego, M, Lubin, P, Maciás Pérez, J, Maffei, B, Maino, D, Mandolesi, N, Marinucci, D, Maris, M, Marshall, D, Martin, P, Martínez González, E, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, Meinhold, P, Melchiorri, A, Mendes, L, Menegoni, E, Mennella, A, Migliaccio, M, Millea, M, Mitra, S, Miville Deschênes, M, Molinari, D, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Moss, A, Munshi, D, Murphy, J, Naselsky, P, Nati, F, Natoli, P, Netterfield, C, Nørgaard Nielsen, H, Noviello, F, Novikov, D, Novikov, I, O'Dwyer, I, Orieux, F, Osborne, S, Oxborrow, C, Paci, F, Pagano, L, Pajot, F, Paladini, R, Paoletti, D, Partridge, B, Pasian, F, Patanchon, G, Paykari, P, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, G, Prézeau, G, Prunet, S, Puget, J, Rachen, J, Rahlin, A, Rebolo, R, Reinecke, M, Remazeilles, M, Renault, C, Ricciardi, S, Riller, T, Ringeval, C, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rowan Robinson, M, Rubinõ Martín, J, Rusholme, B, Sandri, M, Sanselme, L, Santos, D, Savini, G, Scott, D, Seiffert, M, Shellard, E, Spencer, L, Starck, J, Stolyarov, V, Stompor, R, Sudiwala, R, Sureau, F, Sutton, D, Suur Uski, A, Sygnet, J, Tavagnacco, D, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Tuovinen, J, Türler, M, Valenziano, L, Valiviita, J, Van Tent, B, Varis, J, Vielva, P, Villa, F, Vittorio, N, Wade, L, Wandelt, B, Wehus, I, White, M, White, S, Yvon, D, Zacchei, A, Zonca, A, 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), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Cosmological parameter, EXTRAGALACTIC SOURCES, Physics beyond the Standard Model, Astronomy, Cosmic microwave background, data analysis, Budget control, Calibration uncertainty, Astrophysics, cosmic background radiation, Correlation function (astronomy), Cosmic background radiation, Cosmology: observation, 7. Clean energy, 01 natural sciences, Cosmology, Cosmic ray measurement, cosmic background radiation, cosmological parameters, cosmology: observations, methods: data analysis, [INFO.INFO-TS]Computer Science [cs]/Signal and Image Processing, [MATH.MATH-ST]Mathematics [math]/Statistics [math.ST], Cosmological parameters, Cosmology: observations, Methods: data analysis, Two-point correlation function, 010303 astronomy & astrophysics, Spectroscopy, QC, QB, Physics, [PHYS]Physics [physics], [STAT.AP]Statistics [stat]/Applications [stat.AP], Astrophysics::Instrumentation and Methods for Astrophysics, Sigma, Planck temperature, Statistical significance, Computer Science::Computers and Society, observations [cosmology], MICROWAVE BACKGROUND ANISOTROPY, LOW-RESOLUTION DATA, Physics::Space Physics, Physical Sciences, symbols, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, SUPERNOVA LEGACY SURVEY, astro-ph.CO, Uncertainty analysis, ATACAMA COSMOLOGY TELESCOPE, Astrophysics - Cosmology and Nongalactic Astrophysics, Statistical descriptions, Astrophysics and Astronomy, Cosmology and Nongalactic Astrophysics (astro-ph.CO), COMPONENT SEPARATION, education, FOS: Physical sciences, observation [Cosmology], Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, Computer Science::Digital Libraries, NO, Power spectrum, symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, STAR-FORMING GALAXIES, data analysis [methods], Planck, cosmological parameters, Settore MAT/07 - Fisica Matematica, Science & Technology, SOUTH-POLE TELESCOPE, 010308 nuclear & particles physics, Spectral density, Astronomy and Astrophysics, Astronomy and Astrophysic, 115 Astronomy, Space science, Space and Planetary Science, Settore MAT/06 - Probabilita' e Statistica Matematica, data analysi [Methods], 0201 Astronomical And Space Sciences, PROBE WMAP OBSERVATIONS, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], SUNYAEV-ZELDOVICH, cosmology, Methods: data analysi
Abstract: Planck (http://www.esa.int/Planck) is a project of the European Space Agency (ESA), Ade, P.A.R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Bartlett, J.G., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J.J., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Bridges, M., Bucher, M., Burigana, C., Butler, R.C., Calabrese, E., Cardoso, J.-F., Catalano, A., Challinor, A., Chamballu, A., Chiang, H.C., Chiang, L.-Y., Christensen, P.R., Church, S., Clements, D.L., Colombi, S., Colombo, L.P.L., Combet, C., Couchot, F., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Delouis, J.-M., Désert, F.-X., Dickinson, C., Diego, J.M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T.A., Eriksen, H.K., Finelli, F., Forni, O., Frailis, M., Fraisse, A.A., Franceschi, E., Gaier, T.C., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K.M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J.E., Hansen, F.K., Hanson, D., Harrison, D., Helou, G., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Jewell, J., Jones, W.C., Juvela, M., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T.S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J.-M., Lasenby, A., Lattanzi, M., Laureijs, R.J., Lawrence, C.R., Le Jeune, M., Leach, S., Leahy, J.P., Leonardi, R., León-Tavares, J., Lesgourgues, J., Liguori, M., Lilje, P.B., Linden-Vørnle, M., Lindholm, V., López-Caniego, M., Lubin, P.M., Maciás-Pérez, J.F., Maffei, B., Maino, D., Mandolesi, N., Marinucci, D., Maris, M., Marshall, D.J., Martin, P.G., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, M.-A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Nørgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., O'dwyer, I.J., Orieux, F., Osborne, S., Oxborrow, C.A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Paykari, P., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G.W., Prézeau, G., Prunet, S., Puget, J.-L., Rachen, J.P., Rahlin, A., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Riller, T., Ringeval, C., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rowan-Robinson, M., Rubinõ-Martín, J.A., Rusholme, B., Sandri, M., Sanselme, L., Santos, D., Savini, G., Scott, D., Seiffert, M.D., Shellard, E.P.S., Spencer, L.D., Starck, J.-L., Stolyarov, V., Stompor, R., Sudiwala, R., Sureau, F., Sutton, D., Suur-Uski, A.-S., Sygnet, J.-F., Tauber, J.A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L.A., Wandelt, B.D., Wehus, I.K., White, M., White, S.D.M., Yvon, D., Zacchei, A., Zonca, A.
Published: 2014

44. Planck 2013 results

Author: T. Poutanen, Olivier Doré, K. Ganga, O. Perdereau, Peter A. R. Ade, Jose M. Diego, Krzysztof M. Gorski, V. Stolyarov, Y. Giraud-Héraud, E. Franceschi, I. Ristorcelli, Martin Kunz, Duncan Hanson, P. R. Christensen, C. Hernández-Monteagudo, P. M. McGehee, Mathieu Remazeilles, Anthony Lasenby, L. Sanselme, Monique Arnaud, Charles R. Lawrence, Jon E. Gudmundsson, L. Pagano, S. Galeotta, F. Piacentini, E. Keihänen, W. Hovest, F. Melot, William T. Reach, Guilaine Lagache, Jean-François Cardoso, Francesca Perrotta, L. Perotto, Allan Hornstrup, George Helou, Etienne Pointecouteau, M. López-Caniego, Alessandro Melchiorri, Kevin M. Huffenberger, Alain Benoit, D. L. Harrison, R. Leonardi, Michele Liguori, Theodore Kisner, Hans Ulrik Nørgaard-Nielsen, C. North, C. Leroy, M. Maris, N. Ponthieu, A. de Rosa, R.-R. Chary, Jo Dunkley, M. Tucci, Stéphane Colombi, J. J. Bock, M. Ashdown, Pavel Naselsky, R. J. Davis, Andrea Zacchei, H. K. Eriksen, Francine R. Marleau, J. W. Bowyer, Fabrizio Villa, M. Bridges, M. Tomasi, F. Cuttaia, W. A. Holmes, B. Racine, A. Chamballu, Torsten A. Enßlin, Locke D. Spencer, Olivier Forni, J. Aumont, S. R. Hildebrandt, A. Benoit-Lévy, Daniel J. Mortlock, M.-A. Miville-Deschênes, M. Giard, E. Pierpaoli, Aurelien A. Fraisse, M. Frailis, Carlo Baccigalupi, E. Hivon, S. Techene, S. Mottet, P. B. Lilje, D. Sutton, W. C. Jones, F. K. Hansen, J. Knoche, Marco Bersanelli, Roberta Paladini, Simon Prunet, Carlo Burigana, Simon D. M. White, P. Bielewicz, B. P. Crill, Lung-Yih Chiang, S. Donzelli, D. Girard, A. Curto, Peter G. Martin, François R. Bouchet, Serge Gratton, A. Sauvé, F.-X. Désert, J. Bobin, G. W. Pratt, D. Herranz, M. Le Jeune, D. Yvon, Michael Rowan-Robinson, Nicola Vittorio, L. P. L. Colombo, F. Matthai, C. Armitage-Caplan, Giorgio Savini, A. Catalano, Gianluca Morgante, T. Riller, Dmitry Novikov, Bruno Maffei, Clive Dickinson, Xin Chen, J.-L. Puget, Pasquale Mazzotta, J.-F. Sygnet, Stéphane Plaszczynski, L. Vibert, X. Dupac, Carol Anne Oxborrow, M. Reinecke, Davide Pietrobon, E. Battaner, L. A. Wade, Daniela Paoletti, F. Pajot, Reijo Keskitalo, M. Bucher, Douglas Scott, Luigi Danese, Dipak Munshi, George Efstathiou, L. Popa, Ben Rusholme, P. Vielva, D. Santos, A. Mennella, Nabila Aghanim, Luca Valenziano, A. Coulais, F. Atrio-Barandela, Calvin B. Netterfield, G. Giardino, T. R. Jaffe, O. Herent, Marcella Massardi, R. Kneissl, Jacques Delabrouille, François Orieux, J.-M. Delouis, M. Migliaccio, N. Mandolesi, J. A. Murphy, A. Moneti, Radek Stompor, Federico Nati, E. P. S. Shellard, Luca Terenzi, C. Combet, Andrew H. Jaffe, G. Umana, G. de Zotti, René J. Laureijs, Mika Juvela, F. Boulanger, Jussi-Pekka Väliviita, G. Patanchon, F. Couchot, I. D. Novikov, Philip Lubin, Fabio Finelli, Peter Meinhold, F. Paci, Sophie Henrot-Versille, Alessandro Gruppuso, Z. Hou, R. D. Davies, F. Noviello, J. González-Nuevo, G. Prézeau, Paolo Natoli, Andrea Zonca, K. Benabed, A. Gregorio, Marian Douspis, H. C. Chiang, J. R. Bond, Michael P. Hobson, Franck Sureau, B. Van Tent, J.-M. Lamarre, L. Mendes, S. Osborne, A. J. Banday, A.-S. Suur-Uski, Sabino Matarrese, H. Dole, Subhabrata Mitra, J. A. Tauber, Hannu Kurki-Suonio, J. Lesgourgues, G. Hurier, C. J. MacTavish, Lloyd Knox, David L. Clements, G. Roudier, P. de Bernardis, C. Rosset, Silvia Masi, Jean-Luc Starck, D. J. Marshall, J. F. Macías-Pérez, Graca Rocha, L. Montier, F. Pasian, J.-P. Bernard, Benjamin D. Wandelt, M. Tristram, Julian Borrill, G. Polenta, M. Linden-Vørnle, Sarah E. Church, E. Martínez-González, M. Piat, D. Tavagnacco, Rafael Rebolo, R. B. Barreiro, R. Sudiwala, S. Ricciardi, Jörg P. Rachen, C. Renault, Tauber, Jan, Aghanim, N., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cappellini, B., Cardoso, J. F., Catalano, A., Chamballu, A., Chen, X., Chiang, L. Y., Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud Héraud, Y., Gjerløw, E., González Nuevo, J., Górski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot Versillé, S., Hernández Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lawrence, C. R., Leach, S., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden Vørnle, M., Lindholm, V., López Caniego, M., Lubin, P. M., MacIás Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Morisset, N., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Robbers, G., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubinõ Martín, J. A., Rusholme, B., Salerno, E., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur Uski, A. S., Sygnet, J. F., Tauber, J. A., Tavagnacco, Daniele, Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, R., Wehus, I. K., White, S. D. M., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A., Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), 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), 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), 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), 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, 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), PLANCK, Universidad de Cantabria, Hélium : du fondamental aux applications (NEEL - HELFA), 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)-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), 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), École normale supérieure - Paris (ENS-PSL), 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)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), 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), Anne Lähteenmäki Group, Department of Electronics and Nanoengineering, Aalto-yliopisto, Aalto University, HELFA - Hélium : du fondamental aux applications, Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), 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 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), 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), Department of Physics, and Helsinki Institute of Physics
Subjects: Astronomy, Cosmic microwave background, data analysis, Astrophysics, cosmic background radiation, Surveys, Cosmic background radiation, NOISE, RADIOMETERS, data analysis [Methods], observations [Cosmology], Survey, cosmology: observations, surveys [cosmic background radiation, methods], Physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Computer Science::Computers and Society, DATA SETS, Physics::Space Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - Instrumentation and Methods for Astrophysics, Noise (radio), Astrophysics and Astronomy, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], education, FOS: Physical sciences, observation [Cosmology], Computer Science::Digital Libraries, NO, Settore FIS/05 - Astronomia e Astrofisica, surveys, Calibration, PRE-LAUNCH STATUS, Angular resolution, Instrumentation and Methods for Astrophysics (astro-ph.IM), methods: data analysis, Radiometer, MAP-MAKING ALGORITHM, Instrument Data, Spectral density, Astronomy and Astrophysics, Astronomy and Astrophysic, 115 Astronomy, Space science, Cosmology: observations, Methods: data analysis, Space and Planetary Science, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], data analysi [Methods], cosmology
Abstract: We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5 months of operations at 30, 44, and 70 GHz. In particular, we discuss the various steps involved in reducing the data, from telemetry packets through to the production of cleaned, calibrated timelines and calibrated frequency maps. Data are continuously calibrated using the modulation induced on the mean temperature of the cosmic microwave background radiation by the proper motion of the spacecraft. Sky signals other than the dipole are removed by an iterative procedure based on simultaneous fitting of calibration parameters and sky maps. Noise properties are estimated from time-ordered data after the sky signal has been removed, using a generalized least squares map-making algorithm. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices, required to compute statistical uncertainties on LFI and Planck products, are also produced. Main beams are estimated down to the ≈−20 dB level using Jupiter transits, which are also used for the geometrical calibration of the focal plane., This work was supported by the Academy of Finland grants 253204, 256265, and 257989. We acknowledge financial support provided by the Spanish Ministerio de Ciencia e Innovaciõn through the Plan Nacional del Espacio y Plan Nacional de Astronomia y Astrofisica. The development of Planck has been supported by: 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 PRACE (EU).
Published: 2014

45. Planck 2013 results. I. Overview of products and scientific results

Author: J.-P. Bernard, Niraj Welikala, J. A. Murphy, Benjamin D. Wandelt, Julian Borrill, I. Flores-Cacho, Marc Türler, Pavel Naselsky, R. J. Davis, Jean-Baptiste Melin, Jussi Varis, J. Tuovinen, Olivier Forni, M.-A. Miville-Deschênes, J. Dick, Olivier Doré, Paolo Serra, L. Toffolatti, M. C. Falvella, K. Ganga, S. Leach, Jose M. Diego, Anthony Lasenby, F. K. Hansen, C. Li, E. Keihänen, Alessandro Melchiorri, R. A. Burenin, Alain Benoit, Jens Jasche, Antony Lewis, C. Gauthier, Simon D. M. White, Michael W. Peel, F. Piacentini, O. Fabre, Guilaine Lagache, Soumen Basak, George Helou, A. Mangilli, Ben Rusholme, B. Ruiz-Granados, A.-S. Suur-Uski, R. C. Butler, D. Girard, M. López-Caniego, Hervé Bourdin, Pasquale Mazzotta, C. Renault, E. Falgarone, T. Riller, Diego Molinari, A. Coulais, Pablo Fosalba, A. Moneti, William T. Reach, P. Carvalho, D. Tavagnacco, Anthony R. Pullen, Jose Alberto Rubino-Martin, A. Renzi, D. Herranz, C. Hernández-Monteagudo, C. Watson, E. Pierpaoli, F. Matthai, F. Schiavon, Roberta Paladini, Jeffrey Jewell, D. L. Harrison, B. Gandolfo, J. Aumont, Rafael Rebolo, G. Maggio, Ingunn Kathrine Wehus, M. Tucci, Jussi-Pekka Väliviita, S. Fromenteau, Daniel J. Mortlock, T. J. Pearson, X. Dupac, Jan Hamann, A. Ducout, I. J. O'Dwyer, Michele Liguori, Federico Nati, M. Sandri, Massimiliano Lattanzi, G. Patanchon, J. E. Gallegos, F. Paci, B. Cappellini, Luca Terenzi, R. Carr, Martin White, M. Bucher, Barbara Comis, Jun-Qing Xia, D. Sutton, Mariachiara Rossetti, S. Ricciardi, L. Mendes, C. Combet, Sabino Matarrese, Michael L. Brown, M. Bridges, Douglas Scott, L. Popa, R. Miniscalco, G. de Zotti, F. Cuttaia, Loïc Maurin, I. D. Novikov, B. M. Schaefer, Jörg P. Rachen, J.-M. Delouis, Reijo Keskitalo, Gayoung Chon, E. Franceschi, A. Curto, S. Colombi, Krzysztof M. Gorski, Domenico Marinucci, P. R. Christensen, Eloisa Menegoni, James J. Bock, Paul M. Sutter, G. Prézeau, T. Déchelette, T. Poutanen, Shirley Ho, Jean-François Cardoso, C. J. MacTavish, P. M. McGehee, Richard A. Battye, A. Marcos-Caballero, Anna Bonaldi, Charles R. Lawrence, Peter M. W. Kalberla, Mathieu Langer, Nicolas Ponthieu, S. Donzelli, Marius Millea, O. Perdereau, A. Benoit-Lévy, M. Giard, J. Démoclès, Dmitry Pogosyan, F. Pasian, Davide Pietrobon, Matthieu Roman, Matthias Bartelmann, A. Lavabre, Joanna Dunkley, Magnus Hansen, Erminia Calabrese, B. Racine, J. P. Torre, Marat Gilfanov, I. F. Bikmaev, Xun Chen, B. P. Crill, N. Bartolo, Lung-Yih Chiang, A. Riazuelo, A. Hempel, Alessandro Gruppuso, M. Le Jeune, F. Elsner, C. North, G. Umana, P. de Bernardis, C. Rosset, A. Da Silva, Adam Moss, M. Cruz, Ricardo Genova-Santos, Andrea Zacchei, Anne Lähteenmäki, Luigi Danese, J.-L. Puget, N. Morisset, Tomotake Matsumura, George F. Smoot, Theodore Kisner, Todd Gaier, Calvin B. Netterfield, Emanuele Salerno, Radek Stompor, E. Gjerløw, D. Santos, Giorgio Savini, François R. Bouchet, J. Kerp, S. Osborne, Nicola Vittorio, V. Lindholm, S. Galeotta, M. Tristram, R. Barrena, P. Vielva, Mika Juvela, J.-M. Lamarre, Claude Leroy, R. Kneissl, A. Catalano, Mattia Negrello, Marcella Massardi, G. Polenta, M. Linden-Vørnle, Sarah E. Church, Tarun Souradeep, Rashmikant V. Sudiwala, M. Casale, Ranga-Ram Chary, Jean-Luc Starck, Alexandra S. Rahlin, E. P. S. Shellard, Z. Hou, M. Freschi, F. Couchot, F. Noviello, Hannu Kurki-Suonio, G. Hurier, J. F. Macías-Pérez, G. Castex, Herve Aussel, Kevin M. Huffenberger, David Pearson, Irek Khamitov, L. Vibert, Créidhe O'Sullivan, Francine R. Marleau, James R. Fergusson, Lloyd Knox, Graca Rocha, David L. Clements, Georg Robbers, F. Boulanger, Jochen Weller, S. R. Lowe, J. W. Bowyer, Fabrizio Villa, B. Bertincourt, Marian Douspis, J. P. Zibin, C. Armitage-Caplan, W. A. Holmes, G. Roudier, S. Pandolfi, Hans Böhringer, I. Ristorcelli, Althea Wilkinson, W. C. Jones, M. Rowan-Robinson, M. Ashdown, Hiranya V. Peiris, Matteo Viel, A. B. McDonald, H. K. Eriksen, Silvia Masi, C. Filliard, A. Mennella, Nabila Aghanim, M. Tomasi, Laura Bonavera, E. Martínez-González, M. Frailis, Carlo Baccigalupi, E. Hivon, M. Piat, Douglas J. Marshall, Suzanne Foley, Marco Bersanelli, Alan Heavens, J.-F. Sygnet, Christophe Ringeval, Kendrick M. Smith, L. Sanselme, Luca Valenziano, Michael Seiffert, Andrew R. Liddle, M. Tuttlebee, Duncan Hanson, Stéphane Plaszczynski, R. B. Barreiro, Fernando Atrio-Barandela, K. Kiiveri, Michael P. Hobson, Clive Dickinson, Anthony Challinor, G. Giardino, Jonathan León-Tavares, H. Dole, Subhabrata Mitra, J. A. Tauber, S. Ilić, M. Savelainen, Peter Meinhold, J. González-Nuevo, A. A. Fraisse, B. Van Tent, A. J. Banday, P. Platania, Klaus Dolag, Yabebal Fantaye, D. Texier, A. de Rosa, David Taylor, Locke D. Spencer, J. Knoche, Simon Prunet, P. Bielewicz, M. Reinecke, L. Perotto, E. Churazov, Benjamin Winkel, V. Stolyarov, M. Maris, Bruno Maffei, Martin Kunz, Mathieu Remazeilles, F. Pajot, Marcel Clemens, Jon E. Gudmundsson, L. Pagano, François Orieux, N. Mandolesi, Andrew H. Jaffe, Philip Lubin, J. Kim, Jérôme Bobin, Davide Maino, A. Chamballu, Simona Mei, D. Yvon, W. Hovest, Håkon Dahle, Y. Giraud-Héraud, M. Frommert, R. A. Sunyaev, G. Huey, F. Lacasa, Monique Arnaud, J. P. Leahy, R. D. Davies, Nicole P. H. Nesvadba, Pekka Kangaslahti, K. Benabed, P. B. Lilje, Florent Sureau, J. R. Bond, Tuhin Ghosh, Valeria Pettorino, Jacques Delabrouille, Hans Ulrik Nørgaard-Nielsen, Allan Hornstrup, Etienne Pointecouteau, Jason D. McEwen, René J. Laureijs, Fabio Finelli, Christoph Räth, James G. Bartlett, S. R. Hildebrandt, Carlo Burigana, Sophie Henrot-Versille, Paolo Natoli, L. P. L. Colombo, Dmitry Novikov, L. A. Wade, Daniela Paoletti, Bruce Partridge, C. A. Oxborrow, Dipak Munshi, George Efstathiou, M. I. R. Alves, Peter G. Martin, E. Battaner, K. Mikkelsen, Matthieu Béthermin, Julien Lesgourgues, J. Haissinski, Robert A. Watson, Francesca Perrotta, Torsten A. Enßlin, Serge Gratton, F.-X. Désert, Andrea Zonca, A. Gregorio, H. C. Chiang, T. R. Jaffe, M. Migliaccio, Peter A. R. Ade, P. Paykari, R. Leonardi, Alain Blanchard, S. Galli, G. W. Pratt, Gianluca Morgante, L. Montier, 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)-Centre National d’Études Spatiales [Paris] (CNES), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), 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), 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), Hélium : du fondamental aux applications (NEEL - HELFA), Institut Néel (NEEL), 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), 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), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA (UMR_8112)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), 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), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), PLANCK, 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)), 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), HELFA - Hélium : du fondamental aux applications, Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), 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), APC - Gravitation (APC-Gravitation), 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), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, 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), Hélium : du fondamental aux applications (HELFA), 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), 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), 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), Tauber, Jan, Ade, P. A. R., Aghanim, N., Alves, M. I. R., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., Aumont, J., Aussel, H., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Barrena, R., Bartelmann, M., Bartlett, J. G., Bartolo, N., Basak, S., Battaner, E., Battye, R., Benabed, K., Benoît, A., Benoit Lévy, A., Bernard, J. P., Bersanelli, M., Bertincourt, B., Bethermin, M., Bielewicz, P., Bikmaev, I., Blanchard, A., Bobin, J., Bock, J. J., Böhringer, H., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bourdin, H., Bowyer, J. W., Bridges, M., Brown, M. L., Bucher, M., Burenin, R., Burigana, C., Butler, R. C., Calabrese, E., Cappellini, B., Cardoso, J. F., Carr, R., Carvalho, P., Casale, M., Castex, G., Catalano, A., Challinor, A., Chamballu, A., Chary, R. R., Chen, X., Chiang, H. C., Chiang, L. Y., Chon, G., Christensen, P. R., Churazov, E., Church, S., Clemens, M., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Comis, B., Couchot, F., Coulais, A., Crill, B. P., Cruz, M., Curto, A., Cuttaia, F., Da Silva, A., Dahle, H., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rosa, A., De Zotti, G., Déchelette, T., Delabrouille, J., Delouis, J. M., Démoclès, J., Désert, F. X., Dick, J., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Fabre, O., Falgarone, E., Falvella, M. C., Fantaye, Y., Fergusson, J., Filliard, C., Finelli, F., Flores Cacho, I., Foley, S., Forni, O., Fosalba, P., Frailis, M., Fraisse, A. A., Franceschi, E., Freschi, M., Fromenteau, S., Frommert, M., Gaier, T. C., Galeotta, S., Gallegos, J., Galli, S., Gandolfo, B., Ganga, K., Gauthier, C., Génova Santos, R. T., Ghosh, T., Giard, M., Giardino, G., Gilfanov, M., Girard, D., Giraud Héraud, Y., Gjerløw, E., González Nuevo, J., Górski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Gudmundsson, J. E., Haissinski, J., Hamann, J., Hansen, F. K., Hansen, M., Hanson, D., Harrison, D. L., Heavens, A., Helou, G., Hempel, A., Henrot Versillé, S., Hernández Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Ho, S., Hobson, M., Holmes, W. A., Hornstrup, A., Hou, Z., Hovest, W., Huey, G., Huffenberger, K. M., Hurier, G., Ilić, S., Jaffe, A. H., Jaffe, T. R., Jasche, J., Jewell, J., Jones, W. C., Juvela, M., Kalberla, P., Kangaslahti, P., Keihänen, E., Kerp, J., Keskitalo, R., Khamitov, I., Kiiveri, K., Kim, J., Kisner, T. S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki Suonio, H., Lacasa, F., Lagache, G., Lähteenmäki, A., Lamarre, J. M., Langer, M., Lasenby, A., Lattanzi, M., Laureijs, R. J., Lavabre, A., Lawrence, C. R., Le Jeune, M., Leach, S., Leahy, J. P., Leonardi, R., León Tavares, J., Leroy, C., Lesgourgues, J., Lewis, A., Li, C., Liddle, A., Liguori, M., Lilje, P. B., Linden Vørnle, M., Lindholm, V., López Caniego, M., Lowe, S., Lubin, P. M., Maciás Pérez, J. F., Mactavish, C. J., Maffei, B., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marcos Caballero, A., Marinucci, D., Maris, M., Marleau, F., Marshall, D. J., Martin, P. G., Martínez González, E., Masi, S., Massardi, M., Matarrese, S., Matsumura, T., Matthai, F., Maurin, L., Mazzotta, P., Mcdonald, A., Mcewen, J. D., Mcgehee, P., Mei, S., Meinhold, P. R., Melchiorri, A., Melin, J. B., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Mikkelsen, K., Millea, M., Miniscalco, R., Mitra, S., Miville Deschênes, M. A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Morisset, N., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Negrello, M., Nesvadba, N. P. H., Netterfield, C. B., Nørgaard Nielsen, H. U., North, C., Noviello, F., Novikov, D., Novikov, I., O'Dwyer, I. J., Orieux, F., Osborne, S., O'Sullivan, C., Oxborrow, C. A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Pandolfi, S., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Paykari, P., Pearson, D., Pearson, T. J., Peel, M., Peiris, H. V., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pogosyan, D., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. L., Pullen, A. R., Rachen, J. P., Racine, B., Rahlin, A., Räth, C., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Riazuelo, A., Ricciardi, S., Riller, T., Ringeval, C., Ristorcelli, I., Robbers, G., Rocha, G., Roman, M., Rosset, C., Rossetti, M., Roudier, G., Rowan Robinson, M., Rubinõ Martín, J. A., Ruiz Granados, B., Rusholme, B., Salerno, E., Sandri, M., Sanselme, L., Santos, D., Savelainen, M., Savini, G., Schaefer, B. M., Schiavon, F., Scott, D., Seiffert, M. D., Serra, P., Shellard, E. P. S., Smith, K., Smoot, G. F., Souradeep, T., Spencer, L. D., Starck, J. L., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sureau, F., Sutter, P., Sutton, D., Suur Uski, A. S., Sygnet, J. F., Tauber, J. A., Tavagnacco, Daniele, Taylor, D., Terenzi, L., Texier, D., Toffolatti, L., Tomasi, M., Torre, J. P., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Tuttlebee, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vibert, L., Viel, M., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Watson, C., Watson, R., Wehus, I. K., Welikala, N., Weller, J., White, M., White, S. D. M., Wilkinson, A., Winkel, B., Xia, J. Q., Yvon, D., Zacchei, A., Zibin, J. P., Zonca, A., Universidad de Cantabria, Ade, P, Aghanim, N, Alves, M, Armitage-Caplan, C, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Aussel, H, Baccigalupi, C, Banday, A, Barreiro, R, Barrena, R, Bartelmann, M, Bartlett, J, Bartolo, N, Basak, S, Battaner, E, Battye, R, Benabed, K, Benoît, A, Benoit-Lévy, A, Bernard, J, Bersanelli, M, Bertincourt, B, Bethermin, M, Bielewicz, P, Bikmaev, I, Blanchard, A, Bobin, J, Bock, J, Böhringer, H, Bonaldi, A, Bonavera, L, Bond, J, Borrill, J, Bouchet, F, Boulanger, F, Bourdin, H, Bowyer, J, Bridges, M, Brown, M, Bucher, M, Burenin, R, Burigana, C, Butler, R, Calabrese, E, Cappellini, B, Cardoso, J, Carr, R, Carvalho, P, Casale, M, Castex, G, Catalano, A, Challinor, A, Chamballu, A, Chary, R, Chen, X, Chiang, H, Chiang, L, Chon, G, Christensen, P, Churazov, E, Church, S, Clemens, M, Clements, D, Colombi, S, Colombo, L, Combet, C, Comis, B, Couchot, F, Coulais, A, Crill, B, Cruz, M, Curto, A, Cuttaia, F, Da Silva, A, Dahle, H, Danese, L, Davies, R, Davis, R, de Bernardis, P, de Rosa, A, de Zotti, G, Déchelette, T, Delabrouille, J, Delouis, J, Démoclès, J, Désert, F, Dick, J, Dickinson, C, Diego, J, Dolag, K, Dole, H, Donzelli, S, Doré, O, Douspis, M, Ducout, A, Dunkley, J, Dupac, X, Efstathiou, G, Elsner, F, Enßlin, T, Eriksen, H, Fabre, O, Falgarone, E, Falvella, M, Fantaye, Y, Fergusson, J, Filliard, C, Finelli, F, Flores-Cacho, I, Foley, S, Forni, O, Fosalba, P, Frailis, M, Fraisse, A, Franceschi, E, Freschi, M, Fromenteau, S, Frommert, M, Gaier, T, Galeotta, S, Gallegos, J, Galli, S, Gandolfo, B, Ganga, K, Gauthier, C, Génova-Santos, R, Ghosh, T, Giard, M, Giardino, G, Gilfanov, M, Girard, D, Giraud-Héraud, Y, Gjerløw, E, González-Nuevo, J, Górski, K, Gratton, S, Gregorio, A, Gruppuso, A, Gudmundsson, J, Haissinski, J, Hamann, J, Hansen, F, Hansen, M, Hanson, D, Harrison, D, Heavens, A, Helou, G, Hempel, A, Henrot-Versillé, S, Hernández-Monteagudo, C, Herranz, D, Hildebrandt, S, Hivon, E, Ho, S, Hobson, M, Holmes, W, Hornstrup, A, Hou, Z, Hovest, W, Huey, G, Huffenberger, K, Hurier, G, Ilić, S, Jaffe, A, Jaffe, T, Jasche, J, Jewell, J, Jones, W, Juvela, M, Kalberla, P, Kangaslahti, P, Keihänen, E, Kerp, J, Keskitalo, R, Khamitov, I, Kiiveri, K, Kim, J, Kisner, T, Kneissl, R, Knoche, J, Knox, L, Kunz, M, Kurki-Suonio, H, Lacasa, F, Lagache, G, Lähteenmäki, A, Lamarre, J, Langer, M, Lasenby, A, Lattanzi, M, Laureijs, R, Lavabre, A, Lawrence, C, Le Jeune, M, Leach, S, Leahy, J, Leonardi, R, León-Tavares, J, Leroy, C, Lesgourgues, J, Lewis, A, Li, C, Liddle, A, Liguori, M, Lilje, P, Linden-Vørnle, M, Lindholm, V, López-Caniego, M, Lowe, S, Lubin, P, Macías-Pérez, J, Mactavish, C, Maffei, B, Maggio, G, Maino, D, Mandolesi, N, Mangilli, A, Marcos-Caballero, A, Marinucci, D, Maris, M, Marleau, F, Marshall, D, Martin, P, Martínez-González, E, Masi, S, Massardi, M, Matarrese, S, Matsumura, T, Matthai, F, Maurin, L, Mazzotta, P, Mcdonald, A, Mcewen, J, Mcgehee, P, Mei, S, Meinhold, P, Melchiorri, A, Melin, J, Mendes, L, Menegoni, E, Mennella, A, Migliaccio, M, Mikkelsen, K, Millea, M, Miniscalco, R, Mitra, S, Miville-Deschênes, M, Molinari, D, Moneti, A, Montier, L, Morgante, G, Morisset, N, Mortlock, D, Moss, A, Munshi, D, Murphy, J, Naselsky, P, Nati, F, Natoli, P, Negrello, M, Nesvadba, N, Netterfield, C, Nørgaard-Nielsen, H, North, C, Noviello, F, Novikov, D, Novikov, I, O’Dwyer, I, Orieux, F, Osborne, S, O’Sullivan, C, Oxborrow, C, Paci, F, Pagano, L, Pajot, F, Paladini, R, Pandolfi, S, Paoletti, D, Partridge, B, Pasian, F, Patanchon, G, Paykari, P, Pearson, D, Pearson, T, Peel, M, Peiris, H, Perdereau, O, Perotto, L, Perrotta, F, Pettorino, V, Piacentini, F, Piat, M, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Platania, P, Pogosyan, D, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, G, Prézeau, G, Prunet, S, Puget, J, Pullen, A, Rachen, J, Racine, B, Rahlin, A, Räth, C, Reach, W, Rebolo, R, Reinecke, M, Remazeilles, M, Renault, C, Renzi, A, Riazuelo, A, Ricciardi, S, Riller, T, Ringeval, C, Ristorcelli, I, Robbers, G, Rocha, G, Roman, M, Rosset, C, Rossetti, M, Roudier, G, Rowan-Robinson, M, Rubiño-Martín, J, Ruiz-Granados, B, Rusholme, B, Salerno, E, Sandri, M, Sanselme, L, Santos, D, Savelainen, M, Savini, G, Schaefer, B, Schiavon, F, Scott, D, Seiffert, M, Serra, P, Shellard, E, Smith, K, Smoot, G, Souradeep, T, Spencer, L, Starck, J, Stolyarov, V, Stompor, R, Sudiwala, R, Sunyaev, R, Sureau, F, Sutter, P, Sutton, D, Suur-Uski, A, Sygnet, J, Tauber, J, Tavagnacco, D, Taylor, D, Terenzi, L, Texier, D, Toffolatti, L, Tomasi, M, Torre, J, Tristram, M, Tucci, M, Tuovinen, J, Türler, M, Tuttlebee, M, Umana, G, Valenziano, L, Valiviita, J, Van Tent, B, Varis, J, Vibert, L, Viel, M, Vielva, P, Villa, F, Vittorio, N, Wade, L, Wandelt, B, Watson, C, Watson, R, Wehus, I, Welikala, N, Weller, J, White, M, White, S, Wilkinson, A, Winkel, B, Xia, J, Yvon, D, Zacchei, A, Zibin, J, Zonca, A, Department of Physics, and Helsinki Institute of Physics
Subjects: [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, Cosmic microwave background, cosmic microwave backgrounds, Astrophysics, cosmic background radiation, Surveys, CMB, power spectrum, Cosmic background radiation, 7. Clean energy, european space agency, Cosmology, atacama cosmology telescope, space vehicles: instruments, observations [Cosmology], sunyaev-zeldovich effects, detectors [Instrumentation], QB, pre-launch status, instrumentation, Physics, data release, [PHYS]Physics [physics], Instrumentation: detector, Astrophysics::Instrumentation and Methods for Astrophysics, probe wmap observations, microwave background maps, CMB cold spot, Computer Science::Computers and Society, damping tail, component separation, Physics::Space Physics, Physical Sciences, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, symbols, detector [Instrumentation], Baryon acoustic oscillations, Neutrino, hubble-space-telescope, galaxy cluster survey, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics and Astronomy, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmology: observations, Instrumentation: detectors, Space vehicles: instruments, Astronomy and Astrophysics, Space and Planetary Science, education, gravitational lensing, FOS: Physical sciences, observation [Cosmology], Astrophysics::Cosmology and Extragalactic Astrophysics, in-flight performance, Astronomy & Astrophysics, Space vehicles: instrument, Computer Science::Digital Libraries, NO, instruments [Space vehicles], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, instrument [Space vehicles], systematic uncertainties, Planck, Forschungsgruppe Komplexe Plasmen, extragalactic point sources, Science & Technology, cosmology: observation, instrumentation: detectors, Astronomy and Astrophysic, 115 Astronomy, Space science, Settore MAT/06 - Probabilita' e Statistica Matematica, Gravitational lens, [SDU]Sciences of the Universe [physics], cosmology: observations, space vehicles, south-pole telescope, cosmology, Hubble's law
Abstract: The European Space Agency’s Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5 months of Planck data, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the cosmic microwave background (CMB) and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the Sunyaev-Zeldovich effect. The likelihood code used to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter ΛCDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25σ. Planck finds no evidence for non-Gaussianity in the CMB. Planck’s results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluctuations (σ8) derived from CMB data and that derived from Sunyaev-Zeldovich data. The Planck and WMAP power spectra are offset from each other by an average level of about 2% around the first acoustic peak. Analysis of Planck polarization data is not yet mature, therefore polarization results are not released, although the robust detection of E-mode polarization around CMB hot and cold spots is shown graphically., Centre National D'etudes Spatiales, CNRS/INSU-IN2P3, Italian Space Agency (ASI), Danish Natural Science Research Council, European Space Agency, CNRS/INSU-IN2P3-INP (France), Italian National Research Council, Istituto Nazionale Astrofisica (INAF), National Aeronautics & Space Administration (NASA), United States Department of Energy (DOE), Science & Technology Facilities Council (STFC), UKSA (UK), Consejo Superior de Investigaciones Cientificas (CSIC), Spanish Government, JA (Spain), Finnish Funding Agency for Technology & Innovation (TEKES), AoF (Finland), CSC (Finland), Helmholtz Association, German Aerospace Centre (DLR), Max Planck Society, CSA (Canada), DTU Space (Denmark), SER/SSO (Switzerland), RCN (Norway), Science Foundation Ireland, Portuguese Foundation for Science and Technology, European Union (EU), Science & Technology Facilities Council (STFC) ST/I002006/1 ST/J000388/1 ST/H001239/1 ST/K000977/1 ST/K002805/1 ST/J001368/1 ST/K00333X/1 ST/I005129/1 ST/J005673/1 ST/K003674/1 ST/L000768/1 ST/G003874/1 ST/H008586/1 ST/L001314/1 ST/K004131/1 ST/M007685/1 ST/K000985/1 ST/K001051/1 ST/K00106X/1 ST/I005765/1 ST/K002899/1 ST/J004812/1
Published: 2014

46. Planck 2013 results. IV. Low Frequency Instrument beams and window functions

Author: B. Van Tent, A. J. Banday, Radek Stompor, P. Platania, Mika Juvela, M. Frailis, Carlo Baccigalupi, E. Hivon, C. Hernández-Monteagudo, Pasquale Mazzotta, J. Lesgourgues, J.-F. Sygnet, D. Tavagnacco, L. Mendes, Sabino Matarrese, Luca Valenziano, Rafael Rebolo, Michael P. Hobson, Torsten A. Enßlin, A. Curto, T. Poutanen, Alessandro Melchiorri, K. Ganga, J. Knoche, Simon Prunet, Ben Rusholme, D. Sutton, A. Moneti, Jose M. Diego, Jeffrey Jewell, Marian Douspis, P. Bielewicz, Olivier Forni, Guilaine Lagache, Jean-François Cardoso, F. Atrio-Barandela, S. Ricciardi, M. López-Caniego, R. B. Barreiro, L. Montier, A.-S. Suur-Uski, Jörg P. Rachen, F. K. Hansen, Adam Moss, Peter Meinhold, H. Dole, Subhabrata Mitra, J. A. Tauber, L. Perotto, W. C. Jones, K. Kiiveri, F. Matthai, J. González-Nuevo, J.-P. Bernard, Benjamin D. Wandelt, A. Benoit-Lévy, M. Reinecke, Michael Seiffert, M. Tomasi, Silvia Masi, Julian Borrill, F. Perrotta, Serge Gratton, J. Aumont, Sophie Henrot-Versille, J.-L. Puget, Duncan Hanson, Hannu Kurki-Suonio, M. Ashdown, H. K. Eriksen, M. Maris, Marco Bersanelli, Paolo Natoli, E. Martínez-González, L. P. L. Colombo, M. Bucher, Douglas Scott, M. Giard, B. P. Crill, Lung-Yih Chiang, Douglas J. Marshall, V. Stolyarov, Y. Giraud-Héraud, Dmitry Novikov, Daniel J. Mortlock, Davide Pietrobon, F. Cuttaia, E. Pierpaoli, Jean-Luc Starck, Stéphane Plaszczynski, L. A. Wade, F. Pasian, Krzysztof M. Gorski, Daniela Paoletti, Martin Kunz, James J. Bock, Clive Dickinson, Nicola Vittorio, Monique Arnaud, V. Lindholm, M. Tucci, P. R. Christensen, Mathieu Remazeilles, Luigi Danese, Dipak Munshi, François R. Bouchet, Calvin B. Netterfield, George Efstathiou, N. Mandolesi, Anna Bonaldi, J. F. Macías-Pérez, Lloyd Knox, W. Hovest, R. C. Butler, L. Pagano, P. de Bernardis, Andrew H. Jaffe, G. Umana, Todd Gaier, Graca Rocha, Hans Ulrik Nørgaard-Nielsen, C. Rosset, E. P. S. Shellard, Philip Lubin, G. Roudier, Luca Terenzi, E. Franceschi, A. de Rosa, Jérôme Bobin, Davide Maino, A. Chamballu, Jose Alberto Rubino-Martin, Allan Hornstrup, M. Bridges, M. Tristram, D. L. Harrison, Peter G. Martin, Locke D. Spencer, G. de Zotti, Anne Lähteenmäki, Alessandro Gruppuso, G. Polenta, P. Vielva, S. Galeotta, M. Linden-Vørnle, Sarah E. Church, S. Colombi, E. Battaner, Michele Liguori, Marcella Massardi, Etienne Pointecouteau, W. A. Holmes, J.-M. Lamarre, Olivier Doré, I. D. Novikov, Pekka Kangaslahti, I. J. O'Dwyer, G. Prézeau, P. B. Lilje, M. Sandri, L. Toffolatti, Jacques Delabrouille, René J. Laureijs, Fabio Finelli, Anthony Lasenby, E. Keihänen, Andrea Zonca, A. Gregorio, Alain Benoit, T. Riller, D. Santos, Reijo Keskitalo, Marc Türler, X. Dupac, S. R. Hildebrandt, Pavel Naselsky, R. J. Davis, L. Popa, Jussi Varis, O. Perdereau, Carlo Burigana, Charles R. Lawrence, Theodore Kisner, S. Osborne, J. P. Leahy, R. D. Davies, Andrea Zacchei, K. Benabed, Florent Sureau, J. R. Bond, R. Leonardi, Kevin M. Huffenberger, T. R. Jaffe, M. Migliaccio, Jussi-Pekka Väliviita, G. Patanchon, Fabrizio Villa, C. Armitage-Caplan, F. Paci, A. Mennella, Nabila Aghanim, G. W. Pratt, Gianluca Morgante, Nicolas Ponthieu, S. Donzelli, A. Catalano, D. Herranz, J. Tuovinen, B. Partridge, Anne Lähteenmäki Group, Department of Electronics and Nanoengineering, Aalto-yliopisto, Aalto University, Universidad de Cantabria, Hélium : du fondamental aux applications (NEEL - HELFA), Institut Néel (NEEL), 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), APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), 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)-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), 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), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS-PSL), 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)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, 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), PLANCK, Tauber, Jan, Aghanim, N., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J. J., Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bridges, M., Bucher, M., Burigana, C., Butler, R. C., Cardoso, J. F., Catalano, A., Chamballu, A., Chiang, L. Y., Christensen, P. R., Church, S., Colombi, S., Colombo, L. P. L., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T. C., Galeotta, S., Ganga, K., Giard, M., Giraud Héraud, Y., González Nuevo, J., Górski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D., Henrot Versillé, S., Hernández Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Jaffe, A. H., Jaffe, T. R., Jewell, J., Jones, W. C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T. S., Knoche, J., Knox, L., Kunz, M., Kurki Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J. M., Lasenby, A., Laureijs, R. J., Lawrence, C. R., Leahy, J. P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P. B., Linden Vørnle, M., Lindholm, V., López Caniego, M., Lubin, P. M., Maciás Pérez, J. F., Maino, D., Mandolesi, N., Maris, M., Marshall, D. J., Martin, P. G., Martínez González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C. B., Nørgaard Nielsen, H. U., Novikov, D., Novikov, I., O'Dwyer, I. J., Osborne, S., Paci, F., Pagano, L., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Roudier, G., Rubinõ Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M. D., Shellard, E. P. S., Spencer, L. D., Starck, J. L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur Uski, A. S., Sygnet, J. F., Tauber, J. A., Tavagnacco, Daniele, Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Zacchei, A., Zonca, A., Hélium : du fondamental aux applications (HELFA), 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 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), École normale supérieure - Paris (ENS 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), 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), Department of Physics, Helsinki Institute of Physics, 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), 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 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), 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, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI)
Subjects: POWER SPECTRUM, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astronomy, data analysis, Astrophysics, cosmic background radiation, Cosmic background radiation, Window function, MAPS, MICROWAVE, Anisotropy, Telescope, Physics, Astrophysics::Instrumentation and Methods for Astrophysics, Computer Science::Computers and Society, Physics::Space Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics and Astronomy, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Frequency band, education, FOS: Physical sciences, ERRORS, Low frequency, Computer Science::Digital Libraries, NO, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Optics, Settore FIS/05 - Astronomia e Astrofisica, Methods: data analysis, data analysis [methods], PRE-LAUNCH STATUS, Telescopes, Instrumentation and Methods for Astrophysics (astro-ph.IM), Radiometer, business.industry, Solid angle, Spectral density, Astronomy and Astrophysics, telescopes, Astronomy and Astrophysic, 115 Astronomy, Space science, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], data analysi [Methods], Space and Planetary Science, PROBE WMAP OBSERVATIONS, Physics::Accelerator Physics, business, Beam (structure)
Abstract: Planck (http://www.esa.int/Planck) is a project of the European Space Agency (ESA), Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J.J., Bonaldi, A., Bond, J.R., Borrill, J., Bouchet, F.R., Bridges, M., Bucher, M., Burigana, C., Butler, R.C., Cardoso, J.-F., Catalano, A., Chamballu, A., Chiang, L.-Y., Christensen, P.R., Church, S., Colombi, S., Colombo, L.P.L., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Dickinson, C., Diego, J.M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T.A., Eriksen, H.K., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Gaier, T.C., Galeotta, S., Ganga, K., Giard, M., Giraud-Héraud, Y., González-Nuevo, J., Górski, K.M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F.K., Hanson, D., Harrison, D., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Jaffe, A.H., Jaffe, T.R., Jewell, J., Jones, W.C., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T.S., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, A., Lamarre, J.-M., Lasenby, A., Laureijs, R.J., Lawrence, C.R., Leahy, J.P., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P.B., Linden-Vørnle, M., Lindholm, V., López-Caniego, M., Lubin, P.M., Maciás-Pérez, J.F., Maino, D., Mandolesi, N., Maris, M., Marshall, D.J., Martin, P.G., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Matthai, F., Mazzotta, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Naselsky, P., Natoli, P., Netterfield, C.B., Nørgaard-Nielsen, H.U., Novikov, D., Novikov, I., O'dwyer, I.J., Osborne, S., Paci, F., Pagano, L., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Platania, P., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G.W., Prézeau, G., Prunet, S., Puget, J.-L., Rachen, J.P., Rebolo, R., Reinecke, M., Remazeilles, M., Ricciardi, S., Riller, T., Rocha, G., Rosset, C., Roudier, G., Rubinõ-Martín, J.A., Rusholme, B., Sandri, M., Santos, D., Scott, D., Seiffert, M.D., Shellard, E.P.S., Spencer, L.D., Starck, J.-L., Stolyarov, V., Stompor, R., Sureau, F., Sutton, D., Suur-Uski, A.-S., Sygnet, J.-F., Tauber, J.A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L.A., Wandelt, B.D., Zacchei, A., Zonca, A.
Published: 2013

47. Planck early results. V. The Low Frequency Instrument data processing

Author: Poutanen, T., Lähteenmäki, A., León-Tavares, J., Natoli, P., Polenta, G., Falvella, M.C., Bartlett, J.G., Smoot, G.F., Stompor, R., Bonavera, L., Bedini, L., Salerno, E., Banday, A.J., Paladini, R., Prézeau, G., Rocha, G., Seiffert, M.D., Lilje, P.B., Nørgaard-Nielsen, Hans Ulrik, Toffolatti, L., Cruz, M., Moss, A., Scott, D., Colombo, L., Keihänen, E., Keskitalo, R., Kurki-Suonio, H., Suur-Uski, A.-S., Juvela, M., Savelainen, M., Knox, L., Meinhold, P.R., Zonca, A., Leonardi, R., Lubin, P.M., Silk, J.I., Bartolo, N., Matarrese, S., Melchiorri, A., Maino, D., Bersanelli, M., Mennella, A., Tomasi, M., Gregorio, A., Cabella, P., De Gasperis, G., De Troia, G., Migliaccio, M., Quercellini, C., Vittorio, N., Marinucci, D., Génova-Santos, R.T., Rebolo, R., Rubiño-Martín, J.A., Tauber, J.A., Bennett, K., Bremer, M., Giardino, G., Sternberg, J., Partridge, B., Tofani, G., Umana, G., Bonaldi, A., De Zotti, G., Massardi, M., Zacchei, A., Frailis, M., Galeotta, S., Maris, M., Pasian, F., Tavagnacco, D., Gasparo, F., Maggio, G., Vuerli, C., Burigana, C., Butler, R.C., Cuttaia, F., Mandolesi, N., Morgante, G., Ricciardi, S., Sandri, M., Terenzi, L., Villa, F., De Rosa, A., Finelli, F., Franceschi, E., Gruppuso, A., Paoletti, D., Procopio, P., Cappellini, B., Donzelli, S., Stivoli, F., Morisset, N., Rohlfs, R., Binko, P., Meharga, M.T., Türler, M., Chen, X., Huynh, M., Puget, J.-L., Bouchet, F.R., Efstathiou, G., Valiviita, J., Eriksen, H.K., Hansen, F.K., Gómez, F., López-Caniego, M., Barreiro, R.B., Curto, A., Diego, J.M., Herranz, D., Martínez-González, E., Vielva, P., Górski, K.M., Lawrence, C.R., Gaier, T.C., Jewell, J., Mitra, S., Pagano, L., Pearson, D., Pietrobon, D., Wade, L.A., Leahy, J.P., Davies, R.D., Davis, R.J., Dickinson, C., Watson, R., Wilkinson, A., Lamarre, J.-M., Borrill, J., Kisner, T.S., Knoche, J., Matthai, F., Reinecke, M., Dörl, U., Enßlin, T.A., Hell, R., Hovest, W., Rachen, J.P., Robbers, G., White, S.D.M., Tuovinen, J., Baccigalupi, C., Dick, J., González-Nuevo, J., Leach, S., Perrotta, F., Danese, L., Pettorino, V., 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), 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, PLANCK, Zacchei, A., Maino, D., Baccigalupi, C., Bersanelli, M., Bonaldi, A., Bonavera, L., Burigana, C., Butler, R. C., Cuttaia, F., de Zotti, G., Dick, J., Frailis, M., Galeotta, S., González Nuevo, J., Górski, K. M., Gregorio, Anna, Keihänen, E., Keskitalo, R., Knoche, J., Kurki Suonio, H., Lawrence, C. R., Leach, S., Leahy, J. P., López Caniego, M., Mandolesi, N., Maris, M., Matthai, F., Meinhold, P. R., Mennella, A., Morgante, G., Morisset, N., Natoli, P., Pasian, F., Perrotta, F., Polenta, G., Poutanen, T., Reinecke, M., Ricciardi, S., Rohlfs, R., Sandri, M., Suur Uski, A. S., Tauber, J. A., Tavagnacco, Daniele, Terenzi, L., Tomasi, M., Valiviita, J., Villa, F., Zonca, A., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., Bedini, L., Bennett, K., Binko, P., Borrill, J., Bouchet, F. R., Bremer, M., Cabella, P., Cappellini, B., Chen, X., Colombo, L., Cruz, M., Curto, A., Danese, L., Davies, R. D., Davis, R. J., de Gasperis, G., de Rosa, A., de Troia, G., Dickinson, C., Diego, J. M., Donzelli, S., Dörl, U., Efstathiou, G., Ensslin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Franceschi, E., Gaier, T. C., Gasparo, F., Génova Santos, R. T., Giardino, G., Gómez, F., Gruppuso, A., Hansen, F. K., Hell, R., Herranz, D., Hovest, W., Jewell, J., Juvela, M., Kisner, T. S., Knox, L., Lähteenmäki, A., Lamarre, J. M., Leonardi, R., León Tavares, J., Lilje, P. B., Lubin, P. M., Maggio, G., Marinucci, D., Martínez González, E., Massardi, M., Matarrese, S., Meharga, M. T., Melchiorri, A., Migliaccio, M., Mitra, S., Moss, A., Norgaard Nielsen, H. U., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pearson, D., Pettorino, V., Pietrobon, D., Prézeau, G., Procopio, P., Puget, J. L., Quercellini, C., Rachen, J. P., Rebolo, R., Robbers, G., Rocha, G., Rubino Martín, J. A., Salerno, E., Savelainen, M., Scott, D., Seiffert, M. D., Silk, J. I., Smoot, G. F., Sternberg, J., Stivoli, F., Stompor, R., Tofani, G., Tuovinen, J., Türler, M., Umana, G., Vielva, P., Vittorio, N., Vuerli, C., Wade, L. A., Watson, R., White, S. D. M., Wilkinson, A., Department of Physics, Helsinki Institute of Physics, 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)-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), 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)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Universidad de Cantabria, 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), 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, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI)
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], media_common.quotation_subject, data analysis, Cosmic microwave background, education, FOS: Physical sciences, Cosmic background radiation, 01 natural sciences, Cosmology, Methods, observations, Surveys, methods, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, surveys, Settore FIS/05 - Astronomia e Astrofisica, CMB physics, 0103 physical sciences, data analysis [methods], Calibration, Planck, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Remote sensing, media_common, Physics, 010308 nuclear & particles physics, Instrument Data, Planck ESA mission, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Covariance, 115 Astronomy, Space science, methods: data analysis, observations [cosmology], [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Cardinal point, Space and Planetary Science, Sky, cosmic backround radiation, cosmology: observations, cosmic background radiation, cosmology, symbols, Astrophysics - Instrumentation and Methods for Astrophysics, Noise (radio), Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: 19 páginas, 18 figuras, 3 tablas.-- et al., We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discuss the steps involved in reducing the data from telemetry packets to cleaned, calibrated, time-ordered data (TOD) and frequency maps. Data are continuously calibrated using the modulation of the temperature of the cosmic microwave background radiation induced by the motion of the spacecraft. Noise properties are estimated from TOD from which the sky signal has been removed using a generalized least square map-making algorithm. Measured 1/f noise knee-frequencies range from ~100 mHz at 30 GHz to a few tens of mHz at 70GHz. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices required to compute statistical uncertainties on LFI and Planck products are also produced. Main beams are estimated down to the ≈−10dB level using Jupiter transits, which are also used for geometrical calibration of the focal plane., This work was supported by the Academy of Finland grants 121703 and 121962.
Published: 2011

48. Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance

Author: Poutanen, T., Lähteenmäki, A., León-Tavares, J., Polenta, G., Natoli, P., Falvella, M.C., Bartlett, J.G., Smoot, G.F., Bonavera, L., Banday, A.J., Seiffert, M.D., Paladini, R., Prézeau, G., Rocha, G., Lilje, P.B., Hughes, N., Jukkala, P., Kilpia, V.-H., Sjoman, P., Nørgaard-Nielsen, Hans Ulrik, Toffolatti, L., Aja, B., Artal, E., Cruz, M., Moss, A., Scott, D., Colombo, L., Kurki-Suonio, H., Suur-Uski, A.-S., Juvela, M., Keihänen, E., Keskitalo, R., Savelainen, M., Knox, L., Meinhold, P.R., Zonca, A., Leonardi, R., Lubin, P.M., Bartolo, N., Matarrese, S., Melchiorri, A., Mennella, A., Maino, D., Tomasi, M., Franceschet, C., Gregorio, A., Cabella, P., De Gasperis, G., Migliaccio, M., Quercellini, C., Vittorio, N., Marinucci, D., Génova-Santos, R.T., Rebolo, R., Rubi No-Martín, J.A., Mendes, L., Foley, S., Watson, C., Bennett, K., Tauber, J.A., Partridge, B., Nesti, R., Tofani, G., Umana, G., Bonaldi, A., De Zotti, G., Massardi, M., Frailis, M., Galeotta, S., Maris, M., Tavagnacco, D., Zacchei, A., Pasian, F., Butler, R.C., Cuttaia, F., Mandolesi, N., Morgante, G., Sandri, M., Terenzi, L., Villa, F., Burigana, C., De Rosa, A., Finelli, F., Franceschi, E., Gruppuso, A., Malaspina, M., Paoletti, D., Procopio, P., Ricciardi, S., Stringhetti, L., Valenziano, L., Cappellini, B., Donzelli, S., Türler, M., Chen, X., Puget, J.-L., Bouchet, F.R., Efstathiou, G., Valiviita, J., Eriksen, H.K., Hansen, F.K., Gómez, F., Herreros, J.M., Hoyland, R.J., Curto, A., Martínez-González, E., Barreiro, R.B., Diego, J.M., Herranz, D., López-Caniego, M., Vielva, P., D'Arcangelo, O., Simonetto, A., Sozzi, C., Lawrence, C.R., Pearson, D., Gaier, T.C., Górski, K.M., Jewell, J., Kangaslahti, P., Mitra, S., Pagano, L., Pietrobon, D., Prina, M., Wade, L.A., Davis, R.J., Leahy, J.P., Lowe, S., Watson, R., Wilkinson, A., Davies, R.D., Dickinson, C., Roddis, N., Winder, F., Lamarre, J.-M., Borrill, J., Kisner, T.S., Enßlin, T.A., Knoche, J., Matthai, F., Rachen, J.P., Reinecke, M., Robbers, G., White, S.D.M., Tuovinen, J., Varis, J., Pospieszalski, M., Laaninen, M., Dick, J., Leach, S., Perrotta, F., Baccigalupi, C., Danese, L., González-Nuevo, J., Pettorino, V., George, D., Battaglia, P., Leutenegger, P., Miccolis, M., Silvestri, R., 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), PLANCK, Universidad de Cantabria, 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), 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)-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), Mennella, A., Bersanelli, M., Butler, R. C., Curto, A., Cuttaia, F., Davis, R. J., Dick, J., Frailis, M., Galeotta, S., Gregorio, Anna, Kurki Suonio, H., Lawrence, C. R., Leach, S., Leahy, J. P., Lowe, S., Maino, D., Mandolesi, N., Maris, M., Mart'inez González, E., Meinhold, P. R., Morgante, G., Pearson, D., Perrotta, F., Polenta, G., Poutanen, T., Sandri, M., Seiffert, M. D., Suur Uski, A. S., Tavagnacco, Daniele, Terenzi, L., Tomasi, M., Valiviita, J., Villa, F., Watson, R., Wilkinson, A., Zacchei, A., Zonca, A., Aja, B., Artal, E., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., Battaglia, P., Bennett, K., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F. R., Burigana, C., Cabella, P., Cappellini, B., Chen, X., Colombo, L., Cruz, M., Danese, L., D'Arcangelo, O., Davies, R. D., de Gasperis, G., de Rosa, A., de Zotti, G., Dickinson, C., Diego, J. M., Donzelli, S., Efstathiou, G., Ensslin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Foley, S., Franceschet, C., Franceschi, E., Gaier, T. C., Génova Santos, R. T., George, D., Gómez, F., González Nuevo, J., Górski, K. M., Gruppuso, A., Hansen, F. K., Herranz, D., Herreros, J. M., Hoyland, R. J., Hughes, N., Jewell, J., Jukkala, P., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kilpia, V. H., Kisner, T. S., Knoche, J., Knox, L., Laaninen, M., Lähteenmäki, A., Lamarre, J. M., Leonardi, R., León Tavares, J., Leutenegger, P., Lilje, P. B., López Caniego, M., Lubin, P. M., Malaspina, M., Marinucci, D., Massardi, M., Matarrese, S., Matthai, F., Melchiorri, A., Mendes, L., Miccolis, M., Migliaccio, M., Mitra, S., Moss, A., Natoli, P., Nesti, R., Norgaard Nielsen, H. U., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Pettorino, V., Pietrobon, D., Pospieszalski, M., Prézeau, G., Prina, M., Procopio, P., Puget, J. L., Quercellini, C., Rachen, J. P., Rebolo, R., Reinecke, M., Ricciardi, S., Robbers, G., Rocha, G., Roddis, N., Rubino Martín, J. A., Savelainen, M., Scott, D., Silvestri, R., Simonetto, A., Sjoman, P., Smoot, G. F., Sozzi, C., Stringhetti, L., Tauber, J. A., Tofani, G., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Varis, J., Vielva, P., Vittorio, N., Wade, L. A., Watson, C., White, S., Winder, F., Department of Physics, and Helsinki Institute of Physics
Subjects: [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], education, Cosmic background radiation, FOS: Physical sciences, Astrophysics, cosmic background radiation, Low frequency, Cosmic backround radiation, 7. Clean energy, 01 natural sciences, instruments [Space vehicles], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, CMB physics, 0103 physical sciences, Space vehicles: instruments, Instrumentation: detectors, Planck, cosmology: observations, space vehicles: instruments, instrumentation: detectors, observations [Cosmology], 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), detectors [Instrumentation], detectors, Physics, 010308 nuclear & particles physics, Planck ESA mission, Cosmology: observations, Astrophysics::Instrumentation and Methods for Astrophysics, 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], observations, Early results, Space and Planetary Science, symbols, space vehicles, Astrophysics - Instrumentation and Methods for Astrophysics, cosmology, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: 29 páginas, 31 figuras, 15 tablas.-- Planck Collaboration: et al., The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit operation is presented. We describe the main optical parameters and discuss photometric calibration, white noise sensitivity, and noise properties. A preliminary evaluation of the impact of the main systematic effects is presented. For each of the performance parameters, we outline the methods used to obtain them from the flight data and provide a comparison with pre-launch ground assessments, which are essentially confirmed in flight., The Consortia are led by the Principal Investigators: J.-L. Puget in France for HFI (funded principally by CNES and CNRS/INSU-IN2P3) and N. Mandolesi in Italy for LFI (funded principally via ASI). NASA’s US Planck Project, based at JPL and involving scientists at many US institutions, contributes significantly to the efforts of these two Consortia. In Finland, the Planck LFI 70 GHz work was supported by the Finnish Funding Agency for Technology and Innovation (Tekes). This work was also supported by the Academy of Finland, CSC, and DEISA (EU).
Published: 2011

49. Planckearly results. I. ThePlanckmission

Author: P. A. R. Ade[82], N. Aghanim[54], M. Arnaud[68], M. Ashdown[66-4], J. Aumont[54], C. Baccigalupi[80], M. Baker[37], A. Balbi[31], A. J. Banday[89-9-73], R. B. Barreiro[62], J. G. Bartlett[3-64], E. Battaner[91], K. Benabed[55], K. Bennett[38], A. Benoît[53], J.-P. Bernard[89-9], M. Bersanelli[28-46], R. Bhatia[5], J. J. Bock[64-10], A. Bonaldi[42], J. R. Bond[6], J. Borrill[72-84], F. R. Bouchet[55], T. Bradshaw[79], M. Bremer[38], M. Bucher[3], C. Burigana[45], R. C. Butler[45], P. Cabella[31], C. M. Cantalupo[72], B. Cappellini[46], J.-F. Cardoso[69-3-55], R. Carr[35], M. Casale[35], A. Catalano[3-67], L. Cayón[21], A. Challinor[59-66-12], A. Chamballu[51], J. Charra[54], R.-R. Chary[52], L.-Y. Chiang[58], C. Chiang[20], P. R. Christensen[76-32], D. L. Clements[51], S. Colombi[55], F. Couchot[71], A. Coulais[67], B. P. Crill[64-77], G. Crone[38], M. Crook[79], F. Cuttaia[45], L. Danese[80], O. D'Arcangelo[63], R. D. Davies[65], R. J. Davis[65], P. de Bernardis[27], J. de Bruin[37], G. de Gasperis[31], A. de Rosa[45], G. de Zotti[42-80], J. Delabrouille[3], J.-M. Delouis[55], F.-X. Désert[49], J. Dick[80], C. Dickinson[65], K. Dolag[73], H. Dole[54], S. Donzelli[46-60], O. Doré[64-10], U. Dörl[73], M. Douspis[54], X. Dupac[36], G. Efstathiou[59], T. A. Enßlin[73], H. K. Eriksen[60], F. Finelli[45], S. Foley[37], O. Forni[89-9], P. Fosalba[56], M. Frailis[44], E. Franceschi[45], M. Freschi[36], T. C. Gaier[64], S. Galeotta[44], J. Gallegos[36], B. Gandolfo[37], K. Ganga[3-52], M. Giard[89-9], G. Giardino[38], G. Gienger[37], Y. Giraud-Héraud[3], J. González[35], J. González-Nuevo[80], K. M. Górski[64, 93], S. Gratton[66, 59], A. Gregorio[29], A. Gruppuso[45], G. Guyot[48], J. Haissinski[71], F. K. Hansen[60], D. Harrison[59-66], G. Helou[10], S. Henrot-Versillé[71], C. Hernández-Monteagudo[73], D. Herranz[62], S. R. Hildebrandt[10-70-61], E. Hivon[55], M. Hobson[4], W. A. Holmes[64], A. Hornstrup[14], W. Hovest[73], R. J. Hoyland[61], K. M. Huffenberger[92], A. H. Jaffe[51], T. Jagemann[36], W. C. Jones[20], J. J. Juillet[87], M. Juvela[19], P. Kangaslahti[64], E. Keihänen[19], R. Keskitalo[64-19], T. S. Kisner[72], R. Kneissl[34-5], L. Knox[23], M. Krassenburg[38], H. Kurki-Suonio[19-40], G. Lagache[54], A. Lähteenmäki[1-40], J.-M. Lamarre[67], A. E. Lange[52], A. Lasenby[4-66], R. J. Laureijs[38], C. R. Lawrence[64], S. Leach[80], J. P. Leahy[65], R. Leonardi[36-38-24], C. Leroy[54-89-9], P. B. Lilje[60-11], M. Linden-Vørnle[14], M. López-Caniego[62], S. Lowe[65], P. M. Lubin[24], J. F. Macías-Pérez[70], T. Maciaszek[7], C. J. MacTavish[66], B. Maffei[65], D. Maino[28-46], N. Mandolesi[45], R. Mann[81], M. Maris[44], E. Martínez-González[62], S. Masi[27], M. Massardi[42], S. Matarrese[26], F. Matthai[73], P. Mazzotta[31], A. McDonald[37], P. McGehee[52], P. R. Meinhold[24], A. Melchiorri[27], J.-B. Melin[13], L. Mendes[36], A. Mennella[28-44], C. Mevi[37], R. Miniscalco[37], S. Mitra[64], M.-A. Miville-Deschênes[54-6], A. Moneti[55], L. Montier[89-9], G. Morgante[45], N. Morisset[50], D. Mortlock[51], D. Munshi[82-59], A. Murphy[75], P. Naselsky[76-32], P. Natoli[30-2-45], C. B. Netterfield[16], H. U. Nørgaard-Nielsen[14], F. Noviello[54], D. Novikov[51], I. Novikov[76], I. J. O'Dwyer[64], I. Ortiz[35], S. Osborne[86], P. Osuna[35], C. A. Oxborrow[14], F. Pajot[54], R. Paladini[85, 10], B. Partridge[39], F. Pasian[44], T. Passvogel[38], G. Patanchon[3], D. Pearson[64], T. J. Pearson[10-52], O. Perdereau[71], L. Perotto[70], F. Perrotta[80], F. Piacentini[27], M. Piat[3], E. Pierpaoli[18], S. Plaszczynski[71], P. Platania[63], E. Pointecouteau[89-9], G. Polenta[2-43], N. Ponthieu[54], L. Popa[57], T. Poutanen[40-19-1], G. Prézeau[10-64], S. Prunet[55], J.-L. Puget[54], J. P. Rachen[73], W. T. Reach[90], R. Rebolo[61-33], M. Reinecke[73], J.-M. Reix[87], C. Renault[70], S. Ricciardi[45], T. Riller[73], I. Ristorcelli[89-9], G. Rocha[64-10], C. Rosset[3], M. Rowan-Robinson[51], J. A. Rubiño-Martín[61-33], B. Rusholme[52], E. Salerno[8], M. Sandri[45], D. Santos[70], G. Savini[78], B. M. Schaefer[88], D. Scott[17], M. D. Seiffert[64], P. Shellard[12], A. Simonetto[63], G. F. Smoot[22-72-3], C. Sozzi[63], J.-L. Starck[68-13], J. Sternberg[38], F. Stivoli[47], V. Stolyarov[4], R. Stompor[3], L. Stringhetti[45], R. Sudiwala[82], R. Sunyaev[73-83], J.-F. Sygnet[55], D. Tapiador[35], J. A. Tauber[38], D. Tavagnacco[44], D. Taylor[35], L. Terenzi[45], D. Texier[35], L. Toffolatti[15], M. Tomasi[28-46], J.-P. Torre[54], M. Tristram[71], J. Tuovinen[74], M. Türler[50], M. Tuttlebee[37], G. Umana[41], L. Valenziano[45], J. Valiviita[60], J. Varis[74], L. Vibert[54], P. Vielva[62], F. Villa[45], N. Vittorio[31], L. A. Wade[64], B. D. Wandelt[55-25], C. Watson[37], S. D. M. White[73], M. White[22], A. Wilkinson[65], D. Yvon[13], A. Zacchei[44], A. Zonca[24], Plank Collaboration, 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)-Centre National d’Études Spatiales [Paris] (CNES), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), 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)-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), 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), Hélium : du fondamental aux applications (NEEL - HELFA), Institut Néel (NEEL), 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), 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-PSL), 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), 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), 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)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, 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), Centre National d'Études Spatiales [Toulouse] (CNES), Département de Physique des Particules (ex SPP) (DPhP), 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, Laboratoire de Recherche en Informatique (LRI), Université Paris-Sud - Paris 11 (UP11)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS), PLANCK, 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., Désert, F. X., Dick, J., Dickinson, C., Dolag, K., Dole, H., Donzelli, S., Doré, O., Dörl, 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., Giraud Héraud, Y., González, J., González Nuevo, J., Górski, K. M., Gratton, S., Gregorio, Anna, Gruppuso, A., Guyot, G., Haissinski, J., Hansen, F. K., Harrison, D., Helou, G., Henrot Versillé, 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., Macías Pérez, J. F., Maciaszek, T., Mactavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Mann, R., Maris, M., Martínez 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 Deschênes, 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., Prézeau, 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., Rubiño Martín, 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, Daniele, Taylor, D., Terenzi, L., Texier, D., Toffolatti, L., Tomasi, M., Torre, J. P., Tristram, M., Tuovinen, J., Türler, 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., Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), 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), 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), 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), 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), 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), Département de Physique des Particules (ex SPP) (DPP), 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), 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), 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), 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), 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 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), CentraleSupélec-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Department of Physics, and Helsinki Institute of Physics
Subjects: Experimental Physics, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Computer science, Surveys, Cosmic background radiation, 7. Clean energy, 01 natural sciences, CMB physics, Space vehicles: instruments, Instrumentation: detectors, observations [Cosmology], Instrumentation, 010303 astronomy & astrophysics, detectors [Instrumentation], QB, detectors, media_common, Planck ESA mission, Conjunction (astronomy), Cosmology: observations, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmology, observations, Early results, cosmic backround radiation, instruments, symbols, [SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA], cosmology: observations, cosmic background radiation, surveys, space vehicles: instruments, instrumentation: detectors, catalogs, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, space vehicles, cosmology, instrumentation, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], media_common.quotation_subject, education, FOS: Physical sciences, Catalogs, Space vehicles, instruments [Space vehicles], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Planck, Early release, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010308 nuclear & particles physics, Payload, Astronomy, Astronomy and Astrophysics, 115 Astronomy, Space science, Catalogues, Astrophysics - Astrophysics of Galaxies, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA], Space and Planetary Science, Sky, Astrophysics of Galaxies (astro-ph.GA), Satellite
Abstract: 16 páginas, 14 figuras, 3 tablas.-- Planck Collaboration: et al., 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., 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

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49 results on '"Gaier, T. C."'

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