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208. Planck intermediate results

Author

Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Benabed, K., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Burigana, C., Calabrese, E., Cardoso, J. F., Challinor, A., Chiang, H. C., Colombo, L. P.L., Combet, C., Crill, B. P., Curto, A., Cuttaia, F., De Bernardis, P., De Rosa, A., De Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Diego, J. M., Doré, O., Ducout, A., Dupac, X., Dusini, S., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Fantaye, Y., Finelli, F., Forastieri, F., Frailis, M., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Génova-Santos, R. T., Gerbino, M., González-Nuevo, J., Górski, K. M., Gratton, S., Gruppuso, A., Gudmundsson, J. E., Herranz, D., Hivon, E., Huang, Z., Jaffe, A. H., Jones, W. C., Keihänen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Knox, L., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Le Jeune, M., Levrier, F., Lewis, A., Liguori, M., Lilje, P. B., Lilley, M., Lindholm, V., López-Caniego, M., Lubin, P. M., Ma, Y. Z., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P. G., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J. D., Meinhold, P. R., Mennella, A., Migliaccio, M., Millea, M., Miville-Deschênes, M. A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Moss, A., Narimani, A., Natoli, P., Oxborrow, C. A., Pagano, L., Paoletti, D., Partridge, B., Patanchon, G., Patrizii, L., Pettorino, V., Piacentini, F., Polastri, L., Polenta, G., Puget, J. L., Rachen, J. P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Sirignano, C., Sirri, G., Stanco, L., Suur-Uski, A. S., Tauber, J. A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Valiviita, J., Van Tent, F., Vielva, P., Villa, F., Vittorio, N., Wandelt, B. D., Wehus, I. K., White, Martin J., Zacchei, A., Zonca, A., Red Española de Supercomputación, Center for Science (Finland), Academy of Finland, German Research Foundation, Federal Ministry of Education and Research (Germany), Canadian Space Agency, DTU Space (Denmark), Swiss Space Office, Research Council of Norway, Science Foundation Ireland, Ministério da Ciência, Tecnologia e Ensino Superior (Portugal), Fundação para a Ciência e a Tecnologia (Portugal), European Research Council, European Commission, Ministerio de Economía, Industria y Competitividad (España), Consejo Superior de Investigaciones Científicas (España), Department of Energy (US), National Aeronautics and Space Administration (US), Consiglio Nazionale delle Ricerche, Istituto Nazionale di Astrofisica, Agenzia Spaziale Italiana, Centre National D'Etudes Spatiales (France), Centre National de la Recherche Scientifique (France), European Space Agency, Science and Technology Facilities Council (UK), Université Paris-Sud, Leiden University, University of Cambridge, International School for Advanced Studies, University of Bologna, CNRS, CSIC, University of Padova, Indian Institute of Science Education and Research Thiruvananthapuram, University of Milan, University of Manchester, University of Oviedo, University of Toronto, Lawrence Berkeley National Laboratory, University of Ferrara, Cardiff University, Observatoire de Paris, University of KwaZulu-Natal, University of Southern California, Université Grenoble Alpes, California Institute of Technology, Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna, Sapienza University of Rome, Astronomical Observatory of Padua, Imperial College London, European Space Astronomy Centre, National Institute for Nuclear Physics, Max Planck Institute for Astrophysics, University of Oslo, African Institute for Mathematical Sciences, Osservatorio Astronomico di Trieste, Simon Fraser University, University of Chicago, University of La Laguna, Jet Propulsion Laboratory, Princeton University, Sun Yat-Sen University, University of Helsinki, University of California Davis, University of Sussex, University of California Santa Barbara, Jodrell Bank Centre for Astrophysics, University College London, Italian Space Agency, University of Nottingham, University of British Columbia, Technical University of Denmark, Haverford College, Heidelberg University, Radboud University Nijmegen, University of Granada, Topological Quantum Fluids, ESTEC, University of Trieste, University of Rome Tor Vergata, University of Illinois at Urbana-Champaign, University of Adelaide, University of California San Diego, Department of Applied Physics, Aalto-yliopisto, and Aalto University

Subjects
theory [Cosmology], Cosmological parameters, Cosmology: observations, observations [Cosmology], Submillimeter: ISM, Cosmic background radiation, Dust, extinction
Abstract

Planck Collaboration., The characterization of the Galactic foregrounds has been shown to be the main obstacle in thechallenging quest to detect primordial B-modes in the polarized microwave sky. We make use of the Planck-HFI 2015 data release at high frequencies to place new constraints on the properties of the polarized thermal dust emission at high Galactic latitudes. Here, we specifically study the spatial variability of the dust polarized spectral energy distribution (SED), and its potential impact on the determination of the tensor-to-scalar ratio, r. We use the correlation ratio of the angular power spectra between the 217 and 353 GHz channels as a tracer of these potential variations, computed on different high Galactic latitude regions, ranging from 80% to 20% of the sky. The new insight from Planck data is a departure of the correlation ratio from unity that cannot be attributed to a spurious decorrelation due to the cosmic microwave background, instrumental noise, or instrumental systematics. The effect is marginally detected on each region, but the statistical combination of all the regions gives more than 99% confidence for this variation in polarized dust properties. In addition, we show that the decorrelation increases when there is a decrease in the mean column density of the region of the sky being considered, and we propose a simple power-law empirical model for this dependence, which matches what is seen in the Planck data. We explore the effect that this measured decorrelation has on simulations of the BICEP2-Keck Array/Planck analysis and show that the 2015 constraints from these data still allow a decorrelation between the dust at 150 and 353 GHz that is compatible with our measured value. Finally, using simplified models, we show that either spatial variation of the dust SED or of the dust polarization angle are able to produce decorrelations between 217 and 353 GHz data similar to the values we observe in the data., 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, MINECO, J.A., and RES (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); ERC and PRACE (EU). The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP7/2007-2013) / ERC grant agreement No. 267934.

Published
2017

211. An urban political ecology approach to local development in fast-growing, tourism-specialized coastal cities

Author

Ridolfi, E., Pujol, D. S., Ippolito, A., Saradakou, E., and Salvati, L.

Subjects
Benidorm, Southern Europe, Settore SECS-S/03 - Statistica Economica, Local development, Urban growth, Mykonos, Venice
Abstract

Cities everywhere, and especially those located in coastal areas, grow and change rapidly, reconfiguring in many cases through successful urban development strategies. Tourism specialization is considered a driver of urban transformation and environmental change. A key challenge facing cities for years to come will be understanding the critical role that tourism plays in urban policies and planning process. Our study focuses on Urban Political Ecology (UPE) as an emerging framework for analysis of socio-environmental change in metropolitan areas. Specifically, it allows to examine political, social, and ecological processes together with interests, power and relations shaping patterns and processes of urban change. After providing a brief review of UPE and how it expands toward tourism issues, the article examines Benidorm (Spain), Venice (Italy) and Mykonos (Greece) as representative examples of fast-growing, tourismspecialized Mediterranean urban areas. The case studies illustrate how tourism specialization has been for a long time a driver of change closely linked to urban processes. We conclude that UPE allows a comprehensive analysis of tourism's role, problems and potentials in the context of complex socioeconomic dynamics, contributing to identify effective policies governing future urbanization processes in coastal cities., tourismos, Vol. 12 No. 1 (2017)

Published
2017

212. Recession and value of new dwellings : changes in the spatial structure of Greece, 2003-2015

Author

Zitti, M and Salvati, L

Subjects
Economic development -- Greece -- History -- 21st century, Southern Europe, Spatial behaviour -- Greece, Settore SECS-S/03 - Statistica Economica, Spatial approaches, Economic growth, Housing market, Housing -- Greece -- History -- 21st century
Abstract

Recent economic dynamics in southern Europe have been influenced by multifaceted processes with important spatial outcomes. Construction industry has been one of the productive sectors with the most relevant crisis-driven changes in Greece, probably the most affected country in Europe. With the aim to provide a quantitative analysis offering a comprehensive knowledge of regional-scale dynamics in construction industry during expansion and recession times, the present study investigates spatial variations over 2003-2015 in the value of new dwellings, supplemented with other indicators of building activity (number of permits, average building surface, number of floors), at the scale of Greek prefectures. A data mining framework based on principal component analysis and non-parametric correlations with background socioeconomic indicators was developed to identify spatial patterns in building activity during economic expansion (2003-2009) and crisis (2009-2015). According to building permit data, the average value of new dwellings' per surface area increased in a spatially-heterogeneous fashion across the country, with a substantial difference in growth rates between the two investigated time intervals. During expansion, new dwellings' value increased across the country with a slight decline in two regions and a considerable growth in one region. During recession, new dwellings' value decreased in one region and increased markedly in four regions, being relatively stable in the rest of the country. In 2003, the highest values of new dwellings were spatially associated with economically-dynamic districts characterized by agglomeration economies, upper urban functions, and transport accessibility. With crisis, the spatial distribution of dwellings' value was more heterogeneous and not associated to specific background factors, with the highest increase observed in accessible rural districts and coastal areas with tourism specialization. Further investigation on the role of economic cycles in house value spatial trends is particularly required for designing effective post-crisis development measures., peer-reviewed

Published
2017

218. L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysis

Author

Aghanim, N., Ashdown, Mark, Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. Belén, Bartolo, Nicola, Basak, S., Benabed, K., Bernard, J. P., Keihänen, E., Falgarone, E., Fantaye, Y., Finelli, F., Frailis, M., Fraisse, A. A., Mauri, N., Franceschi, E., Frolov, A., Galeotta, S., Rossetti, M., Galli, S., Keskitalo, R., Ganga, K., Génova-Santos, R., Gerbino, M., Ghosh, T., Giard, M., González-Nuevo, J., McEwen, J. D., Górski, K. M., Mitra, S., Gregorio, A., Gruppuso, A., Kisner, T. S., Gudmundsson, J.E., Hansen, F. K., Helou, G., Herranz, D., Hivon, E., Huang, Z., Jaffe, A. H., Miville-Deschênes, M. A., Krachmalnicof, N., Kunz, M., Kurki-Suonio, H., Lagache, Guilaine, Lähteenmäki, Anne, Bonaldi, A., Lamarre, J.-M., Mennella, A., Lasenby, Anthony N., Lattanzi, M., Molinari, D., Lawrence, C. R., Jeune, M. le, Levrier, F., Liguori, Michele, Lilje, P. B., López-Caniego, M., Rocha, G., Lubin, P. M., Macías-Pérez, J. F., Migliaccio, M., Moneti, A., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martínez-González, Enrique, Matarrese, S., Montier, L., Bersanelli, M., Morgante, G., Moss, A., Naselsky, P., Elsner, F., Nørgaard-Nielsen, H. U., Roudier, G., Oxborrow, C. A., Pagano, L., Paoletti, D., Partridge, B., Patrizii, L., Perdereau, O., Bielewicz, P., Perotto, L., Borrill, J., Pettorino, V., Piacentini, F., Rubiño-Martín, J. A., Plaszczynski, S., Polenta, G., Puget, J.-L., Rachen, J. P., Reinecke, M., Remazeilles, Mathieu, Renzi, A., Bouchet, F. R., Ruiz-Granados, Beatriz, Salvati, L., Sandri, M., Savelainen, M., Scott, D., Dusini, S., Sirignano, C., Bonavera, Laura, Sirri, G., Stanco, L., Boulanger, F., Suur-Uski, A.-S., Tauber, J. A., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Efstathiou, G., Trombetti, T., Valiviita, J., Bond, J. R., Bracco, Andrea, Vansyngel, F., Tent, F. van, Vielva, P., Wandelt, B. D., Wehus, I. K., Zacchei, A., Zonca, A., Burigana, C., Calabrese, E., Cardoso, J. F., Chiang, H. C., Colombo, L.P.L., Melchiorri, A., Combet, C., Enßlin, T. A., Comis, B., Crill, B. P., Curto, Andrés, Cuttaia, F., Davis, R. J., Bernardis, P. de, Rosa, A. de, Zotti, G. de, Jones, W. C., Delabrouille, J., Delouis, J. M., Eriksen, H. K., Valentino, E. di, Dickinson, C., Diego, José María, Doré, O., Douspis, M., Ducout, A., Dupac, X., Red Española de Supercomputación, Center for Science (Finland), Academy of Finland, German Research Foundation, Federal Ministry of Education and Research (Germany), Canadian Space Agency, DTU Space (Denmark), Swiss Space Office, Research Council of Norway, Science Foundation Ireland, Ministério da Ciência, Tecnologia e Ensino Superior (Portugal), Fundação para a Ciência e a Tecnologia (Portugal), European Research Council, European Commission, Ministerio de Economía, Industria y Competitividad (España), Consejo Superior de Investigaciones Científicas (España), Department of Energy (US), National Aeronautics and Space Administration (US), Consiglio Nazionale delle Ricerche, Istituto Nazionale di Astrofisica, Agenzia Spaziale Italiana, Centre National D'Etudes Spatiales (France), Centre National de la Recherche Scientifique (France), European Space Agency, and Science and Technology Facilities Council (UK)

Subjects
ISM [Submillimeter], Astrophysics::Cosmology and Extragalactic Astrophysics, observations [Cosmology], Cosmic background radiation, Astrophysics::Galaxy Astrophysics, Dust, extinction
Abstract

Planck Collaboration. The characterization of the Galactic foregrounds has been shown to be the main obstacle in thechallenging quest to detect primordial B-modes in the polarized microwave sky. We make use of the Planck-HFI 2015 data release at high frequencies to place new constraints on the properties of the polarized thermal dust emission at high Galactic latitudes. Here, we specifically study the spatial variability of the dust polarized spectral energy distribution (SED), and its potential impact on the determination of the tensor-to-scalar ratio, r. We use the correlation ratio of the angular power spectra between the 217 and 353 GHz channels as a tracer of these potential variations, computed on different high Galactic latitude regions, ranging from 80% to 20% of the sky. The new insight from Planck data is a departure of the correlation ratio from unity that cannot be attributed to a spurious decorrelation due to the cosmic microwave background, instrumental noise, or instrumental systematics. The effect is marginally detected on each region, but the statistical combination of all the regions gives more than 99% confidence for this variation in polarized dust properties. In addition, we show that the decorrelation increases when there is a decrease in the mean column density of the region of the sky being considered, and we propose a simple power-law empirical model for this dependence, which matches what is seen in the Planck data. We explore the effect that this measured decorrelation has on simulations of the BICEP2-Keck Array/Planck analysis and show that the 2015 constraints from these data still allow a decorrelation between the dust at 150 and 353 GHz that is compatible with our measured value. Finally, using simplified models, we show that either spatial variation of the dust SED or of the dust polarization angle are able to produce decorrelations between 217 and 353 GHz data similar to the values we observe in the data. 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, MINECO, J.A., and RES (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); ERC and PRACE (EU). The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP7/2007-2013) / ERC grant agreement No. 267934.

Published
2017

232. Une cause rare d'infarctus du myocarde sans sus-décalage du segment ST de type 2 : compression cardiaque et obstruction intraventriculaire gauche par une volumineuse hernie hiatale.

Author

Salvati, L., Atesler, S., and Valla, M.

Abstract

Nous rapportons le cas d'une patiente de 89 ans adressée aux urgences pour épigastralgies et vomissements. Une dégradation hémodynamique, associée à des modifications du segment ST et une troponinémie légèrement augmentée, incitait à réaliser une coronarographie en urgence qui s'avérait normale. Le scanner thoraco-abdominal retrouvait une volumineuse hernie hiatale responsable d'une compression cardiaque avec obstruction intraventriculaire gauche objectivée en doppler cardiaque. L'ensemble des symptômes ainsi que les anomalies électrocardiographiques et échocardiographiques ont régressé après aspiration nasogastrique. We report the case of a 89 year-old woman admitted to the emergency department for epigastric pain, nausea, vomiting. Because of a circulatory failure with electrocardiographic ST changes and a slight elevation of ultra-sensible troponin, a coronary angiography was performed and found normal coronary arteries. Thoraco-abdominal CT scan revealed a large hiatal hernia causing a cardiac compression, and a left intraventricular obstruction showed by Doppler echocardiography. All signs resolved after fasting and gastric drainage. [ABSTRACT FROM AUTHOR]

Published
2020
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235. Exploring cosmic origins with CORE: Cluster science

Author

Melin, J.-B., primary, Bonaldi, A., additional, Remazeilles, M., additional, Hagstotz, S., additional, Diego, J.M., additional, Hernández-Monteagudo, C., additional, Génova-Santos, R.T., additional, Luzzi, G., additional, Martins, C.J.A.P., additional, Grandis, S., additional, Mohr, J.J., additional, Bartlett, J.G., additional, Delabrouille, J., additional, Ferraro, S., additional, Tramonte, D., additional, Rubiño-Martín, J.A., additional, Macìas-Pérez, J.F., additional, Achúcarro, A., additional, Ade, P., additional, Allison, R., additional, Ashdown, M., additional, Ballardini, M., additional, Banday, A. J., additional, Banerji, R., additional, Bartolo, N., additional, Basak, S., additional, Basu, K., additional, Battye, R. A., additional, Baumann, D., additional, Bersanelli, M., additional, Bonato, M., additional, Borrill, J., additional, Bouchet, F., additional, Boulanger, F., additional, Brinckmann, T., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Cai, Z.-Y., additional, Calvo, M., additional, Carvalho, C. S., additional, Castellano, M. G., additional, Challinor, A., additional, Chluba, J., additional, Clesse, S., additional, Colafrancesco, S., additional, Colantoni, I., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, de Bernardis, P., additional, de Gasperis, G., additional, Petris, M. De, additional, Zotti, G. De, additional, Valentino, E. Di, additional, Errard, J., additional, Feeney, S. M., additional, Fernández-Cobos, R., additional, Finelli, F., additional, Forastieri, F., additional, Galli, S., additional, Gerbino, M., additional, González-Nuevo, J., additional, Greenslade, J., additional, Hanany, S., additional, Handley, W., additional, Hervias-Caimapo, C., additional, Hills, M., additional, Hivon, E., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lamagna, L., additional, Lasenby, A., additional, Lattanzi, M., additional, Brun, A. M. C. Le, additional, Lesgourgues, J., additional, Lewis, A., additional, Liguori, M., additional, Lindholm, V., additional, Lopez-Caniego, M., additional, Maffei, B., additional, Martinez-Gonzalez, E., additional, Masi, S., additional, Mazzotta, P., additional, McCarthy, D., additional, Melchiorri, A., additional, Molinari, D., additional, Monfardini, A., additional, Natoli, P., additional, Negrello, M., additional, Notari, A., additional, Paiella, A., additional, Paoletti, D., additional, Patanchon, G., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Roman, M., additional, Salvati, L., additional, Tartari, A., additional, Tomasi, M., additional, Trappe, N., additional, Triqueneaux, S., additional, Trombetti, T., additional, Tucker, C., additional, Väliviita, J., additional, de Weygaert, R. van, additional, Tent, B. Van, additional, Vennin, V., additional, Vielva, P., additional, Vittorio, N., additional, Weller, J., additional, Young, K., additional, and Zannoni, M., additional

Published
2018
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236. Exploring cosmic origins with CORE: Inflation

Author

Finelli, F., primary, Bucher, M., additional, Achúcarro, A., additional, Ballardini, M., additional, Bartolo, N., additional, Baumann, D., additional, Clesse, S., additional, Errard, J., additional, Handley, W., additional, Hindmarsh, M., additional, Kiiveri, K., additional, Kunz, M., additional, Lasenby, A., additional, Liguori, M., additional, Paoletti, D., additional, Ringeval, C., additional, Väliviita, J., additional, Tent, B. van, additional, Vennin, V., additional, Ade, P., additional, Allison, R., additional, Arroja, F., additional, Ashdown, M., additional, Banday, A.J., additional, Banerji, R., additional, Bartlett, J.G., additional, Basak, S., additional, de Bernardis, P., additional, Bersanelli, M., additional, Bonaldi, A., additional, Borril, J., additional, Bouchet, F.R., additional, Boulanger, F., additional, Brinckmann, T., additional, Burigana, C., additional, Buzzelli, A., additional, Cai, Z.-Y., additional, Calvo, M., additional, Carvalho, C.S., additional, Castellano, G., additional, Challinor, A., additional, Chluba, J., additional, Colantoni, I., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, D'Amico, G., additional, Delabrouille, J., additional, Desjacques, V., additional, Zotti, G. De, additional, Diego, J.M., additional, Valentino, E. Di, additional, Feeney, S., additional, Fergusson, J.R., additional, Fernandez-Cobos, R., additional, Ferraro, S., additional, Forastieri, F., additional, Galli, S., additional, García-Bellido, J., additional, de Gasperis, G., additional, Génova-Santos, R.T., additional, Gerbino, M., additional, González-Nuevo, J., additional, Grandis, S., additional, Greenslade, J., additional, Hagstotz, S., additional, Hanany, S., additional, Hazra, D.K., additional, Hernández-Monteagudo, C., additional, Hervias-Caimapo, C., additional, Hills, M., additional, Hivon, E., additional, Hu, B., additional, Kisner, T., additional, Kitching, T., additional, Kovetz, E.D., additional, Kurki-Suonio, H., additional, Lamagna, L., additional, Lattanzi, M., additional, Lesgourgues, J., additional, Lewis, A., additional, Lindholm, V., additional, Lizarraga, J., additional, López-Caniego, M., additional, Luzzi, G., additional, Maffei, B., additional, Mandolesi, N., additional, Martínez-González, E., additional, Martins, C.J.A.P., additional, Masi, S., additional, McCarthy, D., additional, Matarrese, S., additional, Melchiorri, A., additional, Melin, J.-B., additional, Molinari, D., additional, Monfardini, A., additional, Natoli, P., additional, Negrello, M., additional, Notari, A., additional, Oppizzi, F., additional, Paiella, A., additional, Pajer, E., additional, Patanchon, G., additional, Patil, S.P., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Ravenni, A., additional, Remazeilles, M., additional, Renzi, A., additional, Roest, D., additional, Roman, M., additional, Rubiño-Martin, J.A., additional, Salvati, L., additional, Starobinsky, A.A., additional, Tartari, A., additional, Tasinato, G., additional, Tomasi, M., additional, Torrado, J., additional, Trappe, N., additional, Trombetti, T., additional, Tucci, M., additional, Tucker, C., additional, Urrestilla, J., additional, de Weygaert, R. van, additional, Vielva, P., additional, Vittorio, N., additional, Young, K., additional, and Zannoni, M., additional

Published
2018
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237. Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps

Author

Zotti, G. De, primary, González-Nuevo, J., additional, Lopez-Caniego, M., additional, Negrello, M., additional, Greenslade, J., additional, Hernández-Monteagudo, C., additional, Delabrouille, J., additional, Cai, Z.-Y., additional, Bonato, M., additional, Achúcarro, A., additional, Ade, P., additional, Allison, R., additional, Ashdown, M., additional, Ballardini, M., additional, Banday, A.J., additional, Banerji, R., additional, Bartlett, J.G., additional, Bartolo, N., additional, Basak, S., additional, Bersanelli, M., additional, Biesiada, M., additional, Bilicki, M., additional, Bonaldi, A., additional, Bonavera, L., additional, Borrill, J., additional, Bouchet, F., additional, Boulanger, F., additional, Brinckmann, T., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Calvo, M., additional, Carvalho, C.S., additional, Castellano, M.G., additional, Challinor, A., additional, Chluba, J., additional, Clements, D.L., additional, Clesse, S., additional, Colafrancesco, S., additional, Colantoni, I., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, de Bernardis, P., additional, de Gasperis, G., additional, Diego, J.M., additional, Valentino, E. Di, additional, Errard, J., additional, Feeney, S.M., additional, Fernández-Cobos, R., additional, Ferraro, S., additional, Finelli, F., additional, Forastieri, F., additional, Galli, S., additional, Génova-Santos, R.T., additional, Gerbino, M., additional, Grandis, S., additional, Hagstotz, S., additional, Hanany, S., additional, Handley, W., additional, Hervias-Caimapo, C., additional, Hills, M., additional, Hivon, E., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lagache, G., additional, Lamagna, L., additional, Lasenby, A., additional, Lattanzi, M., additional, Brun, A. Le, additional, Lesgourgues, J., additional, Lewis, A., additional, Liguori, M., additional, Lindholm, V., additional, Luzzi, G., additional, Maffei, B., additional, Mandolesi, N., additional, Martinez-Gonzalez, E., additional, Martins, C.J.A.P., additional, Masi, S., additional, Massardi, M., additional, Matarrese, S., additional, McCarthy, D., additional, Melchiorri, A., additional, Melin, J.-B., additional, Molinari, D., additional, Monfardini, A., additional, Natoli, P., additional, Notari, A., additional, Paiella, A., additional, Paoletti, D., additional, Partridge, R.B., additional, Patanchon, G., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Remazeilles, M., additional, Roman, M., additional, Rossi, G., additional, Roukema, B.F., additional, Rubiño-Martín, J.-A., additional, Salvati, L., additional, Scott, D., additional, Serjeant, S., additional, Tartari, A., additional, Toffolatti, L., additional, Tomasi, M., additional, Trappe, N., additional, Triqueneaux, S., additional, Trombetti, T., additional, Tucci, M., additional, Tucker, C., additional, Väliviita, J., additional, de Weygaert, R. van, additional, Tent, B. Van, additional, Vennin, V., additional, Vielva, P., additional, Vittorio, N., additional, Young, K., additional, and Zannoni, M., additional

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2018
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238. Exploring cosmic origins with CORE: Survey requirements and mission design

Author

Delabrouille, J., primary, de Bernardis, P., additional, Bouchet, F.R., additional, Achúcarro, A., additional, Ade, P. A. R., additional, Allison, R., additional, Arroja, F., additional, Artal, E., additional, Ashdown, M., additional, Baccigalupi, C., additional, Ballardini, M., additional, Banday, A.J., additional, Banerji, R., additional, Barbosa, D., additional, Bartlett, J., additional, Bartolo, N., additional, Basak, S., additional, Baselmans, J.J.A., additional, Basu, K., additional, Battistelli, E. S., additional, Battye, R., additional, Baumann, D., additional, Benoít, A., additional, Bersanelli, M., additional, Bideaud, A., additional, Biesiada, M., additional, Bilicki, M., additional, Bonaldi, A., additional, Bonato, M., additional, Borrill, J., additional, Boulanger, F., additional, Brinckmann, T., additional, Brown, M.L., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Cabass, G., additional, Cai, Z.-Y., additional, Calvo, M., additional, Caputo, A., additional, Carvalho, C.-S., additional, Casas, F.J., additional, Castellano, G., additional, Catalano, A., additional, Challinor, A., additional, Charles, I., additional, Chluba, J., additional, Clements, D.L., additional, Clesse, S., additional, Colafrancesco, S., additional, Colantoni, I., additional, Contreras, D., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, D'Amico, G., additional, Silva, A. da, additional, de Avillez, M., additional, de Gasperis, G., additional, Petris, M. De, additional, de Zotti, G., additional, Danese, L., additional, Désert, F.-X., additional, Desjacques, V., additional, Valentino, E. Di, additional, Dickinson, C., additional, Diego, J.M., additional, Doyle, S., additional, Durrer, R., additional, Dvorkin, C., additional, Eriksen, H.K., additional, Errard, J., additional, Feeney, S., additional, Fernández-Cobos, R., additional, Finelli, F., additional, Forastieri, F., additional, Franceschet, C., additional, Fuskeland, U., additional, Galli, S., additional, Génova-Santos, R.T., additional, Gerbino, M., additional, Giusarma, E., additional, Gomez, A., additional, González-Nuevo, J., additional, Grandis, S., additional, Greenslade, J., additional, Goupy, J., additional, Hagstotz, S., additional, Hanany, S., additional, Handley, W., additional, Henrot-Versillé, S., additional, Hernández-Monteagudo, C., additional, Hervias-Caimapo, C., additional, Hills, M., additional, Hindmarsh, M., additional, Hivon, E., additional, Hoang, D.T., additional, Hooper, D.C., additional, Hu, B., additional, Keihänen, E., additional, Keskitalo, R., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lagache, G., additional, Lamagna, L., additional, Lapi, A., additional, Lasenby, A., additional, Lattanzi, M., additional, Brun, A.M.C. Le, additional, Lesgourgues, J., additional, Liguori, M., additional, Lindholm, V., additional, Lizarraga, J., additional, Luzzi, G., additional, Macìas-Pérez, J.F., additional, Maffei, B., additional, Mandolesi, N., additional, Martin, S., additional, Martinez-Gonzalez, E., additional, Martins, C.J.A.P., additional, Masi, S., additional, Massardi, M., additional, Matarrese, S., additional, Mazzotta, P., additional, McCarthy, D., additional, Melchiorri, A., additional, Melin, J.-B., additional, Mennella, A., additional, Mohr, J., additional, Molinari, D., additional, Monfardini, A., additional, Montier, L., additional, Natoli, P., additional, Negrello, M., additional, Notari, A., additional, Noviello, F., additional, Oppizzi, F., additional, O'Sullivan, C., additional, Pagano, L., additional, Paiella, A., additional, Pajer, E., additional, Paoletti, D., additional, Paradiso, S., additional, Partridge, R.B., additional, Patanchon, G., additional, Patil, S.P., additional, Perdereau, O., additional, Piacentini, F., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Ponthieu, N., additional, Poulin, V., additional, Prêle, D., additional, Quartin, M., additional, Ravenni, A., additional, Remazeilles, M., additional, Renzi, A., additional, Ringeval, C., additional, Roest, D., additional, Roman, M., additional, Roukema, B.F., additional, Rubiño-Martin, J.-A., additional, Salvati, L., additional, Scott, D., additional, Serjeant, S., additional, Signorelli, G., additional, Starobinsky, A.A., additional, Sunyaev, R., additional, Tan, C.Y., additional, Tartari, A., additional, Tasinato, G., additional, Toffolatti, L., additional, Tomasi, M., additional, Torrado, J., additional, Tramonte, D., additional, Trappe, N., additional, Triqueneaux, S., additional, Tristram, M., additional, Trombetti, T., additional, Tucci, M., additional, Tucker, C., additional, Urrestilla, J., additional, Väliviita, J., additional, de Weygaert, R. Van, additional, Tent, B. Van, additional, Vennin, V., additional, Verde, L., additional, Vermeulen, G., additional, Vielva, P., additional, Vittorio, N., additional, Voisin, F., additional, Wallis, C., additional, Wandelt, B., additional, Wehus, I.K., additional, Weller, J., additional, Young, K., additional, and Zannoni, M., additional

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2018
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239. Exploring cosmic origins with CORE:B-mode component separation

Author

Remazeilles, M., primary, Banday, A.J., additional, Baccigalupi, C., additional, Basak, S., additional, Bonaldi, A., additional, Zotti, G. De, additional, Delabrouille, J., additional, Dickinson, C., additional, Eriksen, H. K., additional, Errard, J., additional, Fernandez-Cobos, R., additional, Fuskeland, U., additional, Hervías-Caimapo, C., additional, López-Caniego, M., additional, Martinez-González, E., additional, Roman, M., additional, Vielva, P., additional, Wehus, I., additional, Achucarro, A., additional, Ade, P., additional, Allison, R., additional, Ashdown, M., additional, Ballardini, M., additional, Banerji, R., additional, Bartlett, J., additional, Bartolo, N., additional, Baumann, D., additional, Bersanelli, M., additional, Bonato, M., additional, Borrill, J., additional, Bouchet, F., additional, Boulanger, F., additional, Brinckmann, T., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Cai, Z.-Y., additional, Calvo, M., additional, Carvalho, C.-S., additional, Castellano, G., additional, Challinor, A., additional, Chluba, J., additional, Clesse, S., additional, Colantoni, I., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, de Bernardis, P., additional, de Gasperis, G., additional, Diego, J.-M., additional, Valentino, E. Di, additional, Feeney, S., additional, Ferraro, S., additional, Finelli, F., additional, Forastieri, F., additional, Galli, S., additional, Genova-Santos, R., additional, Gerbino, M., additional, González-Nuevo, J., additional, Grandis, S., additional, Greenslade, J., additional, Hagstotz, S., additional, Hanany, S., additional, Handley, W., additional, Hernandez-Monteagudo, C., additional, Hills, M., additional, Hivon, E., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lamagna, L., additional, Lasenby, A., additional, Lattanzi, M., additional, Lesgourgues, J., additional, Lewis, A., additional, Liguori, M., additional, Lindholm, V., additional, Luzzi, G., additional, Maffei, B., additional, Martins, C.J.A.P., additional, Masi, S., additional, Matarrese, S., additional, McCarthy, D., additional, Melin, J.-B., additional, Melchiorri, A., additional, Molinari, D., additional, Monfardini, A., additional, Natoli, P., additional, Negrello, M., additional, Notari, A., additional, Paiella, A., additional, Paoletti, D., additional, Patanchon, G., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Rubino-Martin, J.-A., additional, Salvati, L., additional, Tartari, A., additional, Tomasi, M., additional, Tramonte, D., additional, Trappe, N., additional, Trombetti, T., additional, Tucker, C., additional, Valiviita, J., additional, de Weijgaert, R. Van, additional, Tent, B. van, additional, Vennin, V., additional, Vittorio, N., additional, Young, K., additional, and Zannoni, M., additional

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2018
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240. Exploring cosmic origins with CORE: The instrument

Author

de Bernardis, P., primary, Ade, P.A.R., additional, Baselmans, J.J.A., additional, Battistelli, E.S., additional, Benoit, A., additional, Bersanelli, M., additional, Bideaud, A., additional, Calvo, M., additional, Casas, F.J., additional, Castellano, M.G., additional, Catalano, A., additional, Charles, I., additional, Colantoni, I., additional, Columbro, F., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, Petris, M. De, additional, Delabrouille, J., additional, Doyle, S., additional, Franceschet, C., additional, Gomez, A., additional, Goupy, J., additional, Hanany, S., additional, Hills, M., additional, Lamagna, L., additional, Macias-Perez, J., additional, Maffei, B., additional, Martin, S., additional, Martinez-Gonzalez, E., additional, Masi, S., additional, McCarthy, D., additional, Mennella, A., additional, Monfardini, A., additional, Noviello, F., additional, Paiella, A., additional, Piacentini, F., additional, Piat, M., additional, Pisano, G., additional, Signorelli, G., additional, Tan, C.Y., additional, Tartari, A., additional, Trappe, N., additional, Triqueneaux, S., additional, Tucker, C., additional, Vermeulen, G., additional, Young, K., additional, Zannoni, M., additional, Achúcarro, A., additional, Allison, R., additional, Artall, E., additional, Ashdown, M., additional, Ballardini, M., additional, Banday, A.J., additional, Banerji, R., additional, Bartlett, J., additional, Bartolo, N., additional, Basak, S., additional, Bonaldi, A., additional, Bonato, M., additional, Borrill, J., additional, Bouchet, F., additional, Boulanger, F., additional, Brinckmann, T., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Cai, Z.Y., additional, Carvalho, C.S., additional, Challinor, A., additional, Chluba, J., additional, Clesse, S., additional, Gasperis, G. De, additional, Zotti, G. De, additional, Valentino, E. Di, additional, Diego, J.M., additional, Errard, J., additional, Feeney, S., additional, Fernandez-Cobos, R., additional, Finelli, F., additional, Forastieri, F., additional, Galli, S., additional, Génova-Santos, R., additional, Gerbino, M., additional, González-Nuevo, J., additional, Hagstotz, S., additional, Greenslade, J., additional, Handley, W., additional, Hernández-Monteagudo, C., additional, Hervias-Caimapo, C., additional, Hivon, E., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lasenby, A., additional, Lattanzi, M., additional, Lesgourgues, J., additional, Lewis, A., additional, Liguori, M., additional, Lindholm, V., additional, Luzzi, G., additional, Martins, C.J.A.P., additional, Matarrese, S., additional, Melchiorri, A., additional, Melin, J.B., additional, Molinari, D., additional, Natoli, P., additional, Negrello, M., additional, Notari, A., additional, Paoletti, D., additional, Patanchon, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Remazeilles, M., additional, Roman, M., additional, Rubiño-Martín, J.A., additional, Salvati, L., additional, Tomasi, M., additional, Tramonte, D., additional, Trombetti, T., additional, Väliviita, J., additional, de Weyjgaert, R. Van, additional, Tent, B. van, additional, Vennin, V., additional, Vielva, P., additional, and Vittorio, N., additional

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2018
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241. Exploring cosmic origins with CORE: Gravitational lensing of the CMB

Author

Challinor, A., primary, Allison, R., additional, Carron, J., additional, Errard, J., additional, Feeney, S., additional, Kitching, T., additional, Lesgourgues, J., additional, Lewis, A., additional, Zubeldía, Í., additional, Achucarro, A., additional, Ade, P., additional, Ashdown, M., additional, Ballardini, M., additional, Banday, A.J., additional, Banerji, R., additional, Bartlett, J., additional, Bartolo, N., additional, Basak, S., additional, Baumann, D., additional, Bersanelli, M., additional, Bonaldi, A., additional, Bonato, M., additional, Borrill, J., additional, Bouchet, F., additional, Boulanger, F., additional, Brinckmann, T., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Cai, Z.-Y., additional, Calvo, M., additional, Carvalho, C.-S., additional, Castellano, G., additional, Chluba, J., additional, Clesse, S., additional, Colantoni, I., additional, Coppolecchia, A., additional, Crook, M., additional, d'Alessandro, G., additional, de Bernardis, P., additional, de Gasperis, G., additional, Zotti, G. De, additional, Delabrouille, J., additional, Valentino, E. Di, additional, Diego, J.-M., additional, Fernandez-Cobos, R., additional, Ferraro, S., additional, Finelli, F., additional, Forastieri, F., additional, Galli, S., additional, Genova-Santos, R., additional, Gerbino, M., additional, González-Nuevo, J., additional, Grandis, S., additional, Greenslade, J., additional, Hagstotz, S., additional, Hanany, S., additional, Handley, W., additional, Hernandez-Monteagudo, C., additional, Hervías-Caimapo, C., additional, Hills, M., additional, Hivon, E., additional, Kiiveri, K., additional, Kisner, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lamagna, L., additional, Lasenby, A., additional, Lattanzi, M., additional, Liguori, M., additional, Lindholm, V., additional, López-Caniego, M., additional, Luzzi, G., additional, Maffei, B., additional, Martinez-González, E., additional, Martins, C.J.A.P., additional, Masi, S., additional, Matarrese, S., additional, McCarthy, D., additional, Melchiorri, A., additional, Melin, J.-B., additional, Molinari, D., additional, Monfardini, A., additional, Natoli, P., additional, Negrello, M., additional, Notari, A., additional, Paiella, A., additional, Paoletti, D., additional, Patanchon, G., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Remazeilles, M., additional, Roman, M., additional, Rubino-Martin, J.-A., additional, Salvati, L., additional, Tartari, A., additional, Tomasi, M., additional, Tramonte, D., additional, Trappe, N., additional, Trombetti, T., additional, Tucker, C., additional, Valiviita, J., additional, de Weijgaert, R. Van, additional, Tent, B. van, additional, Vennin, V., additional, Vielva, P., additional, Vittorio, N., additional, Young, K., additional, and Zannoni, M., additional

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2018
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242. Exploring cosmic origins with CORE: Mitigation of systematic effects

Author

Natoli, P., primary, Ashdown, M., additional, Banerji, R., additional, Borrill, J., additional, Buzzelli, A., additional, de Gasperis, G., additional, Delabrouille, J., additional, Hivon, E., additional, Molinari, D., additional, Patanchon, G., additional, Polastri, L., additional, Tomasi, M., additional, Bouchet, F.R., additional, Henrot-Versillé, S., additional, Hoang, D.T., additional, Keskitalo, R., additional, Kiiveri, K., additional, Kisner, T., additional, Lindholm, V., additional, McCarthy, D., additional, Piacentini, F., additional, Perdereau, O., additional, Polenta, G., additional, Tristram, M., additional, Achucarro, A., additional, Ade, P., additional, Allison, R., additional, Baccigalupi, C., additional, Ballardini, M., additional, Banday, A.J., additional, Bartlett, J., additional, Bartolo, N., additional, Basak, S., additional, Baumann, D., additional, Bersanelli, M., additional, Bonaldi, A., additional, Bonato, M., additional, Boulanger, F., additional, Brinckmann, T., additional, Bucher, M., additional, Burigana, C., additional, Cai, Z.-Y., additional, Calvo, M., additional, Carvalho, C.-S., additional, Castellano, M.G., additional, Challinor, A., additional, Chluba, J., additional, Clesse, S., additional, Colantoni, I., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, de Bernardis, P., additional, Zotti, G. De, additional, Valentino, E. Di, additional, Diego, J.-M., additional, Errard, J., additional, Feeney, S., additional, Fernandez-Cobos, R., additional, Finelli, F., additional, Forastieri, F., additional, Galli, S., additional, Genova-Santos, R., additional, Gerbino, M., additional, González-Nuevo, J., additional, Grandis, S., additional, Greenslade, J., additional, Gruppuso, A., additional, Hagstotz, S., additional, Hanany, S., additional, Handley, W., additional, Hernandez-Monteagudo, C., additional, Hervías-Caimapo, C., additional, Hills, M., additional, Keihänen, E., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lamagna, L., additional, Lasenby, A., additional, Lattanzi, M., additional, Lesgourgues, J., additional, Lewis, A., additional, Liguori, M., additional, López-Caniego, M., additional, Luzzi, G., additional, Maffei, B., additional, Mandolesi, N., additional, Martinez-González, E., additional, Martins, C.J.A.P., additional, Masi, S., additional, Matarrese, S., additional, Melchiorri, A., additional, Melin, J.-B., additional, Migliaccio, M., additional, Monfardini, A., additional, Negrello, M., additional, Notari, A., additional, Pagano, L., additional, Paiella, A., additional, Paoletti, D., additional, Piat, M., additional, Pisano, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Remazeilles, M., additional, Roman, M., additional, Rossi, G., additional, Rubino-Martin, J.-A., additional, Salvati, L., additional, Signorelli, G., additional, Tartari, A., additional, Tramonte, D., additional, Trappe, N., additional, Trombetti, T., additional, Tucker, C., additional, Valiviita, J., additional, de Weijgaert, R. Van, additional, Tent, B. van, additional, Vennin, V., additional, Vielva, P., additional, Vittorio, N., additional, Wallis, C., additional, Young, K., additional, and Zannoni, M., additional

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2018
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243. Exploring cosmic origins with CORE: Cosmological parameters

Author

Valentino, E. Di, primary, Brinckmann, T., additional, Gerbino, M., additional, Poulin, V., additional, Bouchet, F.R., additional, Lesgourgues, J., additional, Melchiorri, A., additional, Chluba, J., additional, Clesse, S., additional, Delabrouille, J., additional, Dvorkin, C., additional, Forastieri, F., additional, Galli, S., additional, Hooper, D.C., additional, Lattanzi, M., additional, Martins, C.J.A.P., additional, Salvati, L., additional, Cabass, G., additional, Caputo, A., additional, Giusarma, E., additional, Hivon, E., additional, Natoli, P., additional, Pagano, L., additional, Paradiso, S., additional, Rubiño-Martin, J.A., additional, Achúcarro, A., additional, Ade, P., additional, Allison, R., additional, Arroja, F., additional, Ashdown, M., additional, Ballardini, M., additional, Banday, A.J., additional, Banerji, R., additional, Bartolo, N., additional, Bartlett, J.G., additional, Basak, S., additional, Baumann, D., additional, de Bernardis, P., additional, Bersanelli, M., additional, Bonaldi, A., additional, Bonato, M., additional, Borrill, J., additional, Boulanger, F., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Cai, Z.-Y., additional, Calvo, M., additional, Carvalho, C.S., additional, Castellano, G., additional, Challinor, A., additional, Charles, I., additional, Colantoni, I., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, Petris, M. De, additional, Zotti, G. De, additional, Diego, J.M., additional, Errard, J., additional, Feeney, S., additional, Fernandez-Cobos, R., additional, Ferraro, S., additional, Finelli, F., additional, de Gasperis, G., additional, Génova-Santos, R.T., additional, González-Nuevo, J., additional, Grandis, S., additional, Greenslade, J., additional, Hagstotz, S., additional, Hanany, S., additional, Handley, W., additional, Hazra, D.K., additional, Hernández-Monteagudo, C., additional, Hervias-Caimapo, C., additional, Hills, M., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lamagna, L., additional, Lasenby, A., additional, Lewis, A., additional, Liguori, M., additional, Lindholm, V., additional, Lopez-Caniego, M., additional, Luzzi, G., additional, Maffei, B., additional, Martin, S., additional, Martinez-Gonzalez, E., additional, Masi, S., additional, Matarrese, S., additional, McCarthy, D., additional, Melin, J.-B., additional, Mohr, J.J., additional, Molinari, D., additional, Monfardini, A., additional, Negrello, M., additional, Notari, A., additional, Paiella, A., additional, Paoletti, D., additional, Patanchon, G., additional, Piacentini, F., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Quartin, M., additional, Remazeilles, M., additional, Roman, M., additional, Ringeval, C., additional, Tartari, A., additional, Tomasi, M., additional, Tramonte, D., additional, Trappe, N., additional, Trombetti, T., additional, Tucker, C., additional, Väliviita, J., additional, de Weygaert, R. van, additional, Tent, B. Van, additional, Vennin, V., additional, Vermeulen, G., additional, Vielva, P., additional, Vittorio, N., additional, Young, K., additional, and Zannoni, M., additional

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2018
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244. Exploring forest infrastructures equipment through multivariate analysis: complementarities, gaps and overlaps in the Mediterranean basin

Author

Bajocco, S., Raparelli, E., Patriarca, F., Di Matteo, G., Nardi, P., Perini, L., Salvati, L., and Scarascia Mugnozza, G.

Subjects
multidimensional scaling, lcsh:Agriculture, Mediterranean forest research, FORESTERRA, infrastructures, Mediterranean countries, lcsh:S
Abstract

The countries of the Mediterranean basin face several challenges regarding the sustainability of forest ecosystems and the delivery of crucial goods and services that they provide in a context of rapid global changes. Advancing scientific knowledge and foresting innovation is essential to ensure the sustainable management of Mediterranean forests and maximize the potential role of their unique goods and services in building a knowledge-based bioeconomy in the region. In this context, the European project FORESTERRA ("Enhancing FOrest RESearch in the MediTERRAnean through improved coordination and integration”) aims at reinforcing the scientific cooperation on Mediterranean forests through an ambitious transnational framework in order to reduce the existing research fragmentation and maximize the effectiveness of forest research activities. Within the FORESTERRA project framework, this work analyzed the infrastructures equipment of the Mediterranean countries belonging to the project Consortium. According to the European Commission, research infrastructures are facilities, resources and services that are used by the scientific communities to conduct research and foster innovation. To the best of our knowledge, the equipment and availability of infrastructures, in terms of experimental sites, research facilities and databases, have only rarely been explored. The aim of this paper was hence to identify complementarities, gaps and overlaps among the different forest research institutes in order to create a scientific network, optimize the resources and trigger collaborations.

Published
2013

245. TURNING TO ‘RURALITY’: PROFILING URBAN AND RURAL AREAS FOR THE EVALUATION OF REGIONAL DEVELOPMENT POLICIES

Author

Benaki, V and Salvati, L

Subjects
Land classification, Rural development, Agriculture, Economically-disadvantaged, areas, Greece, Settore SECS-S/03 - Statistica Economica, jel:R52, jel:Q15, jel:R14, jel:Q24
Abstract

A better understanding of strength and weaknesses in rural systems through an adequate set of comprehensive and regularly updated indicators, indicates the necessary prerequisite for a flexible response to policy needs, such as policy targeting and monitoring rural development.The present study is aimed at proposing an effective methodology for defining and profiling different typologies of rural areas. A quantitative exercise has been developed in Greece, an European country showing dramatic economic changes in rural areas during the last decades. Results indicate that the optimal classification for rural areas in Greece can be derived through the combined use of the Degree of Handicap of EU Regulation 1257/99 and Degree of urbanism (using the standard OECD criterion). The methodology illustrated here constitutes an appropriate base for providing a tool informing policy measures destined to support the socioeconomic performances of rural areas in Greece.

Published
2013

246. Planck intermediate results LII. Planet flux densities

Author

Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Benabed, K., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Carron, J., Chiang, H. C., Colombo, L. P. L., Comis, B., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Diego, J. M., Dore, O., Ducout, A., Dupac, X., Elsner, F., Ensslin, T. A., Eriksen, H. K., Falgarone, E., Fantaye, Y., Finelli, F., Frailis, M., Fraisse, A. A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Genova-Santos, R. T., Gerbino, Martina, Gonzalez-Nuevo, J., Gorski, K. M., Gruppuso, A., Gudmundsson, Jón E., Hansen, F. K., Helou, G., Henrot-Versille, S., Herranz, D., Hivon, E., Jaffe, A. H., Jones, W. C., Keihanen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Le Jeune, M., Lellouch, E., Levrier, F., Liguori, M., Lilje, P. B., Lindholm, V., Lopez-Caniego, M., Ma, Y. -Z., Macias-Perez, J. F., Maggio, G., Maino, D., Mandolesi, N., Maris, M., Martin, P. G., Martinez-Gonzalez, E., Matarrese, S., Mauri, N., McEwen, J. D., Melchiorri, A., Mennella, A., Migliaccio, M., Miville-Deschenes, M. -A., Molinari, D., Moneti, A., Montier, L., Moreno, R., Morgante, G., Natoli, P., Oxborrow, C. A., Paoletti, D., Partridge, B., Patanchon, G., Patrizii, L., Perdereau, O., Piacentini, F., Plaszczynski, S., Polenta, G., Rachen, J. P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Romelli, E., Rosset, C., Roudier, G., Rubino-Martin, J. A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Sirri, G., Spencer, L. D., Suur-Uski, A. -S., Tauber, J. A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Valiviita, J., Van Tent, F., Vielva, P., Villa, F., Wehus, I. K., Zacchei, A., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Benabed, K., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bucher, M., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Carron, J., Chiang, H. C., Colombo, L. P. L., Comis, B., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Diego, J. M., Dore, O., Ducout, A., Dupac, X., Elsner, F., Ensslin, T. A., Eriksen, H. K., Falgarone, E., Fantaye, Y., Finelli, F., Frailis, M., Fraisse, A. A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Genova-Santos, R. T., Gerbino, Martina, Gonzalez-Nuevo, J., Gorski, K. M., Gruppuso, A., Gudmundsson, Jón E., Hansen, F. K., Helou, G., Henrot-Versille, S., Herranz, D., Hivon, E., Jaffe, A. H., Jones, W. C., Keihanen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Le Jeune, M., Lellouch, E., Levrier, F., Liguori, M., Lilje, P. B., Lindholm, V., Lopez-Caniego, M., Ma, Y. -Z., Macias-Perez, J. F., Maggio, G., Maino, D., Mandolesi, N., Maris, M., Martin, P. G., Martinez-Gonzalez, E., Matarrese, S., Mauri, N., McEwen, J. D., Melchiorri, A., Mennella, A., Migliaccio, M., Miville-Deschenes, M. -A., Molinari, D., Moneti, A., Montier, L., Moreno, R., Morgante, G., Natoli, P., Oxborrow, C. A., Paoletti, D., Partridge, B., Patanchon, G., Patrizii, L., Perdereau, O., Piacentini, F., Plaszczynski, S., Polenta, G., Rachen, J. P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Romelli, E., Rosset, C., Roudier, G., Rubino-Martin, J. A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Sirri, G., Spencer, L. D., Suur-Uski, A. -S., Tauber, J. A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Valiviita, J., Van Tent, F., Vielva, P., Villa, F., Wehus, I. K., and Zacchei, A.

Abstract

Measurements of flux density are described for five planets, Mars, Jupiter, Saturn, Uranus, and Neptune, across the six Planck High Frequency Instrument frequency bands (100-857 GHz) and these are then compared with models and existing data. In our analysis, we have also included estimates of the brightness of Jupiter and Saturn at the three frequencies of the Planck Low Frequency Instrument (30, 44, and 70 GHz). The results provide constraints on the intrinsic brightness and the brightness time-variability of these planets. The majority of the planet flux density estimates are limited by systematic errors, but still yield better than 1% measurements in many cases. Applying data from Planck HFI, the Wilkinson Microwave Anisotropy Probe (WMAP), and the Atacama Cosmology Telescope (ACT) to a model that incorporates contributions from Saturn's rings to the planet's total flux density suggests a best fit value for the spectral index of Saturn's ring system of beta(ring) = 2 : 30 +/- 0 : 03 over the 30-1000 GHz frequency range. Estimates of the polarization amplitude of the planets have also been made in the four bands that have polarization-sensitive detectors (100-353 GHz); this analysis provides a 95% confidence level upper limit on Mars's polarization of 1.8, 1.7, 1.2, and 1.7% at 100, 143, 217, and 353 GHz, respectively. The average ratio between the Planck-HFI measurements and the adopted model predictions for all five planets (excluding Jupiter observations for 353 GHz) is 1.004, 1.002, 1.021, and 1.033 for 100, 143, 217, and 353 GHz, respectively. Model predictions for planet thermodynamic temperatures are therefore consistent with the absolute calibration of Planck-HFI detectors at about the three-percent level. We compare our measurements with published results from recent cosmic microwave background experiments. In particular, we observe that the flux densities measured by Planck HFI and WMAP agree to within 2%. These results allow experiments operating in the

Published
2017
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247. Exploring cosmic origins with CORE: mitigation of systematic effects

Author

Natoli, P., Ashdown, M., Banerji, R., Borrill, J., Buzzelli, A., de Gasperis, G., Delabrouille, J., Hivon, E., Molinari, D., Patanchon, G., Polastri, L., Tomasi, M., Bouchet, F. R., Henrot-Versillé, S., Hoang, D. T., Keskitalo, R., Kiiveri, K., Kisner, T., Lindholm, V., McCarthy, D., Piacentini, F., Perdereau, O., Polenta, G., Tristram, M., Achucarro, A., Ade, P., Allison, R., Baccigalupi, C., Ballardini, M., Banday, A. J., Bartlett, J., Bartolo, N., Basak, S., Baselmans, J., Baumann, D., Bersanelli, M., Bonaldi, A., Bonato, M., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Cai, Z. -Y., Calvo, M., Carvalho, C. -S., Castellano, G., Challinor, A., Chluba, J., Clesse, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., de Bernardis, P., De Zotti, G., Di Valentino, E., Diego, J. -M., Errard, J., Feeney, S., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Galli, S., Genova-Santos, R., Gerbino, M., Gonzalez-Nuevo, J., Grandis, S., Greenslade, J., Gruppuso, A., Hagstotz, S., Hanany, S., Handley, W., Hernandez-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Keihänen, E., Kitching, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Lesgourgues, J., Lewis, A., Liguori, M., López-Caniego, M., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Melchiorri, A., Melin, J. -B., Migliaccio, M., Monfardini, A., Negrello, M., Notari, A., Pagano, L., Paiella, A., Paoletti, D., Piat, M., Pisano, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Rubino-Martin, J. -A., Salvati, L., Signorelli, G., Tartari, A., Tramonte, D., Trappe, N., Trombetti, T., Tucker, C., Valiviita, J., Van de Weijgaert, R., van Tent, B., Vennin, V., Vielva, P., Vittorio, N., Wallis, C., Young, K., Zannoni, M., Natoli, P., Ashdown, M., Banerji, R., Borrill, J., Buzzelli, A., de Gasperis, G., Delabrouille, J., Hivon, E., Molinari, D., Patanchon, G., Polastri, L., Tomasi, M., Bouchet, F. R., Henrot-Versillé, S., Hoang, D. T., Keskitalo, R., Kiiveri, K., Kisner, T., Lindholm, V., McCarthy, D., Piacentini, F., Perdereau, O., Polenta, G., Tristram, M., Achucarro, A., Ade, P., Allison, R., Baccigalupi, C., Ballardini, M., Banday, A. J., Bartlett, J., Bartolo, N., Basak, S., Baselmans, J., Baumann, D., Bersanelli, M., Bonaldi, A., Bonato, M., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Cai, Z. -Y., Calvo, M., Carvalho, C. -S., Castellano, G., Challinor, A., Chluba, J., Clesse, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., de Bernardis, P., De Zotti, G., Di Valentino, E., Diego, J. -M., Errard, J., Feeney, S., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Galli, S., Genova-Santos, R., Gerbino, M., Gonzalez-Nuevo, J., Grandis, S., Greenslade, J., Gruppuso, A., Hagstotz, S., Hanany, S., Handley, W., Hernandez-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Keihänen, E., Kitching, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Lesgourgues, J., Lewis, A., Liguori, M., López-Caniego, M., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Melchiorri, A., Melin, J. -B., Migliaccio, M., Monfardini, A., Negrello, M., Notari, A., Pagano, L., Paiella, A., Paoletti, D., Piat, M., Pisano, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Rubino-Martin, J. -A., Salvati, L., Signorelli, G., Tartari, A., Tramonte, D., Trappe, N., Trombetti, T., Tucker, C., Valiviita, J., Van de Weijgaert, R., van Tent, B., Vennin, V., Vielva, P., Vittorio, N., Wallis, C., Young, K., and Zannoni, M.

Abstract

We present an analysis of the main systematic effects that could impact the measurement of CMB polarization with the proposed CORE space mission. We employ timeline-to-map simulations to verify that the CORE instrumental set-up and scanning strategy allow us to measure sky polarization to a level of accuracy adequate to the mission science goals. We also show how the CORE observations can be processed to mitigate the level of contamination by potentially worrying systematics, including intensity-to-polarization leakage due to bandpass mismatch, asymmetric main beams, pointing errors and correlated noise. We use analysis techniques that are well validated on data from current missions such as Planck to demonstrate how the residual contamination of the measurements by these effects can be brought to a level low enough not to hamper the scientific capability of the mission, nor significantly increase the overall error budget. We also present a prototype of the CORE photometric calibration pipeline, based on that used for Planck, and discuss its robustness to systematics, showing how CORE can achieve its calibration requirements. While a fine-grained assessment of the impact of systematics requires a level of knowledge of the system that can only be achieved in a future study phase, the analysis presented here strongly suggests that the main areas of concern for the CORE mission can be addressed using existing knowledge, techniques and algorithms., Comment: 54 pages, 26 figures, 3 tables

Published
2017
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248. Exploring cosmic origins with CORE: effects of observer peculiar motion

Author

Burigana, C., Carvalho, C. S., Trombetti, T., Notari, A., Quartin, M., De Gasperis, G., Buzzelli, A., Vittorio, N., De Zotti, G., de Bernardis, P., Chluba, J., Bilicki, M., Danese, L., Delabrouille, J., Toffolatti, L., Lapi, A., Negrello, M., Mazzotta, P., Scott, D., Contreras, D., Achucarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J., Bartolo, N., Basak, S., Bersanelli, M., Bonaldi, A., Bonato, M., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Cabella, P., Cai, Z. -Y., Calvo, M., Castellano, G., Challinor, A., Clesse, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., Diego, J. -M., Di Marco, A., Di Valentino, E., Errard, J., Feeney, S., Fernandez-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Genova-Santos, R., Gerbino, M., Gonzalez-Nuevo, J., Grandis, S., Greenslade, J., Hagstotz, S., Hanany, S., Handley, W., Hernandez-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Lesgourgues, J., Liguori, M., Lindholm, V., Lopez-Caniego, M., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., McCarthy, D., Melchiorri, A., Melin, J. -B., Molinari, D., Monfardini, A., Natoli, P., Paiella, A., Paoletti, D., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Remazeilles, M., Roman, M., Rubino-Martin, J. -A., Salvati, L., Tartari, A., Tomasi, M., Tramonte, D., Trappe, N., Tucker, C., Valiviita, J., Van de Weijgaert, R., van Tent, B., Vennin, V., Vielva, P., Young, K., Zannoni, M., Burigana, C., Carvalho, C. S., Trombetti, T., Notari, A., Quartin, M., De Gasperis, G., Buzzelli, A., Vittorio, N., De Zotti, G., de Bernardis, P., Chluba, J., Bilicki, M., Danese, L., Delabrouille, J., Toffolatti, L., Lapi, A., Negrello, M., Mazzotta, P., Scott, D., Contreras, D., Achucarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J., Bartolo, N., Basak, S., Bersanelli, M., Bonaldi, A., Bonato, M., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Cabella, P., Cai, Z. -Y., Calvo, M., Castellano, G., Challinor, A., Clesse, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., Diego, J. -M., Di Marco, A., Di Valentino, E., Errard, J., Feeney, S., Fernandez-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Genova-Santos, R., Gerbino, M., Gonzalez-Nuevo, J., Grandis, S., Greenslade, J., Hagstotz, S., Hanany, S., Handley, W., Hernandez-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lamagna, L., Lasenby, A., Lattanzi, M., Lesgourgues, J., Liguori, M., Lindholm, V., Lopez-Caniego, M., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., McCarthy, D., Melchiorri, A., Melin, J. -B., Molinari, D., Monfardini, A., Natoli, P., Paiella, A., Paoletti, D., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Remazeilles, M., Roman, M., Rubino-Martin, J. -A., Salvati, L., Tartari, A., Tomasi, M., Tramonte, D., Trappe, N., Tucker, C., Valiviita, J., Van de Weijgaert, R., van Tent, B., Vennin, V., Vielva, P., Young, K., and Zannoni, M.

Abstract

We discuss the effects on the CMB, CIB, and thermal SZ effect due to the peculiar motion of an observer with respect to the CMB rest frame, which induces boosting effects. We investigate the scientific perspectives opened by future CMB space missions, focussing on the CORE proposal. The improvements in sensitivity offered by a mission like CORE, together with its high resolution over a wide frequency range, will provide a more accurate estimate of the CMB dipole. The extension of boosting effects to polarization and cross-correlations will enable a more robust determination of purely velocity-driven effects that are not degenerate with the intrinsic CMB dipole, allowing us to achieve a S/N ratio of 13; this improves on the Planck detection and essentially equals that of an ideal cosmic-variance-limited experiment up to a multipole l of 2000. Precise inter-frequency calibration will offer the opportunity to constrain or even detect CMB spectral distortions, particularly from the cosmological reionization, because of the frequency dependence of the dipole spectrum, without resorting to precise absolute calibration. The expected improvement with respect to COBE-FIRAS in the recovery of distortion parameters (in principle, a factor of several hundred for an ideal experiment with the CORE configuration) ranges from a factor of several up to about 50, depending on the quality of foreground removal and relative calibration. Even for 1% accuracy in both foreground removal and relative calibration at an angular scale of 1 deg, we find that dipole analyses for a mission like CORE will be able to improve the recovery of the CIB spectrum amplitude by a factor of 17 in comparison with current results based on FIRAS. In addition to the scientific potential of a mission like CORE for these analyses, synergies with other planned and ongoing projects are also discussed., Comment: 61+5 pages, 17 figures, 25 tables, 8 sections, 5 appendices. In press on JCAP - Version 3 - Minor changes, affiliations fixed, references updated - version in line with corrected proofs

Published
2017
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249. Exploring Cosmic Origins with CORE: Survey requirements and mission design

Author

Delabrouille, J., de Bernardis, P., Bouchet, F. R., Achúcarro, A., Ade, P. A. R., Allison, R., Arroja, F., Artal, E., Ashdown, M., Baccigalupi, C., Ballardini, M., Banday, A. J., Banerji, R., Barbosa, D., Bartlett, J., Bartolo, N., Basak, S., Baselmans, J. J. A., Basu, K., Battistelli, E. S., Battye, R., Baumann, D., Benoît, A., Bersanelli, M., Bideaud, A., Biesiada, M., Bilicki, M., Bonaldi, A., Bonato, M., Borrill, J., Boulanger, F., Brinckmann, T., Brown, M. L., Bucher, M., Burigana, C., Buzzelli, A., Cabass, G., Cai, Z. -Y., Calvo, M., Caputo, A., Carvalho, C. -S., Casas, F. J., Castellano, G., Catalano, A., Challinor, A., Charles, I., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Contreras, D., Coppolecchia, A., Crook, M., D'Alessandro, G., D'Amico, G., da Silva, A., de Avillez, M., de Gasperis, G., De Petris, M., de Zotti, G., Danese, L., Désert, F. -X., Desjacques, V., Di Valentino, E., Dickinson, C., Diego, J. M., Doyle, S., Durrer, R., Dvorkin, C., Eriksen, H. -K., Errard, J., Feeney, S., Fernández-Cobos, R., Finelli, F., Forastieri, F., Franceschet, C., Fuskeland, U., Galli, S., Génova-Santos, R. T., Gerbino, M., Giusarma, E., Gomez, A., González-Nuevo, J., Grandis, S., Greenslade, J., Goupy, J., Hagstotz, S., Hanany, S., Handley, W., Henrot-Versillé, S., Hernández-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Hindmarsh, M., Hivon, E., Hoang, D. T., Hooper, D. C., Hu, B., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lapi, A., Lasenby, A., Lattanzi, M., Brun, A. M. C. Le, Lesgourgues, J., Liguori, M., Lindholm, V., Lizarraga, J., Luzzi, G., Macìas-Pérez, J. F., Maffei, B., Mandolesi, N., Martin, S., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., Mazzotta, P., McCarthy, D., Melchiorri, A., Melin, J. -B., Mennella, A., Mohr, J., Molinari, D., Monfardini, A., Montier, L., Natoli, P., Negrello, M., Notari, A., Noviello, F., Oppizzi, F., O'Sullivan, C., Pagano, L., Paiella, A., Pajer, E., Paoletti, D., Paradiso, S., Partridge, R. B., Patanchon, G., Patil, S. P., Perdereau, O., Piacentini, F., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Ponthieu, N., Poulin, V., Prêle, D., Quartin, M., Ravenni, A., Remazeilles, M., Renzi, A., Ringeval, C., Roest, D., Roman, M., Roukema, B. F., Rubino-Martin, J. -A., Salvati, L., Scott, D., Serjeant, S., Signorelli, G., Starobinsky, A. A., Sunyaev, R., Tan, C. Y., Tartari, A., Tasinato, G., Toffolatti, L., Tomasi, M., Torrado, J., Tramonte, D., Trappe, N., Triqueneaux, S., Tristram, M., Trombetti, T., Tucci, M., Tucker, C., Urrestilla, J., Väliviita, J., Van de Weygaert, R., Van Tent, B., Vennin, V., Verde, L., Vermeulen, G., Vielva, P., Vittorio, N., Voisin, F., Wallis, C., Wandelt, B., Wehus, I., Weller, J., Young, K., Zannoni, M., Delabrouille, J., de Bernardis, P., Bouchet, F. R., Achúcarro, A., Ade, P. A. R., Allison, R., Arroja, F., Artal, E., Ashdown, M., Baccigalupi, C., Ballardini, M., Banday, A. J., Banerji, R., Barbosa, D., Bartlett, J., Bartolo, N., Basak, S., Baselmans, J. J. A., Basu, K., Battistelli, E. S., Battye, R., Baumann, D., Benoît, A., Bersanelli, M., Bideaud, A., Biesiada, M., Bilicki, M., Bonaldi, A., Bonato, M., Borrill, J., Boulanger, F., Brinckmann, T., Brown, M. L., Bucher, M., Burigana, C., Buzzelli, A., Cabass, G., Cai, Z. -Y., Calvo, M., Caputo, A., Carvalho, C. -S., Casas, F. J., Castellano, G., Catalano, A., Challinor, A., Charles, I., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Contreras, D., Coppolecchia, A., Crook, M., D'Alessandro, G., D'Amico, G., da Silva, A., de Avillez, M., de Gasperis, G., De Petris, M., de Zotti, G., Danese, L., Désert, F. -X., Desjacques, V., Di Valentino, E., Dickinson, C., Diego, J. M., Doyle, S., Durrer, R., Dvorkin, C., Eriksen, H. -K., Errard, J., Feeney, S., Fernández-Cobos, R., Finelli, F., Forastieri, F., Franceschet, C., Fuskeland, U., Galli, S., Génova-Santos, R. T., Gerbino, M., Giusarma, E., Gomez, A., González-Nuevo, J., Grandis, S., Greenslade, J., Goupy, J., Hagstotz, S., Hanany, S., Handley, W., Henrot-Versillé, S., Hernández-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Hindmarsh, M., Hivon, E., Hoang, D. T., Hooper, D. C., Hu, B., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lapi, A., Lasenby, A., Lattanzi, M., Brun, A. M. C. Le, Lesgourgues, J., Liguori, M., Lindholm, V., Lizarraga, J., Luzzi, G., Macìas-Pérez, J. F., Maffei, B., Mandolesi, N., Martin, S., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., Mazzotta, P., McCarthy, D., Melchiorri, A., Melin, J. -B., Mennella, A., Mohr, J., Molinari, D., Monfardini, A., Montier, L., Natoli, P., Negrello, M., Notari, A., Noviello, F., Oppizzi, F., O'Sullivan, C., Pagano, L., Paiella, A., Pajer, E., Paoletti, D., Paradiso, S., Partridge, R. B., Patanchon, G., Patil, S. P., Perdereau, O., Piacentini, F., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Ponthieu, N., Poulin, V., Prêle, D., Quartin, M., Ravenni, A., Remazeilles, M., Renzi, A., Ringeval, C., Roest, D., Roman, M., Roukema, B. F., Rubino-Martin, J. -A., Salvati, L., Scott, D., Serjeant, S., Signorelli, G., Starobinsky, A. A., Sunyaev, R., Tan, C. Y., Tartari, A., Tasinato, G., Toffolatti, L., Tomasi, M., Torrado, J., Tramonte, D., Trappe, N., Triqueneaux, S., Tristram, M., Trombetti, T., Tucci, M., Tucker, C., Urrestilla, J., Väliviita, J., Van de Weygaert, R., Van Tent, B., Vennin, V., Verde, L., Vermeulen, G., Vielva, P., Vittorio, N., Voisin, F., Wallis, C., Wandelt, B., Wehus, I., Weller, J., Young, K., and Zannoni, M.

Abstract

Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. The rationale and options, and the methodologies used to assess the mission's performance, are of interest to other future CMB mission design studies. CORE is designed as a near-ultimate CMB polarisation mission which, for optimal complementarity with ground-based observations, will perform the observations that are known to be essential to CMB polarisation scienceand cannot be obtained by any other means than a dedicated space mission., Comment: 79 pages, 14 figures

Published
2017
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250. Exploring Cosmic Origins with CORE: The Instrument

Author

de Bernardis, P., Ade, P. A. R., Baselmans, J. J. A., Battistelli, E. S., Benoit, A., Bersanelli, M., Bideaud, A., Calvo, M., Casas, F. J., Castellano, G., Catalano, A., Charles, I., Colantoni, I., Columbro, F., Coppolecchia, A., Crook, M., D'Alessandro, G., De Petris, M., Delabrouille, J., Doyle, S., Franceschet, C., Gomez, A., Goupy, J., Hanany, S., Hills, M., Lamagna, L., Macias-Perez, J., Maffei, B., Martin, S., Martinez-Gonzalez, E., Masi, S., McCarthy, D., Mennella, A., Monfardini, A., Noviello, F., Paiella, A., Piacentini, F., Piat, M., Pisano, G., Signorelli, G., Tan, C. Y., Tartari, A., Trappe, N., Triqueneaux, S., Tucker, C., Vermeulen, G., Young, K., Zannoni, M., Achúcarro, A., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J., Bartolo, N., Basak, S., Bonaldi, A., Bonato, M., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Cai, Z. Y., Carvalho, C. S., Challinor, A., Chluba, J., Clesse, S., De Gasperis, G., De Zotti, G., Di Valentino, E., Diego, J. M., Errard, J., Feeney, S., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Galli, S., Génova-Santos, R., Gerbino, M., González-Nuevo, J., Hagstotz, S., Greenslade, J., Handley, W., Hernández-Monteagudo, C., Hervias-Caimapo, C., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lasenby, A., Lattanzi, M., Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Luzzi, G., Martins, C. J. A. P., Melchiorri, A., Melin, J. B., Molinari, D., Natoli, P., Negrello, M., Notari, A., Paoletti, D., Patanchon, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rubiño-Martín, J. A., Salvati, L., Tomasi, M., Tramonte, D., Trombetti, T., Väliviita, J., Van de Weijgaert, R., van Tent, B., Vennin, V., Vielva, P., Vittorio, N., de Bernardis, P., Ade, P. A. R., Baselmans, J. J. A., Battistelli, E. S., Benoit, A., Bersanelli, M., Bideaud, A., Calvo, M., Casas, F. J., Castellano, G., Catalano, A., Charles, I., Colantoni, I., Columbro, F., Coppolecchia, A., Crook, M., D'Alessandro, G., De Petris, M., Delabrouille, J., Doyle, S., Franceschet, C., Gomez, A., Goupy, J., Hanany, S., Hills, M., Lamagna, L., Macias-Perez, J., Maffei, B., Martin, S., Martinez-Gonzalez, E., Masi, S., McCarthy, D., Mennella, A., Monfardini, A., Noviello, F., Paiella, A., Piacentini, F., Piat, M., Pisano, G., Signorelli, G., Tan, C. Y., Tartari, A., Trappe, N., Triqueneaux, S., Tucker, C., Vermeulen, G., Young, K., Zannoni, M., Achúcarro, A., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J., Bartolo, N., Basak, S., Bonaldi, A., Bonato, M., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Cai, Z. Y., Carvalho, C. S., Challinor, A., Chluba, J., Clesse, S., De Gasperis, G., De Zotti, G., Di Valentino, E., Diego, J. M., Errard, J., Feeney, S., Fernandez-Cobos, R., Finelli, F., Forastieri, F., Galli, S., Génova-Santos, R., Gerbino, M., González-Nuevo, J., Hagstotz, S., Greenslade, J., Handley, W., Hernández-Monteagudo, C., Hervias-Caimapo, C., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lasenby, A., Lattanzi, M., Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Luzzi, G., Martins, C. J. A. P., Melchiorri, A., Melin, J. B., Molinari, D., Natoli, P., Negrello, M., Notari, A., Paoletti, D., Patanchon, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rubiño-Martín, J. A., Salvati, L., Tomasi, M., Tramonte, D., Trombetti, T., Väliviita, J., Van de Weijgaert, R., van Tent, B., Vennin, V., Vielva, P., and Vittorio, N.

Abstract

We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave Background. The instrument is optimized to be compatible with the strict budget requirements of a medium-size space mission within the Cosmic Vision Programme of the European Space Agency. The instrument has no moving parts, and uses arrays of diffraction-limited Kinetic Inductance Detectors to cover the frequency range from 60 GHz to 600 GHz in 19 wide bands, in the focal plane of a 1.2 m aperture telescope cooled at 40 K, allowing for an accurate extraction of the CMB signal from polarized foreground emission. The projected CMB polarization survey sensitivity of this instrument, after foregrounds removal, is 1.7 {\mu}K$\cdot$arcmin. The design is robust enough to allow, if needed, a downscoped version of the instrument covering the 100 GHz to 600 GHz range with a 0.8 m aperture telescope cooled at 85 K, with a projected CMB polarization survey sensitivity of 3.2 {\mu}K$\cdot$arcmin., Comment: 43 pages

Published
2017
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