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PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Vision program a set of important scientific questions that require high resolution, high sensitivity, full-sky observations of the sky emission at wavelengths ranging from millimeter-wave to the far-infrared. PRISM's main objective is to explore the distant universe, probing cosmic history from very early times until now as well as the structures, distribution of matter, and velocity flows throughout our Hubble volume. PRISM will survey the full sky in a large number of frequency bands in both intensity and polarization and will measure the absolute spectrum of sky emission more than three orders of magnitude better than COBE FIRAS. The aim of this Extended White Paper is to provide a more detailed overview of the highlights of the new science that will be made possible by PRISM
PRISM (Polarized radiation imaging and spectroscopy mission) : an extended white paper / P. André, C. Baccigalupi, A. Banday, D. Barbosa, B. Barreiro, J. Bartlett, N. Bartolo, E. Battistelli, R. Battye, G. Bendo, A. Benoît, J.P. Bernard, M. Bersanelli, M. Béthermin, P. Bielewicz, A. Bonaldi, F.C. Bouchet, F.C. Boulanger, J. Brand, M. Bucher, C. Burigana, Z.Y. Cai, P. Camus, F. Casas, V. Casasola, G. Castex, A. Challinor, J. Chluba, G. Chon, S. Colafrancesco, B. Comis, F. Cuttaia, G. D'Alessandro, A.D. Silva, R. Davis, M.D. Avillez, P.D. Bernardis, M.D. Petris, A.D. Rosa, G.D. Zotti, J. Delabrouille, F.C.X. Désert, C. Dickinson, J.M. Diego, J. Dunkley, T. Enßlin, J. Errard, E. Falgarone, P. Ferreira, K. Ferrière, F. Finelli, A. Fletcher, P. Fosalba, G. Fuller, S. Galli, K. Ganga, J. García-Bellido, A. Ghribi, M. Giard, Y. Giraud-Héraud, J. Gonzalez-Nuevo, K. Grainge, A. Gruppuso, A. Hall, J.C. Hamilton, M. Haverkorn, C. Hernandez-Monte-Agudo, D. Herranz, M. Jackson, A. Jaffe, R. Khatri, M. Kunz, L. Lamagna, M. Lattanzi, P. Leahy, J. Lesgourgues, M. Liguori, E. Liuzzo, M. Lopez-Caniego, J. Macias-Perez, B. Maffei, D. Maino, A. Mangilli, E. Martinez-Gonzalez, C. Martins, S. Masi, M. Massardi, S. Matarrese, A. Melchiorri, J.B. Melin, A. Mennella, A. Mignano, M.A. Miville-Deschênes, A. Monfardini, A. Murphy, P. Naselsky, F. Nati, P. Natoli, M. Negrello, F. Noviello, C. O'Sullivan, F. Paci, L. Pagano, R. Paladino, N. Palanque-Delabrouille, D. Paoletti, H. Peiris, F. Perrotta, F. Piacentini, M. Piat, L. Piccirillo, G. Pisano, G. Polenta, A. Pollo, N. Ponthieu, M. Remazeilles, S. Ricciardi, M. Roman, C. Rosset, J.A. Rubino-Martin, M. Salatino, A. Schillaci, P. Shellard, J. Silk, A. Starobinsky, R. Stompor, R. Sunyaev, A. Tartari, L. Terenzi, L. Toffolatti, M. Tomasi, N. Trappe, M. Tristram, T. Trombetti, M. Tucci, R.V.D. Weijgaert, B.V. Tent, L. Verde, P. Vielva, B. Wandelt, R. Watson, S. Withington. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - 2014:2(2014 Feb 05), pp. 006.1-006.68. [10.1088/1475-7516/2014/02/006]
PRISM (Polarized radiation imaging and spectroscopy mission) : an extended white paper
P. André;C. Baccigalupi;A. Banday;D. Barbosa;B. Barreiro;J. Bartlett;N. Bartolo;E. Battistelli;R. Battye;G. Bendo;A. Benoît;J. P. Bernard;M. Bersanelli;M. Béthermin;P. Bielewicz;A. Bonaldi;F. C. Bouchet;F. C. Boulanger;J. Brand;M. Bucher;C. Burigana;Z. Y. Cai;P. Camus;F. Casas;V. Casasola;G. Castex;A. Challinor;J. Chluba;G. Chon;S. Colafrancesco;B. Comis;F. Cuttaia;G. D'Alessandro;A. D. Silva;R. Davis;M. D. Avillez;P. D. Bernardis;M. D. Petris;A. D. Rosa;G. D. Zotti;J. Delabrouille;F. C. X. Désert;C. Dickinson;J. M. Diego;J. Dunkley;T. Enßlin;J. Errard;E. Falgarone;P. Ferreira;K. Ferrière;F. Finelli;A. Fletcher;P. Fosalba;G. Fuller;S. Galli;K. Ganga;J. García Bellido;A. Ghribi;M. Giard;Y. Giraud Héraud;J. Gonzalez Nuevo;K. Grainge;A. Gruppuso;A. Hall;J. C. Hamilton;M. Haverkorn;C. Hernandez Monte Agudo;D. Herranz;M. Jackson;A. Jaffe;R. Khatri;M. Kunz;L. Lamagna;M. Lattanzi;P. Leahy;J. Lesgourgues;M. Liguori;E. Liuzzo;M. Lopez Caniego;J. Macias Perez;B. Maffei;D. Maino;A. Mangilli;E. Martinez Gonzalez;C. Martins;S. Masi;M. Massardi;S. Matarrese;A. Melchiorri;J. B. Melin;A. Mennella;A. Mignano;M. A. Miville Deschênes;A. Monfardini;A. Murphy;P. Naselsky;F. Nati;P. Natoli;M. Negrello;F. Noviello;C. O'Sullivan;F. Paci;L. Pagano;R. Paladino;N. Palanque Delabrouille;D. Paoletti;H. Peiris;F. Perrotta;F. Piacentini;M. Piat;L. Piccirillo;G. Pisano;G. Polenta;A. Pollo;N. Ponthieu;M. Remazeilles;S. Ricciardi;M. Roman;C. Rosset;J. A. Rubino Martin;M. Salatino;A. Schillaci;P. Shellard;J. Silk;A. Starobinsky;R. Stompor;R. Sunyaev;A. Tartari;L. Terenzi;L. Toffolatti;M. Tomasi;N. Trappe;M. Tristram;T. Trombetti;M. Tucci;R. V. D. Weijgaert;B. V. Tent;L. Verde;P. Vielva;B. Wandelt;R. Watson;S. Withington
2014
Abstract
PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Vision program a set of important scientific questions that require high resolution, high sensitivity, full-sky observations of the sky emission at wavelengths ranging from millimeter-wave to the far-infrared. PRISM's main objective is to explore the distant universe, probing cosmic history from very early times until now as well as the structures, distribution of matter, and velocity flows throughout our Hubble volume. PRISM will survey the full sky in a large number of frequency bands in both intensity and polarization and will measure the absolute spectrum of sky emission more than three orders of magnitude better than COBE FIRAS. The aim of this Extended White Paper is to provide a more detailed overview of the highlights of the new science that will be made possible by PRISM
PRISM (Polarized radiation imaging and spectroscopy mission) : an extended white paper / P. André, C. Baccigalupi, A. Banday, D. Barbosa, B. Barreiro, J. Bartlett, N. Bartolo, E. Battistelli, R. Battye, G. Bendo, A. Benoît, J.P. Bernard, M. Bersanelli, M. Béthermin, P. Bielewicz, A. Bonaldi, F.C. Bouchet, F.C. Boulanger, J. Brand, M. Bucher, C. Burigana, Z.Y. Cai, P. Camus, F. Casas, V. Casasola, G. Castex, A. Challinor, J. Chluba, G. Chon, S. Colafrancesco, B. Comis, F. Cuttaia, G. D'Alessandro, A.D. Silva, R. Davis, M.D. Avillez, P.D. Bernardis, M.D. Petris, A.D. Rosa, G.D. Zotti, J. Delabrouille, F.C.X. Désert, C. Dickinson, J.M. Diego, J. Dunkley, T. Enßlin, J. Errard, E. Falgarone, P. Ferreira, K. Ferrière, F. Finelli, A. Fletcher, P. Fosalba, G. Fuller, S. Galli, K. Ganga, J. García-Bellido, A. Ghribi, M. Giard, Y. Giraud-Héraud, J. Gonzalez-Nuevo, K. Grainge, A. Gruppuso, A. Hall, J.C. Hamilton, M. Haverkorn, C. Hernandez-Monte-Agudo, D. Herranz, M. Jackson, A. Jaffe, R. Khatri, M. Kunz, L. Lamagna, M. Lattanzi, P. Leahy, J. Lesgourgues, M. Liguori, E. Liuzzo, M. Lopez-Caniego, J. Macias-Perez, B. Maffei, D. Maino, A. Mangilli, E. Martinez-Gonzalez, C. Martins, S. Masi, M. Massardi, S. Matarrese, A. Melchiorri, J.B. Melin, A. Mennella, A. Mignano, M.A. Miville-Deschênes, A. Monfardini, A. Murphy, P. Naselsky, F. Nati, P. Natoli, M. Negrello, F. Noviello, C. O'Sullivan, F. Paci, L. Pagano, R. Paladino, N. Palanque-Delabrouille, D. Paoletti, H. Peiris, F. Perrotta, F. Piacentini, M. Piat, L. Piccirillo, G. Pisano, G. Polenta, A. Pollo, N. Ponthieu, M. Remazeilles, S. Ricciardi, M. Roman, C. Rosset, J.A. Rubino-Martin, M. Salatino, A. Schillaci, P. Shellard, J. Silk, A. Starobinsky, R. Stompor, R. Sunyaev, A. Tartari, L. Terenzi, L. Toffolatti, M. Tomasi, N. Trappe, M. Tristram, T. Trombetti, M. Tucci, R.V.D. Weijgaert, B.V. Tent, L. Verde, P. Vielva, B. Wandelt, R. Watson, S. Withington. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - 2014:2(2014 Feb 05), pp. 006.1-006.68. [10.1088/1475-7516/2014/02/006]
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P. André, C. Baccigalupi, A. Banday, D. Barbosa, B. Barreiro, J. Bartlett, N. Bartolo, E. Battistelli, R. Battye, G. Bendo, A. Benoît, J.P. Bernard, M. Bersanelli, M. Béthermin, P. Bielewicz, A. Bonaldi, F.C. Bouchet, F.C. Boulanger, J. Brand, M. Bucher, C. Burigana, Z.Y. Cai, P. Camus, F. Casas, V. Casasola, G. Castex, A. Challinor, J. Chluba, G. Chon, S. Colafrancesco, B. Comis, F. Cuttaia, G. D'Alessandro, A.D. Silva, R. Davis, M.D. Avillez, P.D. Bernardis, M.D. Petris, A.D. Rosa, G.D. Zotti, J. Delabrouille, F.C.X. Désert, C. Dickinson, J.M. Diego, J. Dunkley, T. Enßlin, J. Errard, E. Falgarone, P. Ferreira, K. Ferrière, F. Finelli, A. Fletcher, P. Fosalba, G. Fuller, S. Galli, K. Ganga, J. García Bellido, A. Ghribi, M. Giard, Y. Giraud Héraud, J. Gonzalez Nuevo, K. Grainge, A. Gruppuso, A. Hall, J.C. Hamilton, M. Haverkorn, C. Hernandez Monte Agudo, D. Herranz, M. Jackson, A. Jaffe, R. Khatri, M. Kunz, L. Lamagna, M. Lattanzi, P. Leahy, J. Lesgourgues, M. Liguori, E. Liuzzo, M. Lopez Caniego, J. Macias Perez, B. Maffei, D. Maino, A. Mangilli, E. Martinez Gonzalez, C. Martins, S. Masi, M. Massardi, S. Matarrese, A. Melchiorri, J.B. Melin, A. Mennella, A. Mignano, M.A. Miville Deschênes, A. Monfardini, A. Murphy, P. Naselsky, F. Nati, P. Natoli, M. Negrello, F. Noviello, C. O'Sullivan, F. Paci, L. Pagano, R. Paladino, N. Palanque Delabrouille, D. Paoletti, H. Peiris, F. Perrotta, F. Piacentini, M. Piat, L. Piccirillo, G. Pisano, G. Polenta, A. Pollo, N. Ponthieu, M. Remazeilles, S. Ricciardi, M. Roman, C. Rosset, J.A. Rubino Martin, M. Salatino, A. Schillaci, P. Shellard, J. Silk, A. Starobinsky, R. Stompor, R. Sunyaev, A. Tartari, L. Terenzi, L. Toffolatti, M. Tomasi, N. Trappe, M. Tristram, T. Trombetti, M. Tucci, R.V.D. Weijgaert, B.V. Tent, L. Verde, P. Vielva, B. Wandelt, R. Watson, S. Withington
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/255750
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Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande.
