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Title
We demonstrate that, for the baseline design of the CORE satellite mission, the polarized foregrounds can be controlled at the level required to allow the detection of the primordial cosmic microwave background (CMB) B-mode polarization with the desi...
Sekimoto, Yutaro;Ade, P;Arnold, K;Aumont, J;Austermann, J;Baccigalupi, C;Banday, A;Banerji, Ranajoy;Basak, S;Beckman, S;Bersanelli, M;Borrill, J;Boulanger, F;Brown, ML;Bucher, M;Calabrese, E;Challinor, A;Chinone, Y;Columbro, F;Cukierman, A;Curtis, D;de Bernardis, P;de Petris, M;Dobbs, M;Dotani, T;Duband, L;Ducout, A;Ebisawa, K;Elleflot, T;Eriksen, Hans Kristian Kamfjord;Errard, J;Flauger, R;Franceschet, C;Fuskeland, Unni;Ganga, K;Gao, RJ;Ghigna, T;Grain, J;Gruppuso, A;Halverson, N;Hargrave, P;Hasebe, T;Hasegawa, M;Hattori, M;Hazumi, M;Henrot-Versille, S;Hill, C;Hirota, Y;Hivon, E;Hoang, TD;Hubmayr, J;Ichiki, K;Imada, H;Ishino, H;Jaehnig, G;Kanai, H;Kashima, S;Kataoka, Y;Katayama, N;Kawasaki, T;Keskitalo, R;Kibayashi, A;Kikuchi, T;Kimura, K;Kisner, T;Kobayashi, Y;Kogiso, N;Kohri, K;Komatsu, E;Komatsu, K;Konishi, K;Krachmalnicoff, N;Kuo, LC;Kurinsky, N;Kushino, A;Lamagna, L;Lee, TA;Linder, E;Maffei, B;Maki, M;Mangilli, A;Martinez-Gonzalez, E;Masi, S;Matsumura, T;Mennella, A;Minami, Y;Mistuda, K;Molinari, D;Montier, L;Morgante, G;Mot, B;Murata, Y;Murphy, A;Nagai, M;Nagata, R;Nakamura, S;Namikawa, T;Natoli, P;Nishibori, T;Nishino, H;Noviello, F;O'Sullivan, C;Ochi, H;Ogawa, H;Ohsaki, H;Ohta, I;Okada, N;Patanchon, G;Piacentini, F;Pisano, G;Polenta, G;Poletti, D;Puglisi, G;Raum, C;Realini, S;Remazeilles, M;Sakurai, H;Sakurai, Y;Savini, G;Sherwin, B;Shinozaki, K;Shiraishi, M;Signorelli, G;Smecher, G;Stompor, R;Sugai, H;Sugiyama, S;Suzuki, A;Suzuki, J;Takaku, R;Takakura, H;Takakura, S;Taylor, E;Terao, Y;Thompson, KL;Thorne, B;Tomasi, M;Tomida, H;Trappe, N;Tristram, M;Tsuji, M;Tsujimoto, M;Uozumi, S;Utsunomiya, S;Vittorio, N;Watanabe, N;Wehus, Ingunn Kathrine;Westbrook, B;Winter, B;Yamamoto, R;Yamasaki, N;Yanagisawa, M;Yoshida, T;Yumoto, J;Zannoni, M;Zonca, A
LiteBIRD is a candidate for JAXA’s strategic large mission to observe the cosmic microwave background (CMB) polarization over the full sky at large angular scales. It is planned to be launched in the 2020s with an H3 launch vehicle for three years of...
Hasebe, T;Kashima, S;Ade, PAR;Akiba, Y;Alonso, D;Arnold, K;Aumont, J;Baccigalupi, C;Barron, D;Basak, S;Beckman, S;Borrill, J;Boulanger, F;Bucher, M;Calabrese, E;Chinone, Y;Cho, H-M;Cukierman, A;Curtis, DW;De Haan, T;Dobbs, M;Dominjon, A;Dotani, T;Duband, L;Ducout, A;Dunkley, J;Duval, JM;Elleflot, T;Eriksen, HK;Errard, J;Fischer, J;Fujino, T;Funaki, T;Fuskeland, U;Ganga, K;Goeckner-Wald, N;Grain, J;Halverson, NW;Hamada, T;Hasegawa, M;Hattori, K;Hattori, M;Hayes, L;Hazumi, M;Hidehira, N;Hill, CA;Hilton, G;Hubmayr, J;Ichiki, K;Iida, T;Imada, H;Inoue, M;Inoue, Y;Irwin, KD;Ishino, H;Jeong, O;Kanai, H;Kaneko, D;Katayama, N;Kawasaki, T;Kernasovskiy, SA;Keskitalo, R;Kibayashi, A;Kida, Y;Kimura, K;Kisner, T;Kohri, K;Komatsu, E;Komatsu, K;Kuo, CL;Kurinsky, NA;Kusaka, A;Lazarian, A;Lee, AT;Li, D;Linder, E;Maffei, B;Mangilli, A;Maki, M;Matsumura, T;Matsuura, S;Meilhan, D;Mima, S;Minami, Y;Mitsuda, K;Montier, L;Nagai, M;Nagasaki, T;Nagata, R;Nakajima, M;Nakamura, S;Namikawa, T;Naruse, M;Nishino, H;Nitta, T;Noguchi, T;Ogawa, H;Oguri, S;Okada, N;Okamoto, A;Okamura, T;Otani, C;Patanchon, G;Pisano, G;Rebeiz, G;Remazeilles, M;Richards, PL;Sakai, S;Sakurai, Y;Sato, Y;Sato, N;Sawada, M;Segawa, Y;Sekimoto, Y;Seljak, U;Sherwin, BD;Shimizu, T;Shinozaki, K;Stompor, R;Sugai, H;Sugita, H;Suzuki, A;Suzuki, J;Tajima, O;Takada, S;Takaku, R;Takakura, S;Takatori, S;Tanabe, D;Taylor, E;Thompson, KL;Thorne, B;Tomaru, T;Tomida, T;Tomita, N;Tristram, M;Tucker, C;Turin, P;Tsujimoto, M;Uozumi, S;Utsunomiya, S;Uzawa, Y;Vansyngel, F;Wehus, IK;Westbrook, B;Willer, M;Whitehorn, N;Yamada, Y;Yamamoto, R;Yamasaki, N;Yamashita, T;Yoshida, M
The high-frequency telescope for LiteBIRD is designed with refractive and reflective optics. In order to improve sensitivity, this paper suggests the new optical configurations of the HFT which have approximately 7 times larger focal planes than that...
orcid:0000-0002-8490-8117;orcid:0000-0001-6740-5350;orcid:0000-0003-2226-9169;orcid:0000-0002-5193-516X;orcid:0000-0002-1851-3918;orcid:0000-0002-7614-6677;orcid:0000-0002-7567-4451;Ade, P;Aguirre, J;Ahmed, Z;Aiola, S;Ali, A;Alonso, D;Alvarez, MA;Arnold, K;Ashton, P;Austermann, J;Awan, H;Baccigalupi, C;Baildon, T;Barron, D;Battaglia, N;Battye, R;Baxter, E;Bazarko, A;Beall, JA;Bean, R;Beck, D;Beckman, S;Beringue, B;Bianchini, F;Boada, S;Boettger, D;Bond, JR;Borrill, J;Brown, ML;Bruno, SM;Bryan, S;Calabrese, E;Calafut, V;Calisse, P;Carron, J;Challinor, A;Chesmore, G;Chinone, Y;Chluba, J;Cho, H-MS;Choi, S;Coppi, G;Cothard, NF;Coughlin, K;Crichton, D;Crowley, KD;Crowley, KT;Cukierman, A;D'Ewart, JM;Dunner, R;de Haan, T;Devlin, M;Dicker, S;Didier, J;Dobbs, M;Dober, B;Duell, CJ;Duff, S;Duivenvoorden, A;Dunkley, J;Dusatko, J;Errard, J;Fabbian, G;Feeney, S;Ferraro, S;Fluxa, P;Freese, K;Frisch, JC;Frolov, A;Fuller, G;Fuzia, B;Galitzki, N;Gallardo, PA;Ghersi, JTG;Gao, J;Gawiser, E;Gerbino, M;Gluscevic, V;Goeckner-Wald, N;Golec, J;Gordon, S;Gralla, M;Green, D;Grigorian, A;Groh, J;Groppi, C;Guan, Y;Gudmundsson, JE;Han, D;Hargrave, P;Hasegawa, M;Hasselfield, M;Hattori, M;Haynes, V;Hazumi, M;He, Y;Healy, E;Henderson, SW;Hervias-Caimapo, C;Hill, CA;Hill, JC;Hilton, G;Hilton, M;Hincks, AD;Hinshaw, G;Hlozek, R;Ho, S;Ho, S-PP;Howe, L;Huang, Z;Hubmayr, J;Huffenberger, K;Hughes, JP;Ijjas, A;Ikape, M;Irwin, K;Jaffe, AH;Jain, B;Jeong, O;Kaneko, D;Karpel, ED;Katayama, N;Keating, B;Kernasovskiy, SS;Keskitalo, R;Kisner, T;Kiuchi, K;Klein, J;Knowles, K;Koopman, B;Kosowsky, A;Krachmalnicoff, N;Kuenstner, SE;Kuo, C-L;Kusaka, A;Lashner, J;Lee, A;Lee, E;Leon, D;Leung, JS-Y;Lewis, A;Li, Y;Li, Z;Limon, M;Linder, E;Lopez-Caraballo, C;Louis, T;Lowry, L;Lungu, M;Madhavacheril, M;Mak, D;Maldonado, F;Mani, H;Mates, B;Matsuda, F;Maurin, L;Mauskopf, P;May, A;McCallum, N;McKenney, C;McMahon, J;Meerburg, PD;Meyers, J;Miller, A;Mirmelstein, M;Moodley, K;Munchmeyer, M;Munson, C;Naess, S;Nati, F;Navaroli, M;Newburgh, L;Ho, NN;Niemack, M;Nishino, H;Orlowski-Scherer, J;Page, L;Partridge, B;Peloton, J;Perrotta, F;Piccirillo, L;Pisano, G;Poletti, D;Puddu, R;Puglisi, G;Raum, C;Reichardt, CL;Remazeilles, M;Rephaeli, Y;Riechers, D;Rojas, F;Roy, A;Sadeh, S;Sakurail, Y;Salatino, M;Rao, MS;Schaan, E;Schmittfull, M;Sehgal, N;Seibert, J;Seljak, U;Sherwin, B;Shimon, M;Sierra, C;Sievers, J;Sikhosana, P;Silva-Feaver, M;Simon, SM;Sinclair, A;Siritanasak, P;Smith, K;Smith, SR;Spergel, D;Staggs, ST;Stein, G;Stevens, JR;Stompor, R;Suzuki, A;Tajima, O;Takakura, S;Teply, G;Thomas, DB;Thorne, B;Thornton, R;Trac, H;Tsai, C;Tucker, C;Ullom, J;Vagnozzi, S;van Engelen, A;Van Lanen, J;Van Winkle, DD;Vavagiakis, EM;Verges, C;Vissers, M;Wagoner, K;Walker, S;Ward, J;Westbrook, B;Whitehorn, N;Williams, J;Williams, J;Wollack, EJ;Xu, Z;Yu, B;Yu, C;Zago, F;Zhang, H;Zhu, N
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Sekimoto, Y.;Ade, P.;Arnold, K.;Aumont, J.;Austermann, J.;Baccigalupi, C.;Banday, A.;Banerji, R.;Basak, S.;Beckman, S.;Bersanelli, M.;Borrill, J.;Boulanger, F.;Brown, M. L.;Bucher, M.;Calabrese, E.;Casas, F. J.;Challinor, A.;Chinone, Y.;Columbro, F.;Cukierman, A.;Curtis, D.;De Bernardis, P.;De Petris, M.;Dobbs, M.;Dotani, T.;Duband, L.;Duval, J. M.;Ducout, A.;Ebisawa, K.;Elleot, T.;Eriksen, H.;Errard, J.;Flauger, R.;Franceschet, C.;Fuskeland, U.;Ganga, K.;Gao, R. J.;Ghigna, T.;Grain, J.;Gruppuso, A.;Halverson, N.;Hargrave, P.;Hasebe, T.;Hasegawa, M.;Hattori, M.;Hazumi, M.;Henrot-Versille, S.;Hill, C.;Hirota, Y.;Hivon, E.;Hoang, T. D.;Hubmayr, J.;Ichiki, K.;Imada, H.;Ishino, H.;Jaehnig, G.;Kanai, H.;Kashima, S.;Kataoka, Y.;Katayama, N.;Kawasaki, T.;Keskitalo, R.;Kibayashi, A.;Kikuchi, T.;Kimura, K.;Kisner, T.;Kobayashi, Y.;Kogiso, N.;Kohri, K.;Komatsu, Eiichiro;Komatsu, K.;Konishi, K.;Krachmalnicoff, N.;Kuo, L. C.;Kurinsky, N.;Kushino, A.;Lamagna, L.;Lee, T. A.;Linder, E.;Maffei, B.;Maki, M.;Mangilli, A.;Martinez-Gonzalez, E.;Masi, S.;Matsumura, T.;Mennella, A.;Minami, Y.;Mistuda, K.;Molinari, D.;Montier, L.;Morgante, G.;Mot, B.;Murata, Y.;Murphy, A.;Nagai, M.;Nagata, R.;Nakamura, S.;Namikawa, T.;Natoli, P.;Nishibori, T.;Nishino, H.;Noviello, F.;O'Sullivan, C.;Ochi, H.;Ogawa, H.;Ogawa, H.;Ohsaki, H.;Ohta, I.;Okada, N.;Patanchon, G.;Piacentini, F.;Pisano, G.;Polenta, G.;Poletti, D.;Puglisi, G.;Raum, C.;Realini, S.;Remazeilles, M.;Sakurai, H.;Sakurai, Y.;Savini, G.;Sherwin, B.;Shinozaki, K.;Shiraishi, M.;Signorelli, G.;Smecher, G.;Stompor, R.;Sugai, H.;Sugiyama, S.;Suzuki, A.;Suzuki, J.;Takaku, R.;Takakura, H.;Takakura, S.;Taylor, E.;Terao, Y.;Thompson, K. L.;Thorne, B.;Tomasi, M.;Tomida, H.;Trappe, N.;Tristram, M.;Tsuji, M.;Tsujimoto, M.;Uozumi, S.;Utsunomiya, S.;Vittorio, N.;Watanabe, N.;Wehus, I.;Westbrook, B.;Winter, B.;Yamamoto, R.;Yamasaki, N.;Yanagisawa, M.;Yoshida, T.;Yumoto, J.;Zannoni, M.;Zonca, A.
LiteBIRD is a candidate for JAXA's strategic large mission to observe the cosmic microwave background (CMB) polarization over the full sky at large angular scales. It is planned to be launched in the 2020s with an H3 launch vehicle for three years of...
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.;Matarrese, 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.
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...
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.;Benoít, 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.;Silva, A. da;de Avillez, M.;de Gasperis, G.;Petris, M. De;de Zotti, G.;Danese, L.;Désert, F. -X.;Desjacques, V.;Valentino, E. Di;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.;Rubiño-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.;de Weygaert, R. Van;Tent, B. Van;Vennin, V.;Verde, L.;Vermeulen, G.;Vielva, P.;Vittorio, N.;Voisin, F.;Wallis, C.;Wandelt, B.;Wehus, I. K.;Weller, J.;Young, K.;Zannoni, M.
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 ad...
André, Patrice Charles Maxime;Baccigalupi, Carlo;Banday, A;Barbosa, D;Barreiro, B;Bartlett, J;Bartolo, Nicola;Battistelli, E;Battye, R;Bendo, G;Benoit, A;Bernard, Jp;Bersanelli, M;Bethermin, Matthieu Michel;Bielewicz, Pawel;Bonaldi, Anna Valentina;Bouchet, Freddy;Boulanger, Francois Bernard Marie;Brand, J;Bucher, Mario;Burigana, Carlo;Cai, Zy;Camus, P;Casas, F;Casasola, V;Castex, Guillaume Jean Serge;Challinor, A;Chluba, J;Chon, G;Colafrancesco, S;Comis, B;Cuttaia, F;D'Alessandro, G;Da Silva, A;Davis, R;De Avillez, M;De Bernardis, P;De Petris, M;De Rosa, A;De Zotti, Gianfranco;Delabrouille, J;Desert, Fx;Dickinson, C;Diego, Jm;Dunkley, J;Ensslin, T;Errard, J;Falgarone, E;Ferreira, P;Ferriere, K;Finelli, F;Fletcher, A;Fosalba, P;Fuller, G;Galli, S;Ganga, K;Garcia-bellido, J;Ghribi, A;Giard, M;Giraud-heraud, Y;Gonzalez-nuevo, J;Grainge, K;Gruppuso, A;Hall, A;Hamilton, Jc;Haverkorn, M;Hernandez-monteagudo, C;Herranz, D;Jackson, M;Jaffe, Andrew Howard;Khatri, R;Kunz, M;Lamagna, L;Lattanzi, M;Leahy, P;Lesgourgues, J;Liguori, M;Liuzzo, E;Lopez-caniego, M;Macias-perez, J;Maffei, B;Maino, Davide;Mangilli, A;Martinez-gonzalez, E;Martins, C;Masi, S;Massardi, Marcella;Matarrese, Sabino;Melchiorri, A;Melin, Jb;Mennella, Aniello;Mignano, A;Miville-deschenes, Ma;Monfardini, A;Murphy, A;Naselsky, P;Nati, F;Natoli, Paolo;Negrello, Mattia;Noviello, F;O'Sullivan, C;Paci, Francesco;Pagano, L;Paladino, R;Palanque-delabrouille, N;Paoletti, D;Peiris, H;Perrotta, Francesca;Piacentini, Francesco;Piat, M;Piccirillo, L;Pisano, G;Polenta, G;Pollo, A;Ponthieu, N;Remazeilles, M;Ricciardi, S;Roman, M;Rosset, C;Rubino-martin, Ja;Salatino, M;Schillaci, A;Shellard, P;Silk, J;Starobinsky, A;Stompor, Radoslaw;Sunyaev, R;Tartari, A;Terenzi, L;Toffolatti, L;Tomasi, M;Trappe, N;Tristram, M;Trombetti, T;Tucci, M;Van De Weijgaert, R;Van Tent, B;Verde, Licia;Vielva, P;Wandelt, B;Watson, R;Withington, S.
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 re...
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