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The Q/U Imaging ExperimenT (QUIET) employs coherent receivers at 43GHz and 95GHz, operating on the Chajnantor plateau in the Atacama Desert in Chile, to measure the anisotropy in the polarization of the CMB. QUIET primarily targets the B modes from p...
Collaboration, PRISM;André, P;Baccigalupi, C;Banday, A;Barbosa, D;Barreiro, B;Bartlett, J;Bartolo, N;Battistelli, E;Battye, R;Bendo, G;Benoît, A;Bernard, JP;Bersanelli, M;Béthermin, M;Bielewicz, P;Bonaldi, A;Bouchet, FC;Boulanger, FC;Brand, J;Bucher, M;Burigana, C;Cai, ZY;Camus, P;Casas, F;Casasola, V;Castex, G;Challinor, A;Chluba, J;Chon, G;Colafrancesco, S;Comis, B;Cuttaia, F;D'Alessandro, G;Silva, AD;Davis, R;Avillez, MD;Bernardis, PD;Petris, MD;Rosa, AD;Zotti, GD;Delabrouille, J;Désert, FCX;Dickinson, C;Diego, JM;Dunkley, J;Enßlin, T;Errard, J;Falgarone, E;Ferreira, P;Ferrière, K;Finelli, F;Fletcher, A;Fosalba, P;Fuller, G;Galli, S;Ganga, K;García-Bellido, J;Ghribi, A;Giard, M;Giraud-Héraud, Y;Gonzalez-Nuevo, J;Grainge, K;Gruppuso, A;Hall, A;Hamilton, JC;Haverkorn, M;Hernandez-Monte-agudo, C;Herranz, D;Jackson, M;Jaffe, A;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, D;Mangilli, A;Martinez-Gonzalez, E;Martins, C;Masi, S;Massardi, M;Matarrese, S;Melchiorri, A;Melin, JB;Mennella, A;Mignano, A;Miville-Deschênes, MA;Monfardini, A;Murphy, A;Naselsky, P;Nati, F;Natoli, P;Negrello, M;Noviello, F;O'Sullivan, C;Paci, F;Pagano, L;Paladino, R;Palanque-Delabrouille, N;Paoletti, D;Peiris, H;Perrotta, F;Piacentini, F;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, R;Sunyaev, R;Tartari, A;Terenzi, L;Toffolatti, L;Tomasi, M;Trappe, N;Tristram, M;Trombetti, T;Tucci, M;Weijgaert, RVD;Tent, BV;Verde, L;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...
We describe the design and expected performance of Clover, a new instrument designed to measure the B-mode polarization of the cosmic microwave background. The proposed instrument will comprise three independent telescopes operating at 90, 150 and 22...
The polarization of the atmosphere has been a long-standing concern for ground-based experiments targeting cosmic microwave background (CMB) polarization. Ice crystals in upper tropospheric clouds scatter thermal radiation from the ground and produce...
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
The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scientific goals of the experiment, motivate the design, and forecast its pe...
We constrain parity-violating interactions to the surface of last scattering using spectra from the QUaD experiment's second and third seasons of observations by searching for a possible systematic rotation of the polarization directions of cosmic mi...
Collaboration, PRISM;André, P;Baccigalupi, C;Banday, A;Barbosa, D;Barreiro, B;Bartlett, J;Bartolo, N;Battistelli, E;Battye, R;Bendo, G;Benoît, A;Bernard, JP;Bersanelli, M;Béthermin, M;Bielewicz, P;Bonaldi, A;Bouchet, FC;Boulanger, FC;Brand, J;Bucher, M;Burigana, C;Cai, ZY;Camus, P;Casas, F;Casasola, V;Castex, G;Challinor, A;Chluba, J;Chon, G;Colafrancesco, S;Comis, B;Cuttaia, F;D'Alessandro, G;Silva, AD;Davis, R;Avillez, MD;Bernardis, PD;Petris, MD;Rosa, AD;Zotti, GD;Delabrouille, J;Désert, FCX;Dickinson, C;Diego, JM;Dunkley, J;Enßlin, T;Errard, J;Falgarone, E;Ferreira, P;Ferrière, K;Finelli, F;Fletcher, A;Fosalba, P;Fuller, G;Galli, S;Ganga, K;García-Bellido, J;Ghribi, A;Giard, M;Giraud-Héraud, Y;Gonzalez-Nuevo, J;Grainge, K;Gruppuso, A;Hall, A;Hamilton, JC;Haverkorn, M;Hernandez-Monte-agudo, C;Herranz, D;Jackson, M;Jaffe, A;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, D;Mangilli, A;Martinez-Gonzalez, E;Martins, C;Masi, S;Massardi, M;Matarrese, S;Melchiorri, A;Melin, JB;Mennella, A;Mignano, A;Miville-Deschênes, MA;Monfardini, A;Murphy, A;Naselsky, P;Nati, F;Natoli, P;Negrello, M;Noviello, F;O'Sullivan, C;Paci, F;Pagano, L;Paladino, R;Palanque-Delabrouille, N;Paoletti, D;Peiris, H;Perrotta, F;Piacentini, F;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, R;Sunyaev, R;Tartari, A;Terenzi, L;Toffolatti, L;Tomasi, M;Trappe, N;Tristram, M;Trombetti, T;Tucci, M;Weijgaert, RVD;Tent, BV;Verde, L;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...
We describe the design and expected performance of Clover, a new instrument designed to measure the B-mode polarization of the cosmic microwave background. The proposed instrument will comprise three independent telescopes operating at 90, 150 and 22...
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
The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scientific goals of the experiment, motivate the design, and forecast its pe...
The polarization of the atmosphere has been a long-standing concern for ground-based experiments targeting cosmic microwave background (CMB) polarization. Ice crystals in upper tropospheric clouds scatter thermal radiation from the ground and produce...