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Planck intermediate results
- Adam, R;
- Ade, PAR;
- Aghanim, N;
- Arnaud, M;
- Aumont, J;
- Baccigalupi, C;
- Banday, AJ;
- Barreiro, RB;
- Bartlett, JG;
- Bartolo, N;
- Battaner, E;
- Benabed, K;
- Benoit-Lévy, A;
- Bernard, J-P;
- Bersanelli, M;
- Bielewicz, P;
- Bonaldi, A;
- Bonavera, L;
- Bond, JR;
- Borrill, J;
- Bouchet, FR;
- Boulanger, F;
- Bracco, A;
- Bucher, M;
- Burigana, C;
- Butler, RC;
- Calabrese, E;
- Cardoso, J-F;
- Catalano, A;
- Challinor, A;
- Chamballu, A;
- Chary, R-R;
- Chiang, HC;
- Christensen, PR;
- Clements, DL;
- Colombi, S;
- Colombo, LPL;
- Combet, C;
- Couchot, F;
- Coulais, A;
- Crill, BP;
- Curto, A;
- Cuttaia, F;
- Danese, L;
- Davies, RD;
- Davis, RJ;
- de Bernardis, P;
- de Zotti, G;
- Delabrouille, J;
- Delouis, J-M;
- Désert, F-X;
- Dickinson, C;
- Diego, JM;
- Dolag, K;
- Dole, H;
- Donzelli, S;
- Doré, O;
- Douspis, M;
- Ducout, A;
- Dunkley, J;
- Dupac, X;
- Efstathiou, G;
- Elsner, F;
- Enßlin, TA;
- Eriksen, HK;
- Falgarone, E;
- Finelli, F;
- Forni, O;
- Frailis, M;
- Fraisse, AA;
- Franceschi, E;
- Frejsel, A;
- Galeotta, S;
- Galli, S;
- Ganga, K;
- Ghosh, T;
- Giard, M;
- Giraud-Héraud, Y;
- Gjerløw, E;
- González-Nuevo, J;
- Górski, KM;
- Gratton, S;
- Gregorio, A;
- Gruppuso, A;
- Guillet, V;
- Hansen, FK;
- Hanson, D;
- Harrison, DL;
- Helou, G;
- Henrot-Versillé, S;
- Hernández-Monteagudo, C;
- Herranz, D;
- Hivon, E;
- Hobson, M;
- Holmes, WA;
- Huffenberger, KM;
- Hurier, G;
- Jaffe, AH;
- Jaffe, TR;
- Jewell, J;
- Jones, WC;
- Juvela, M;
- Keihänen, E;
- Keskitalo, R;
- Kisner, TS;
- Kneissl, R;
- Knoche, J;
- Knox, L;
- Krachmalnicoff, N;
- Kunz, M;
- Kurki-Suonio, H;
- Lagache, G;
- Lamarre, J-M;
- Lasenby, A;
- Lattanzi, M;
- Lawrence, CR;
- Leahy, JP;
- Leonardi, R;
- Lesgourgues, J;
- Levrier, F;
- Liguori, M;
- Lilje, PB;
- Linden-Vørnle, M;
- López-Caniego, M;
- Lubin, PM;
- Macías-Pérez, JF;
- Maffei, B;
- Maino, D;
- Mandolesi, N;
- Mangilli, A;
- Maris, M;
- Martin, PG;
- Martínez-González, E;
- Masi, S;
- Matarrese, S;
- Mazzotta, P;
- Meinhold, PR;
- Melchiorri, A;
- Mendes, L;
- Mennella, A;
- Migliaccio, M;
- Mitra, S;
- Miville-Deschênes, M-A;
- Moneti, A;
- Montier, L;
- Morgante, G;
- Mortlock, D;
- Moss, A;
- Munshi, D;
- Murphy, JA;
- Naselsky, P;
- Nati, F;
- Natoli, P;
- Netterfield, CB;
- Nørgaard-Nielsen, HU;
- Noviello, F;
- Novikov, D;
- Novikov, I;
- Pagano, L;
- Pajot, F;
- Paladini, R;
- Paoletti, D;
- Partridge, B;
- Pasian, F;
- Patanchon, G;
- Pearson, TJ;
- Perdereau, O;
- Perotto, L;
- Perrotta, F;
- Pettorino, V;
- Piacentini, F;
- Piat, M;
- Pierpaoli, E;
- Pietrobon, D;
- Plaszczynski, S;
- Pointecouteau, E;
- Polenta, G;
- Ponthieu, N;
- Popa, L;
- Pratt, GW;
- Prunet, S;
- Puget, J-L;
- Rachen, JP;
- Reach, WT;
- Rebolo, R;
- Remazeilles, M;
- Renault, C;
- Renzi, A;
- Ricciardi, S;
- Ristorcelli, I;
- Rocha, G;
- Rosset, C;
- Rossetti, M;
- Roudier, G;
- Rouillé d’Orfeuil, B;
- Rubiño-Martín, JA;
- Rusholme, B;
- Sandri, M;
- Santos, D;
- Savelainen, M;
- Savini, G;
- Scott, D;
- Soler, JD;
- Spencer, LD;
- Stolyarov, V;
- Stompor, R;
- Sudiwala, R;
- Sunyaev, R;
- Sutton, D;
- Suur-Uski, A-S;
- Sygnet, J-F;
- Tauber, JA;
- Terenzi, L;
- Toffolatti, L;
- Tomasi, M;
- Tristram, M;
- Tucci, M;
- Tuovinen, J;
- Valenziano, L;
- Valiviita, J;
- Van Tent, B;
- Vibert, L;
- Vielva, P;
- Villa, F;
- Wade, LA;
- Wandelt, BD;
- Watson, R;
- Wehus, IK;
- White, M;
- White, SDM;
- Yvon, D;
- Zacchei, A;
- Zonca, A
Published Web Location
https://doi.org/10.1051/0004-6361/201425034Abstract
The polarized thermal emission from diffuse Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 100 GHz. In this paper we exploit the uniqueness of the Planck HFI polarization data from 100 to 353 GHz to measure the polarized dust angular power spectra CℓEE and CℓBB over the multipole range 40
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