Browsing Institutt for teoretisk astrofysikk by Author "Polegre, AM"

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  • Planck 2013 results. VII. HFI time response and beams 
    Ade, P. A. R.; Aghanim, N; Armitage-Caplan, C; Arnaud, M; Ashdown, M; Atrio-Barandela, F; Aumont, J; Baccigalupi, C; Banday, AJ; Barreiro, RB; Battaner, E; Benabed, K; Benoit, A; Benoit-Levy, A; Bernard, JP; Bersanelli, M; Bielewicz, P; Bobin, J; Bock, JJ; Bond, JR; Borrill, J; Bouchet, FR; Bowyer, JW; Bridges, M; Bucher, M; Burigana, C; Cardoso, JF; Catalano, A; Challinor, A; Chamballu, A; Chary, RR; Chiang, HC; Chiang, LY; Christensen, PR; Church, S; Clements, DL; Colombi, S; Colombo, LPL; Couchot, F; Coulais, A; Crill, BP; Curto, A; Cuttaia, F; Danese, L; Davies, RD; De Bernardis, P; De Rosa, A; De Zotti, G; Delabrouille, J; Delouis, JM; Desert, FX; Diego, JM; Dole, H; Donzelli, S; Dore, O; Douspis, M; Dunkley, J; Dupac, X; Efstathiou, G; Enßlin, TA; Eriksen, Hans Kristian Kamfjord; Finelli, F; Forni, O; Frailis, M; Fraisse, AA; Franceschi, E; Galeotta, S; Ganga, K; Giard, M; Giraud-Heraud, Y; Gonzalez-Nuevo, J; Gorski, KM; Gratton, S; Gregorio, A; Gruppuso, A; Gudmundsson, JE; Haissinski, J; Hansen, Frode Kristian; Hanson, D; Harrison, D; Henrot-Versille, S; Hernandez-Monteagudo, C; Herranz, D; Hildebrandt, SR; Hivon, E; Hobson, M; Holmes, WA; Hornstrup, A; Hou, Z; Hovest, W; Huffenberger, KM; Jaffe, AH; Jaffe, TR; Jones, WC; Juvela, M; Keihänen, E; Keskitalo, R; Kisner, TS; Kneissl, R; Knoche, J; Knox, L; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, JM; Lasenby, A; Laureijs, RJ; Lawrence, CR; Leonardi, R; Leroy, C; Lesgourgues, J; Liguori, M; Lilje, Per Barth; Linden-Vørnle, M; Lopez-Caniego, M; Lubin, PM; MacIas-Perez, JF; MacTavish, CJ; Maffei, B; Mandolesi, N; Maris, M; Marshall, DJ; Martin, PG; Martinez-Gonzalez, E; Masi, S; Massardi, M; Matarrese, S; Matsumura, T; Matthai, F; Mazzotta, P; McGehee, P; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschenes, MA; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, JA; Naselsky, P; Nati, F; Natoli, P; Netterfield, CB; Nørgaard-Nielsen, HU; Noviello, F; Novikov, D; Novikov, I; Osborne, S; Oxborrow, CA; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Patanchon, G; Perdereau, O; Perotto, L; Perrotta, F; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polegre, AM; Polenta, G; Ponthieu, N; Popa, L; Poutanen, T; Pratt, GW; Prezeau, G; Prunet, S; Puget, JL; Rachen, JP; Reinecke, M; Remazeilles, M; Renault, C; Ricciardi, S; Riller, T; Ristorcelli, I; Rocha, G; Rosset, C; Roudier, G; Rowan-Robinson, M; Rusholme, B; Sandri, M; Santos, D; Sauve, A; Savini, G; Scott, D; Shellard, EPS; Spencer, LD; Starck, JL; Stolyarov, V; Stompor, R; Sudiwala, R; Sureau, F; Sutton, D; Suur-Uski, AS; Sygnet, JF; Tauber, JA; Tavagnacco, D; Terenzi, L; Tomasi, M; Tristram, M; Tucci, M; Umana, G; Valenziano, L; Väliviita, Jussi-Pekka; Van Tent, B; Vielva, P; Villa, F; Vittorio, N; Wade, LA; Wandelt, BD; Yvon, D; Zacchei, A; Zonca, A (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
    This paper characterizes the effective beams, the effective beam window functions and the associated errors for the Planck High Frequency Instrument (HFI) detectors. The effective beam is theangular response including the ...
  • Planck 2013 results. XIV. Zodiacal emission 
    Ade, P. A. R.; Aghanim, N; Armitage-Caplan, C; Arnaud, M; Ashdown, M; Atrio-Barandela, F; Aumont, J; Baccigalupi, C; Banday, AJ; Barreiro, RB; Bartlett, JG; Battaner, E; Benabed, K; Benoit, A; Benoit-Levy, A; Bernard, JP; Bersanelli, M; Bielewicz, P; Bobin, J; Bock, JJ; Bonaldi, A; Bond, JR; Borrill, J; Bouchet, FR; Boulanger, F; Bridges, M; Bucher, M; Burigana, C; Butler, RC; Cardoso, JF; Catalano, A; Chamballu, A; Chary, RR; Chen, X; Chiang, HC; Chiang, LY; Christensen, PR; Church, S; Clements, DL; Colley, JM; Colombi, S; Colombo, LPL; Couchot, F; Coulais, A; Crill, BP; Curto, A; Cuttaia, F; Danese, L; Davies, RD; De Bernardis, P; De Rosa, A; De Zotti, G; Delabrouille, J; Delouis, JM; Desert, FX; Dickinson, C; Diego, JM; Dole, H; Donzelli, S; Dore, O; Douspis, M; Dupac, X; Efstathiou, G; Enßlin, TA; Eriksen, Hans Kristian Kamfjord; Finelli, F; Forni, O; Frailis, M; Fraisse, AA; Franceschi, E; Galeotta, S; Ganga, K; Giard, M; Giraud-Heraud, Y; Gonzalez-Nuevo, J; Gorski, KM; Gratton, S; Gregorio, A; Gruppuso, A; Hansen, Frode Kristian; Hanson, D; Harrison, D; Helou, G; Henrot-Versille, S; Hernandez-Monteagudo, C; Herranz, D; Hildebrandt, SR; Hivon, E; Hobson, M; Holmes, WA; Hornstrup, A; Hovest, W; Huffenberger, KM; Jaffe, AH; Jaffe, TR; Jones, WC; Juvela, M; Keihänen, E; Keskitalo, R; Kisner, TS; Kneissl, R; Knoche, J; Knox, L; Kunz, M; Kurki-Suonio, H; Lagache, G; Lähteenmäki, A; Lamarre, JM; Lasenby, A; Laureijs, RJ; Lawrence, CR; Leonardi, R; Lesgourgues, J; Liguori, M; Lilje, Per Barth; Linden-Vørnle, M; Lopez-Caniego, M; Lubin, PM; MacIas-Perez, JF; Maffei, B; Maino, D; Mandolesi, N; Maris, M; Marshall, DJ; Martin, PG; Martinez-Gonzalez, E; Masi, S; Massardi, M; Matarrese, S; Matthai, F; Mazzotta, P; Meinhold, PR; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschenes, MA; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Mottet, S; Munshi, D; Murphy, JA; Naselsky, P; Nati, F; Natoli, P; Netterfield, CB; Nørgaard-Nielsen, HU; Noviello, F; Novikov, D; Novikov, I; Osborne, S; O'Sullivan, C; Oxborrow, CA; Paci, F; Pagano, L; Pajot, F; Paladini, R; Paoletti, D; Pasian, F; Patanchon, G; Perdereau, O; Perotto, L; Perrotta, F; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polegre, AM; Polenta, G; Ponthieu, N; Popa, L; Poutanen, T; Pratt, GW; Prezeau, G; Prunet, S; Puget, JL; Rachen, JP; Reach, WT; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Ricciardi, S; Riller, T; Ristorcelli, I; Rocha, G; Rosset, C; Roudier, G; Rowan-Robinson, M; Rusholme, B; Sandri, M; Santos, D; Savini, G; Scott, D; Seiffert, MD; Shellard, EPS; Smoot, GF; Spencer, LD; Starck, JL; Stolyarov, V; Stompor, R; Sudiwala, R; Sureau, F; Sutton, D; Suur-Uski, AS; Sygnet, JF; Tauber, JA; Tavagnacco, D; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Umana, G; Valenziano, L; Väliviita, Jussi-Pekka; Van Tent, B; Vielva, P; Villa, F; Vittorio, N; Wade, LA; Wandelt, BD; Yvon, D; Zacchei, A; Zonca, A (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2014)
    The Planck satellite provides a set of all-sky maps at nine frequencies from 30 GHz to 857 GHz. Planets, minor bodies, and diffuse interplanetary dust emission (IPD) are all observed. The IPD can be separated from Galactic ...