Browsing Institutt for teoretisk astrofysikk by Author "Gregorio, A"

Now showing items 61-64 of 64

  • Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps 
    Ade, P. A. R.; Aghanim, N.; Alves, M. I. R.; Arnaud, M.; Arzoumanian, D.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Bartolo, N.; Battaner, E.; Benabed, K.; Benoit-Lévy, A.; Bernard, J.-P.; Berne, O.; Bersanelli, M.; Bielewicz, P.; Bonaldi, A.; Bonavera, L.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bracco, A.; Burigana, C.; Calabrese, E.; Cardoso, J.-F.; Catalano, A.; Chamballu, A.; Chiang, H. C.; Christensen, P. R.; Clements, D. L.; Colombi, S.; Colombo, L. P. L.; Combet, C.; Couchot, F.; Crill, B. P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; Davis, R. J.; de Bernardis, P.; de Rosa, A.; de Zotti, G.; Delabrouille, J.; Dickinson, C.; Diego, J. M.; Donzelli, Simona; Doré, O.; Douspis, M.; Ducout, A; Dupac, X; Elsner, F; Enßlin, TA; Eriksen, Hans Kristian Kamfjord; Falgarone, E; Ferriere, K; Finelli, F; Forni, O; Frailis, M; Fraisse, AA; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Ghosh, T; Giard, M; Giraud-Heraud, Y; Gjerløw, Eirik; Gonzalez-Nuevo, J; Gorski, KM; Gregorio, A; Gruppuso, A; Guillet, V; Hansen, Frode Kristian; Hanson, D; Harrison, DL; Hernandez-Monteagudo, C; Herranz, D; Hildebrandt, SR; Hivon, E; Hobson, M; Holmes, WA; Huffenberger, KM; Hurier, G; Jaffe, AH; Jaffe, TR; Jones, WC; Juvela, M; Keskitalo, R; Kisner, TS; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, JM; Lasenby, A; Lawrence, CR; Leonardi, R; Levrier, F; Liguori, M; Lilje, Per Barth; Linden-Vørnle, M; Lopez-Caniego, M; Lubin, PM; Macias-Perez, JF; Maffei, B; Mandolesi, N; Mangilli, A; Maris, M; Martin, PG; Martinez-Gonzalez, E; Masi, S; Matarrese, S; Mazzotta, 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; Nørgaard-Nielsen, HU; Noviello, F; Novikov, D; Novikov, I; Oppermann, N; Pagano, L; Pajot, F; Paladini, R; Paoletti, D; Pasian, F; Perrotta, F; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Pratt, GW; Puget, JL; Rachen, JP; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ricciardi, S; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rubino-Martin, JA; Rusholme, B; Sandri, M; Savelainen, M; Savini, G; Scott, D; Soler, JD; Stolyarov, V; Sutton, D; Suur-Uski, AS; Sygnet, JF; Tauber, JA; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, LA; Wandelt, BD; Yvon, D; Zacchei, A; Zonca, A (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
    Planck observations at 353 GHz provide the first fully sampled maps of the polarized dust emission towards interstellar filaments and their backgrounds (i.e., the emission observed in the surroundings of the filaments). ...
  • Planck intermediate results: XXXIV. The magnetic field structure in the Rosette Nebula 
    Aghanim, Nabila; Alves, M. I. R.; Arnaud, M.; Arzoumanian, D.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Bartolo, N.; Battaner, E.; Benabed, K.; Benoit-Lévy, A.; Bernard, J.-P.; Bersanelli, M.; Bielewicz, P.; Bonaldi, A.; Bonavera, L.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bracco, A.; Burigana, C.; Calabrese, E.; Cardoso, J.-F.; Catalano, A.; Chamballu, A.; Chiang, H. C.; Christensen, P. R.; Colombi, S.; Colombo, L. P. L.; Combet, C.; Couchot, F.; Crill, B. P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; Davis, R. J.; de Bernardis, P.; de Rosa, A.; de Zotti, G.; Delabrouille, J; Dickinson, C.; Diego, J. M.; Dole, H.; Donzelli, Simona; Doré, O.; Douspis, M.; Ducout, A.; Dupac, X; Efstathiou, G; Elsner, F; Enßlin, TA; Eriksen, Hans Kristian Kamfjord; Falgarone, E; Ferriere, K; Finelli, F; Forni, O; Frailis, M; Fraisse, AA; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Ghosh, T; Giard, M; Gjerløw, Eirik; Gonzalez-Nuevo, J; Gorski, KM; Gregorio, A; Gruppuso, A; Guillet, V; Hansen, Frode Kristian; Hanson, D; Harrison, DL; Henrot-Versille, S; Herranz, D; Hildebrandt, SR; Hivon, E; Hobson, M; Holmes, WA; Hornstrup, A; Hovest, W; Huffenberger, KM; Hurier, G; Jaffe, AH; Jaffe, TR; Jewell, J; Juvela, M; Keskitalo, R; Kisner, TS; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, JM; Lasenby, A; Lattanzi, M; Lawrence, CR; Leonardi, R; Levrier, F; Liguori, M; Lilje, Per Barth; Linden-Vørnle, M; Lopez-Caniego, M; Lubin, PM; Macias-Perez, JF; Maffei, B; Maino, D; Mandolesi, N; Mangilli, A; Maris, M; Martin, PG; Martinez-Gonzalez, E; Masi, S; Matarrese, S; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Miville-Deschenes, MA; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Moss, A; Munshi, D; Murphy, JA; Naselsky, P; Nati, F; Natoli, P; Netterfield, CB; Noviello, F; Novikov, D; Novikov, I; Oppermann, N; Pagano, L; Pajot, F; Paladini, R; Paoletti, D; Pasian, F; Patanchon, G; Perdereau, O; Pettorino, V; Piacentini, F; Piat, M; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Ponthieu, N; Pratt, GW; Prezeau, G; Prunet, S; Puget, JL; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rubino-Martin, JA; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Savini, G; Scott, D; Soler, JD; Spencer, LD; Stolyarov, V; Sutton, D; Suur-Uski, AS; Sygnet, JF; Tauber, JA; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, LA; Wandelt, BD; Wehus, Ingunn Kathrine; Wiesemeyer, H; Yvon, D; Zacchei, A; Zonca, A (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
    Planck has mapped the polarized dust emission over the whole sky, making it possible to trace the Galactic magnetic field structure that pervades the interstellar medium (ISM). We combine polarization data from Planck with ...
  • Planck intermediate results: XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds 
    Ade, P. A. R.; Aghanim, N.; Alves, M. I. R.; Arnaud, M.; Arzoumanian, D.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Bartolo, N.; Battaner, E.; Benabed, K.; Benoît, A.; Benoit-Lévy, A.; Bernard, J.-P.; Bersanelli, M.; Bielewicz, P.; Bock, J. J.; Bonavera, L.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bracco, A.; Burigana, C.; Calabrese, E.; Cardoso, J.-F.; Catalano, A.; Chiang, H. C.; Christensen, P. R.; Colombo, L. P. L.; Combet, C.; Couchot, F.; Crill, B. P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; Davis, R. J.; de Bernardis, P.; de Rosa, A.; de Zotti, G.; Delabrouille, J; Dickinson, C.; Diego, J. M.; Dole, H.; Donzelli, S.; Doré, O.; Douspis, M.; Ducout, A.; Dupac, X; Efstathiou, G; Elsner, F; Enßlin, TA; Eriksen, Hans Kristian Kamfjord; Falceta-Goncalves, D; Falgarone, E; Ferriere, K; Finelli, F; Forni, O; Frailis, M; Fraisse, AA; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Ghosh, T; Giard, M; Gjerløw, Eirik; Gonzalez-Nuevo, J; Gorski, KM; Gregorio, A; Gruppuso, A; Gudmundsson, JE; Guillet, V; Harrison, DL; Helou, G; Hennebelle, P; Henrot-Versille, S; Hernandez-Monteagudo, C; Herranz, D; Hildebrandt, SR; Hivon, E; Holmes, WA; Hornstrup, A; Huffenberger, KM; Hurier, G; Jaffe, AH; Jaffe, TR; Jones, WC; Juvela, M; Keihänen, E; Keskitalo, R; Kisner, TS; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, JM; Lasenby, A; Lattanzi, M; Lawrence, CR; Leonardi, R; Levrier, F; Liguori, M; Lilje, Per Barth; Linden-Vørnle, M; Lopez-Caniego, M; Lubin, PM; Macias-Perez, JF; Maino, D; Mandolesi, N; Mangilli, A; Maris, M; Martin, PG; Martinez-Gonzalez, E; Masi, S; Matarrese, S; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Miville-Deschenes, MA; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, JA; Naselsky, P; Nati, F; Netterfield, CB; Noviello, F; Novikov, D; Novikov, I; Oppermann, N; Oxborrow, CA; Pagano, L; Pajot, F; Paladini, R; Paoletti, D; Pasian, F; Perotto, L; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Ponthieu, N; Pratt, GW; Prunet, S; Puget, JL; Rachen, JP; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rossetti, M; Roudier, G; Rubino-Martin, JA; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Savini, G; Scott, D; Soler, Juan D; Stolyarov, V; Sudiwala, R; Sutton, D; Suur-Uski, AS; Sygnet, JF; Tauber, JA; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Umana, G; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, LA; Wandelt, BD; Wehus, Ingunn Kathrine; Ysard, N; Yvon, D; Zonca, A (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
    Within ten nearby (d <  450 pc) Gould belt molecular clouds we evaluate statistically the relative orientation between the magnetic field projected on the plane of sky, inferred from the polarized thermal emission of ...
  • Planck intermediate results: XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect 
    Ade, P. A. R.; Aghanim, N.; Arnaud, M.; Ashdown, M.; Aubourg, E.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Bartolo, N.; Battaner, E.; Benabed, K.; Benoit-Lévy, A.; Bersanelli, M.; Bielewicz, P.; Bock, J. J.; Bonaldi, A.; Bonavera, L.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Burigana, C.; Calabrese, E.; Cardoso, J.-F.; Catalano, A.; Chamballu, A.; Chiang, H. C.; Christensen, P. R.; Clements, D. L.; Colombo, L. P. L.; Combet, C.; Crill, B. P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; Davis, R. J.; de Bernardis, P.; de Zotti, G.; Delabrouille, J.; Dickinson, C.; Diego, J. M.; Dolag, K.; Donzelli, Simona; Doré, O.; Douspis, M.; Ducout, A.; Dupac, X.; Efstathiou, G.; Elsner, F.; Enßlin, T. A.; Eriksen, Hans Kristian Kamfjord; Finelli, F.; Forni, O; Frailis, M; Fraisse, AA; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Genova-Santos, RT; Giard, M; Gjerløw, Eirik; Gonzalez-Nuevo, J; Gorski, KM; Gregorio, A; Gruppuso, A; Hansen, Frode Kristian; Harrison, DL; Henrot-Versille, S; Hernandez-Monteagudo, C; Herranz, D; Hildebrandt, SR; Hivon, E; Hobson, M; Hornstrup, A; Huffenberger, KM; Hurier, G; Jaffe, AH; Jaffe, TR; Jones, WC; Juvela, M; Keihänen, E; Keskitalo, R; Kitaura, F; Kneissl, R; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, JM; Lasenby, A; Lattanzi, M; Lawrence, CR; Leonardi, R; Leon-Tavares, J; Levrier, F; Liguori, M; Lilje, Per Barth; Linden-Vørnle, M; Lopez-Caniego, M; Lubin, PM; Ma, YZ; Macias-Perez, JF; Maffei, B; Maino, D; Mak, DSY; Mandolesi, N; Mangilli, A; Maris, M; Martin, PG; Martinez-Gonzalez, E; Masi, S; Matarrese, S; McGehee, P; Melchiorri, A; Mennella, A; Migliaccio, M; Miville-Deschenes, MA; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, JA; Naselsky, P; Nati, F; Natoli, P; Noviello, F; Novikov, D; Novikov, I; Oxborrow, CA; Pagano, L; Pajot, F; Paoletti, D; Perdereau, O; Perotto, L; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pointecouteau, E; Polenta, G; Ponthieu, N; Pratt, GW; Puget, JL; Puisieux, S; Rachen, JP; Racine, Benjamin; Reach, WT; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rubino-Martin, JA; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Savini, G; Scott, D; Spencer, LD; Stolyarov, V; Sudiwala, R; Sunyaev, R; Sutton, D; Suur-Uski, AS; Sygnet, JF; Tauber, JA; Terenzi, L; Toffolatti, L; Tomasi, M; Tucci, M; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, LA; Wandelt, BD; Wang, W; Wehus, Ingunn Kathrine; Yvon, D; Zacchei, A; Zonca, A (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2016)
    By looking at the kinetic Sunyaev-Zeldovich effect (kSZ) in Planck nominal mission data, we present a significant detection of baryons participating in large-scale bulk flows around central galaxies (CGs) at redshift z ≈ ...