%0 Generic %1 citeulike:13901793 %A Collaboration, Planck %A Adam, R. %A Ade, P. A. R. %A Alves, M. I. R. %A Ashdown, M. %A Aumont, J. %A Baccigalupi, C. %A Banday, A. J. %A Barreiro, R. B. %A Bartolo, N. %A Battaner, E. %A Benabed, K. %A Benoit-Lévy, A. %A Bernard, J. P. %A Bersanelli, M. %A Bielewicz, P. %A Bonavera, L. %A Bond, J. R. %A Borrill, J. %A Bouchet, F. R. %A Boulanger, F. %A Bucher, M. %A Burigana, C. %A Butler, R. C. %A Calabrese, E. %A Cardoso, J. F. %A Catalano, A. %A Chiang, H. C. %A Christensen, P. R. %A Colombo, L. P. L. %A Combet, C. %A Couchot, F. %A Crill, B. P. %A Curto, A. %A Cuttaia, F. %A Danese, L. %A Davis, R. J. %A de Bernardis, P. %A de Rosa, A. %A de Zotti, G. %A Delabrouille, J. %A Dickinson, C. %A Diego, J. M. %A Dolag, K. %A Doré, O. %A Ducout, A. %A Dupac, X. %A Elsner, F. %A Enßlin, T. A. %A Eriksen, H. K. %A Ferrière, K. %A Finelli, F. %A Forni, O. %A Frailis, M. %A Fraisse, A. A. %A Franceschi, E. %A Galeotta, S. %A Ganga, K. %A Ghosh, T. %A Giard, M. %A Gjerløw, E. %A González-Nuevo, J. %A Górski, K. M. %A Gregorio, A. %A Gruppuso, A. %A Gudmundsson, J. E. %A Hansen, F. K. %A Harrison, D. L. %A Hernández-Monteagudo, C. %A Herranz, D. %A Hildebrandt, S. R. %A Hobson, M. %A Hornstrup, A. %A Hurier, G. %A Jaffe, A. H. %A Jaffe, T. R. %A Jones, W. C. %A Juvela, M. %A Keihänen, E. %A Keskitalo, R. %A Kisner, T. S. %A Knoche, J. %A Kunz, M. %A Kurki-Suonio, H. %A Lamarre, J. M. %A Lasenby, A. %A Lattanzi, M. %A Lawrence, C. R. %A Leahy, J. P. %A Leonardi, R. %A Levrier, F. %A Lilje, P. B. %A Linden-Vørnle, M. %A López-Caniego, M. %A Lubin, P. M. %A Mac\'ıas-Pérez, J. F. %A Maggio, G. %A Maino, D. %A Mandolesi, N. %A Mangilli, A. %A Maris, M. %A Martin, P. G. %A Masi, S. %A Melchiorri, A. %A Mennella, A. %A Migliaccio, M. %A Miville-Deschênes, M. A. %A Moneti, A. %A Montier, L. %A Morgante, G. %A Munshi, D. %A Murphy, J. A. %A Naselsky, P. %A Nati, F. %A Natoli, P. %A Nørgaard-Nielsen, H. U. %A Oppermann, N. %A Orlando, E. %A Pagano, L. %A Pajot, F. %A Paladini, R. %A Paoletti, D. %A Pasian, F. %A Perotto, L. %A Pettorino, V. %A Piacentini, F. %A Piat, M. %A Pierpaoli, E. %A Plaszczynski, S. %A Pointecouteau, E. %A Polenta, G. %A Ponthieu, N. %A Pratt, G. W. %A Prunet, S. %A Puget, J. L. %A Rachen, J. P. %A Reinecke, M. %A Remazeilles, M. %A Renault, C. %A Renzi, A. %A Ristorcelli, I. %A Rocha, G. %A Rossetti, M. %A Roudier, G. %A Rubi\ no-Mart\'ın, J. A. %A Rusholme, B. %A Sandri, M. %A Santos, D. %A Savelainen, M. %A Scott, D. %A Spencer, L. D. %A Stolyarov, V. %A Stompor, R. %A Strong, A. W. %A Sudiwala, R. %A Sunyaev, R. %A Suur-Uski, A. S. %A Sygnet, J. F. %A Tauber, J. A. %A Terenzi, L. %A Toffolatti, L. %A Tomasi, M. %A Tristram, M. %A Tucci, M. %A Valenziano, L. %A Valiviita, J. %A Van Tent, B. %A Vielva, P. %A Villa, F. %A Wade, L. A. %A Wandelt, B. D. %A Wehus, I. K. %A Yvon, D. %A Zacchei, A. %A Zonca, A. %D 2016 %K imported %T Planck intermediate results. XLII. Large-scale Galactic magnetic fields %U http://arxiv.org/abs/1601.00546 %X Recent models for the large-scale Galactic magnetic fields in the literature were largely constrained by synchrotron emission and Faraday rotation measures. We select three different but representative models and compare their predicted polarized synchrotron and dust emission with that measured by the Planck satellite. We first update these models to match the Planck synchrotron products using a common model for the cosmic-ray leptons. We discuss the impact on this analysis of the ongoing problems of component separation in the Planck microwave bands and of the uncertain cosmic-ray spectrum. In particular, the inferred degree of ordering in the magnetic fields is sensitive to these systematic uncertainties. We then compare the resulting simulated emission to the observed dust emission and find that the dust predictions do not match the morphology in the Planck data, particularly the vertical profile in latitude. We show how the dust data can then be used to further improve these magnetic field models, particularly in the thin disc of the Galaxy where the dust is concentrated. We demonstrate this for one of the models and present it as a proof of concept for how we will advance these studies in future using complementary information from ongoing and planned observational projects.

@misc{citeulike:13901793, abstract = {{Recent models for the large-scale Galactic magnetic fields in the literature were largely constrained by synchrotron emission and Faraday rotation measures. We select three different but representative models and compare their predicted polarized synchrotron and dust emission with that measured by the Planck satellite. We first update these models to match the Planck synchrotron products using a common model for the cosmic-ray leptons. We discuss the impact on this analysis of the ongoing problems of component separation in the Planck microwave bands and of the uncertain cosmic-ray spectrum. In particular, the inferred degree of ordering in the magnetic fields is sensitive to these systematic uncertainties. We then compare the resulting simulated emission to the observed dust emission and find that the dust predictions do not match the morphology in the Planck data, particularly the vertical profile in latitude. We show how the dust data can then be used to further improve these magnetic field models, particularly in the thin disc of the Galaxy where the dust is concentrated. We demonstrate this for one of the models and present it as a proof of concept for how we will advance these studies in future using complementary information from ongoing and planned observational projects.}}, added-at = {2019-03-25T08:20:55.000+0100}, archiveprefix = {arXiv}, author = {Collaboration, Planck and Adam, R. and Ade, P. A. R. and Alves, M. I. R. and Ashdown, M. and Aumont, J. and Baccigalupi, C. and Banday, A. J. and Barreiro, R. B. and Bartolo, N. and Battaner, E. and Benabed, K. and Benoit-L\'{e}vy, A. and Bernard, J. P. and Bersanelli, M. and Bielewicz, P. and Bonavera, L. and Bond, J. R. and Borrill, J. and Bouchet, F. R. and Boulanger, F. and Bucher, M. and Burigana, C. and Butler, R. C. and Calabrese, E. and Cardoso, J. F. and Catalano, A. and Chiang, H. C. and Christensen, P. R. and Colombo, L. P. L. and Combet, C. and Couchot, F. and Crill, B. P. and Curto, A. and Cuttaia, F. and Danese, L. and Davis, R. J. and de Bernardis, P. and de Rosa, A. and de Zotti, G. and Delabrouille, J. and Dickinson, C. and Diego, J. M. and Dolag, K. and Dor\'{e}, O. and Ducout, A. and Dupac, X. and Elsner, F. and En{\ss}lin, T. A. and Eriksen, H. K. and Ferri\`{e}re, K. and Finelli, F. and Forni, O. and Frailis, M. and Fraisse, A. A. and Franceschi, E. and Galeotta, S. and Ganga, K. and Ghosh, T. and Giard, M. and Gjerl{\o}w, E. and Gonz\'{a}lez-Nuevo, J. and G\'{o}rski, K. M. and Gregorio, A. and Gruppuso, A. and Gudmundsson, J. E. and Hansen, F. K. and Harrison, D. L. and Hern\'{a}ndez-Monteagudo, C. and Herranz, D. and Hildebrandt, S. R. and Hobson, M. and Hornstrup, A. and Hurier, G. and Jaffe, A. H. and Jaffe, T. R. and Jones, W. C. and Juvela, M. and Keih\"{a}nen, E. and Keskitalo, R. and Kisner, T. S. and Knoche, J. and Kunz, M. and Kurki-Suonio, H. and Lamarre, J. M. and Lasenby, A. and Lattanzi, M. and Lawrence, C. R. and Leahy, J. P. and Leonardi, R. and Levrier, F. and Lilje, P. B. and Linden-V{\o}rnle, M. and L\'{o}pez-Caniego, M. and Lubin, P. M. and Mac\'{\i}as-P\'{e}rez, J. F. and Maggio, G. and Maino, D. and Mandolesi, N. and Mangilli, A. and Maris, M. and Martin, P. G. and Masi, S. and Melchiorri, A. and Mennella, A. and Migliaccio, M. and Miville-Desch\^{e}nes, M. A. and Moneti, A. and Montier, L. and Morgante, G. and Munshi, D. and Murphy, J. A. and Naselsky, P. and Nati, F. and Natoli, P. and N{\o}rgaard-Nielsen, H. U. and Oppermann, N. and Orlando, E. and Pagano, L. and Pajot, F. and Paladini, R. and Paoletti, D. and Pasian, F. and Perotto, L. and Pettorino, V. and Piacentini, F. and Piat, M. and Pierpaoli, E. and Plaszczynski, S. and Pointecouteau, E. and Polenta, G. and Ponthieu, N. and Pratt, G. W. and Prunet, S. and Puget, J. L. and Rachen, J. P. and Reinecke, M. and Remazeilles, M. and Renault, C. and Renzi, A. and Ristorcelli, I. and Rocha, G. and Rossetti, M. and Roudier, G. and Rubi\ {n}o-Mart\'{\i}n, J. A. and Rusholme, B. and Sandri, M. and Santos, D. and Savelainen, M. and Scott, D. and Spencer, L. D. and Stolyarov, V. and Stompor, R. and Strong, A. W. and Sudiwala, R. and Sunyaev, R. and Suur-Uski, A. S. and Sygnet, J. F. and Tauber, J. A. and Terenzi, L. and Toffolatti, L. and Tomasi, M. and Tristram, M. and Tucci, M. and Valenziano, L. and Valiviita, J. and Van Tent, B. and Vielva, P. and Villa, F. and Wade, L. A. and Wandelt, B. D. and Wehus, I. K. and Yvon, D. and Zacchei, A. and Zonca, A.}, biburl = {https://www.bibsonomy.org/bibtex/25e5e9dc46ae039cf2803d66feea8bd50/ericblackman}, citeulike-article-id = {13901793}, citeulike-linkout-0 = {http://arxiv.org/abs/1601.00546}, citeulike-linkout-1 = {http://arxiv.org/pdf/1601.00546}, day = 4, eprint = {1601.00546}, interhash = {f8b1751b7ce974570363d722f2b75dc3}, intrahash = {5e5e9dc46ae039cf2803d66feea8bd50}, keywords = {imported}, month = jan, posted-at = {2016-01-10 04:21:35}, priority = {2}, timestamp = {2019-03-25T08:20:55.000+0100}, title = {{Planck intermediate results. XLII. Large-scale Galactic magnetic fields}}, url = {http://arxiv.org/abs/1601.00546}, year = 2016 }