Planck 2018 results. XII. Galactic astrophysics using polarized dust emission
@article{Aghanim2018Planck2R,
title={Planck 2018 results. XII. Galactic astrophysics using polarized dust emission},
author={Planck Collaboration N. Aghanim and Y. Akrami and M. Alves and M. Ashdown and J. Aumont and C. Baccigalupi and M. Ballardini and A. Banday and R. B. Barreiro and N. Bartolo and S. Basak and K. Benabed and J. Bernard and M. Bersanelli and P. Bielewicz and J. Bock and J. R. Bond and J. Borrill and F. Bouchet and F. Boulanger and A. Bracco and M. Bucher and C. Burigana and E. Calabrese and J. Cardoso and J. Carron and R. Chary and H. Chiang and L. Colombo and C. Combet and B. P. Crill and F. Cuttaia and P. Bernardis and G. Zotti and J. Delabrouille and J. Delouis and E. D. Valentino and C. Dickinson and J. Diego and O. Dor'e and M. Douspis and A. Ducout and X. Dupac and G. Efstathiou and F. Elsner and T. A. Ensslin and H. Eriksen and E. Falgarone and Y. Fantaye and R. Fernandez-Cobos and K. Ferri{\`e}re and F. Finelli and F. Forastieri and M. Frailis and A. Fraisse and E. Franceschi and A. Frolov and S. Galeotta and S. Galli and K. Ganga and R. G'enova-Santos and M. Gerbino and T. Ghosh and J. Gonz{\'a}lez-Nuevo and K. G{\'o}rski and S. Gratton and G. Green and A. Gruppuso and J. Gudmundsson and V. Guillet and W. Handley and F. Hansen and G. Helou and D. Herranz and E. Hivon and Z. Huang and A. Jaffe and W. Jones and E. Keihanen and R. Keskitalo and K. Kiiveri and J. Kim and N. Krachmalnicoff and M. Kunz and H. Kurki-Suonio and G. Lagache and J. Lamarre and A. Lasenby and M. Lattanzi and C. Lawrence and M. L. Jeune and F. Levrier and M. Liguori and P. Lilje and V. Lindholm and M. L{\'o}pez-Caniego and P. Lubin and Y.-Z. Ma and J. Mac'ias-P'erez and G. Maggio and D. Maino and N. Mandolesi and A. Mangilli and A. Marcos-Caballero and M. Maris and P. Martin and E. Martinez-Gonzalez and S. Matarrese and N. Mauri and J. McEwen and A. Melchiorri and A. Mennella and M. Migliaccio and M. Miville-Desch{\^e}nes and D. Molinari and A. Moneti and L. Montier and G. Morgante and A. Moss and P. Natoli and L. Pagano and D. Paoletti and G. Patanchon and F. Perrotta and V. Pettorino and F. Piacentini and L. Polastri and G. Polenta and J. Puget and J. Rachen and M. Reinecke and M. Remazeilles and A. Renzi and I. Ristorcelli and G. Rocha and C. Rosset and G. Roudier and J. A. Rubi{\~n}o-Mart{\'i}n and B. Ruiz-Granados and L. Salvati and M. Sandri and M. Savelainen and D. Scott and C. Sirignano and R. Sunyaev and A. Suur-Uski and J. Tauber and D. Tavagnacco and M. Tenti and L. Toffolatti and M. Tomasi and T. Trombetti and J. Valiviita and F. Vansyngel and B. Tent and P. Vielva and F. Villa and N. Vittorio and B. Wandelt and I. Wehus and A. Zacchei and A. Zonca},
journal={Astronomy and Astrophysics},
year={2018},
volume={641},
pages={12}
}We present 353 GHz full-sky maps of the polarization fraction p, angle ψ, and dispersion of angles S of Galactic dust thermal emission produced from the 2018 release of Planck data. We confirm that the mean and maximum of p decrease with increasing N_H. The uncertainty on the maximum polarization fraction, p_(max)=22.0% at 80 arcmin resolution, is dominated by the uncertainty on the zero level in total intensity. The observed inverse behaviour between p and S is interpreted with models of the… CONTINUE READING
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