# Planck intermediate results - XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

@article{Adam2016PlanckIR, title={Planck intermediate results - XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes}, author={Planck Collaboration R. Adam and P. Ade and N. Aghanim and M. Arnaud and J. Aumont and C. Baccigalupi and A. Banday and R. B. Barreiro and J. Bartlett and N. Bartolo and E. Battaner and K. Benabed and A. Benoit-L{\'e}vy and J. Bernard and M. Bersanelli and P. Bielewicz and A. Bonaldi and L. Bonavera and J. Bond and J. Borrill and F. Bouchet and F. Boulanger and A. Bracco and M. Bucher and C. Burigana and R. C. Butler and E. Calabrese and J. Cardoso and A. Catalano and A. Challinor and A. Chamballu and R. Chary and H. Chiang and P. Christensen and D. Clements and S. Colombi and L. Colombo and C. Combet and F. Couchot and A. Coulais and B. Crill and A. Curto and F. Cuttaia and L. Danese and R. Davies and R. Davis and P. Bernardis and G. Zotti and J. Delabrouille and J. Delouis and F. D'esert and C. Dickinson and J. Diego and K. Dolag and H. Dole and S. Donzelli and O. Dor'e and M. Douspis and A. Ducout and J. Dunkley and X. Dupac and G. Efstathiou and F. Elsner and T. Ensslin and H. Eriksen and E. Falgarone and F. Finelli and O. Forni and M. Frailis and A. Fraisse and E. Franceschi and A. Frejsel and S. Galeotta and S. Galli and K. Ganga and T. Ghosh and M. Giard and Y. Giraud-H'eraud and E. Gjerl{\o}w and J. Gonz'alez-Nuevo and K. M. G'orski and S. Gratton and A. Gregorio and A. Gruppuso and V. Guillet and F. Hansen and D. Hanson and D. Harrison and G. Helou and S. Henrot-Versill'e and C. Hern'andez-Monteagudo and D. Herranz and E. Hivon and M. Hobson and W. Holmes and K. Huffenberger and G. Hurier and A. Jaffe and T. Jaffe and J. Jewell and W. Jones and M. Juvela and E. Keihanen and R. Keskitalo and T. Kisner and R. Kneissl and J. Knoche and L. Knox 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 J. Leahy and R. Leonardi and J. Lesgourgues and F. L{\'e}vrier and M. Liguori and P. Lilje and M. Linden-Vornle and M. L'opez-Caniego and P. Lubin and J. Mac'ias-P'erez and B. Maffei and D. Maino and N. Mandolesi and A. Mangilli and M. Maris and P. Martin and E. Mart'inez-Gonz'alez and S. Masi and S. Matarrese and P. Mazzotta and A. Melchiorri and L. Mendes and A. Mennella and M. Migliaccio and S. Mitra and M. Miville-Desch{\^e}nes and A. Moneti and L. Montier and G. Morgante and D. Mortlock and A. Moss and D. Munshi and J. A. Murphy and P. Naselsky and F. Nati and P. Natoli and C. Netterfield and H. N{\o}rgaard-Nielsen and F. Noviello and D. Novikov and I. Novikov and L. Pagano and F. Pajot and R. Paladini and D. Paoletti and B. Partridge and F. Pasian and G. Patanchon and T. Pearson and O. Perdereau and L. Perotto and F. Perrotta and V. Pettorino and F. Piacentini and M. Piat and E. Pierpaoli and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and N. Ponthieu and L. Popa and G. Pratt and S. Prunet and J. Puget and J. Rachen and W. Reach and R. Rebolo and M. Remazeilles and C. Renault and A. Renzi and S. Ricciardi and I. Ristorcelli and G. Rocha and C. Rosset and M. Rossetti and G. Roudier and B. R. d'Orfeuil and J. Rubino-Mart'in and B. Rusholme and M. Sandri and D. Santos and M. Savelainen and G. Savini and D. Scott and J. Soler and L. Spencer and V. Stolyarov and R. Stompor and R. Sudiwala and R. Sunyaev and D. Sutton and A. Suur-Uski and J. Sygnet and J. Tauber and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and M. Tucci and J. Tuovinen and L. Valenziano and J. Valiviita and B. Tent and L. Vibert and P. Vielva and F. Villa and L. Wade and B. Wandelt and R. Watson and I. Wehus and M. White and S. White and D. Yvon and A. Zacchei and A. Zonca}, journal={Astronomy and Astrophysics}, year={2016}, volume={586}, pages={1-25} }

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 C_l^(EE) and C_l^(BB) over the multipole range 40 <l< 600 well away from the Galactic plane. These measurements will bring new insights into interstellar… Expand

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#### References

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Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust

- Physics
- 2014