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 Peter A. R. Ade and Nabila Aghanim and Monique D. Arnaud and J. Aumont and Carlo Baccigalupi and Anthony J. Banday and Rita Bel{\'e}n Barreiro and James G. Bartlett and Nicola Bartolo and Eduardo Battaner and Karim Benabed and Aur{\'e}lien Benoit-L{\'e}vy and J-Ph. Bernard and M. Bersanelli and Pawel Bielewicz and Anna Bonaldi and Laura Bonavera and J. Richard Bond and Julian Borrill and Francois R. Bouchet and Francois Boulanger and Andrea Bracco and Manfred Bucher and Carlo Burigana and R. C. Butler and Erminia Calabrese and J.-F. Cardoso and A. Catalano and Anthony Challinor and A. Chamballu and Ranga Ram Chary and H. C. Chiang and Philip R. Christensen and David L. Clements and St{\'e}phane Colombi and Loris P. L. Colombo and C{\'e}line Combet and François Couchot and A. Coulais and Brendan P. Crill and A. Fernandez Curto and F. Cuttaia and Luigi Danese and Rodney D. Davies and R. J. Davis and Paolo Bernardis and Gianfranco De Zotti and Jacques Delabrouille and J. M. Delouis and F. X. D'esert and Clive Dickinson and Jose M. Diego and Klaus Dolag and Herve A. Dole and Simona Donzelli and Olivier Dor'e and Marian Douspis and Anne Ducout and Jo Dunkley and Xavier Dupac and George P. Efstathiou and Franz Elsner and Torsten A. Ensslin and Hans Kristian Eriksen and Edith Falgarone and Fabio Finelli and Olivier Forni and Marco Frailis and Aur'elien A. Fraisse and Enrico Franceschi and Anne Mette Frejsel and S. Galeotta and Silvia Galli and Ken Ganga and Tuhin Ghosh and Martin Giard and Yannick Giraud-H'eraud and Eirik Gjerl{\o}w and Joaquin Gonz'alez-Nuevo and Krzysztof M. G'orski and Steven Gratton and Anna Gregorio and Alessandro Gruppuso and V. Guillet and F. K. Hansen and Duncan Hanson and D. L. Harrison and George Helou and Sophie Henrot-Versill'e and Carlos Hern'andez-Monteagudo and Diego Herranz and Eric Hivon and Michael P. Hobson and Warren Albert Holmes and Kevin M. Huffenberger and Guillaume Hurier and Andrew H. Jaffe and Tess R. Jaffe and Jeffrey B. Jewell and William C. Jones and Mika Juvela and Elina Keihanen and Reijo Keskitalo and Theodore Kisner and R{\"u}diger Kneissl and J{\"o}rg Knoche and Lloyd Knox and Nicoletta Krachmalnicoff and Martin Kunz and Hannu Kurki-Suonio and Guilaine Lagache and J-M. Lamarre and Anthony N. Lasenby and Massimiliano Lattanzi and Charles R. Lawrence and Janet Leahy and Rodrigo Leonardi and Julien Lesgourgues and François L{\'e}vrier and Michele Liguori and Per B. Lilje and M. J. D. Linden-V{\o}rnle and Marcos L'opez-Caniego and Philip Lubin and Juan-Fancisco Mac'ias-P'erez and Bruno Maffei and Davide Maino and Nazzareno Mandolesi and Anna Mangilli and Michele Maris and P. G. Martin and E. Mart'inez-Gonz'alez and Serena Masi and S. Matarrese and Pasquale Mazzotta and Alessandro Melchiorri and Luis Mendes and Aniello Mennella and Marina Migliaccio and Supriyo Mitra and Marc-Antoine Miville-Desch{\^e}nes and Andrea Moneti and Laurent Montier and G. Morgante and Daniel J. Mortlock and Adam Moss and Dipak Munshi and J. Anthony Murphy and Pavel D. Naselsky and Federico Nati and Paolo Natoli and Calvin Barth Netterfield and Hans Ulrik N{\o}rgaard-Nielsen and Fabio Noviello and Dmitri D Novikov and Ilya Novikov and Luca Pagano and François Pajot and Roberta Paladini and Daniela Paoletti and Bruce Partridge and Fabio Pasian and Guillaume Patanchon and Timothy J. Pearson and Olivier Perdereau and L. Perotto and F. Perrotta and Valeria Pettorino and Francesco Piacentini and Michel Piat and Elena Pierpaoli and Davide Pietrobon and St{\'e}phane Plaszczynski and Etienne Pointecouteau and Gianluca Polenta and N. Ponthieu and L. A. Popa and Gabriel W. Pratt and Simon Prunet and J-L. Puget and Jorg P. Rachen and William T. Reach and Rafael Rebolo and Mathieu Remazeilles and C'ecile Renault and Alessandro Renzi and Stefano Ricciardi and Isabelle Ristorcelli and Graca M. Rocha and C. Dutruc Rosset and Mariachiara Rossetti and Gael M. Roudier and Benjamin Rouill'e d'Orfeuil and Jos'e Alberto Rubino-Mart'in and Ben Rusholme and M. Sandri and D. Santos and Matti Savelainen and Giorgio Savini and Douglas Scott and Juan Diego Soler and Locke D Spencer and Vasily Stolyarov and Radek Stompor and R. Sudiwala and Rashid Sunyaev and David O. Sutton and A.-S. Suur-Uski and J. -F. Sygnet and Jan Tauber and Luca Terenzi and Luigi Toffolatti and Maurizio Tomasi and M. Tristram and Marco Tucci and Jussi Tuovinen and Luca Valenziano and Jussi Valiviita and Bartjan van Tent and L. Vibert and Patricio Vielva and Fabrizio Villa and Lawrence A. Wade and Benjamin D. Wandelt and Robert A. Watson and Ingunn Kathrine Wehus and Martin White and Simon D. M. White and D. Yvon and Andrea Zacchei and Andrea 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… 
Planck intermediate results L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysis
The characterization of the Galactic foregrounds has been shown to be the main obstacle in thechallenging quest to detect primordial B -modes in the polarized microwave sky. We make use of the Planck
Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization
Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We use these data to characterize the frequency dependence of dust emission. We
Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz, which is the most sensitive Planck channel for dust polarization. We construct and analyse maps of dust
Planck 2018 results
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization in the quest for the curl-like B-mode polarization from primordial
Planck intermediate results XLIV. Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
We study the statistical properties of interstellar dust polarization at high Galactic latitude, using the Stokes parameter Planck maps at 353 GHz. Our aim is to advance the understanding of the
Polarized galactic synchrotron and dust emission and their correlation
We present an analysis of the level of polarized dust and synchrotron emission using the WMAP9 and Planck data. The primary goal of this study is to inform the assessment of foreground contamination
Planck intermediate results: XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible
The Planck survey provides unprecedented full-sky coverage of the submillimetre polarized emission from Galactic dust. In addition to the information on the direction of the Galactic magnetic field,
Dust polarization modelling at large scale over the northern Galactic cap using EBHIS and Planck data
The primary source of systematic uncertainty in the quest for the B-mode polarization of the Cosmic Microwave Background (CMB) introduced by primordial gravitational waves is polarized thermal
Statistical simulations of the dust foreground to cosmic microwave background polarization (Corrigendum)
The characterization of the dust polarization foreground to the Cosmic Microwave Background (CMB) is a necessary step towards the detection of the B-mode signal associated with primordial
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References

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Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization
Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We use these data to characterize the frequency dependence of dust emission. We
Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz, which is the most sensitive Planck channel for dust polarization. We construct and analyse maps of dust
Planck intermediate results: XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible
The Planck survey provides unprecedented full-sky coverage of the submillimetre polarized emission from Galactic dust. In addition to the information on the direction of the Galactic magnetic field,
Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence
Polarized emission observed by Planck HFI at 353 GHz towards a sample of nearby fields is presented, focusing on the statistics of polarization fractions p and angles ψ. The polarization fractions
Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies
The dust-Hi correlation is used to characterize the emission properties of dust in the diffuse interstellar medium (ISM) from far infrared wavelengths to microwave frequencies. The field of this
Joint 3D modelling of the polarized Galactic synchrotron and thermal dust foreground diffuse emission
Aims. We present for the first time a coherent model of the polarized Galactic synchrotron and thermal dust emissions that are likely to form the predominant diffuse foregrounds for measuring the
Comparing polarized synchrotron and thermal dust emission in the galactic plane
As the next step toward an improved large scale Galactic magnetic field model, we present a simple comparison of polarised synchrotron and thermal dust emission on the Galactic plane. We find that
Galactic foreground contributions to the 5-year Wilkinson Microwave Anisotropy Probe maps
We compute the cross-correlation between intensity and polarization from the 5-year Wilkinson Microwave Anisotropy Probe (WMAP5) data in different sky regions with respect to template maps for
First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was
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