Planck 2013 results. XII. Diffuse component separation

@article{Ade2013Planck2R,
  title={Planck 2013 results. XII. Diffuse component separation},
  author={P. A. R. Ade and Nabila Aghanim and Charmaine Armitage-Caplan and Monique D. Arnaud and Mark Ashdown and Fernando Atrio-Barandela and J. Aumont and Carlo Baccigalupi and Anthony J. Banday and Rita Bel{\'e}n Barreiro and James G. Bartlett and Eduardo Battaner and Karim Benabed and Aur{\'e}lien Benoit and Aur{\'e}lien Benoit-L{\'e}vy and J-Ph. Bernard and M. Bersanelli and Pawel Bielewicz and J{\'e}r{\^o}me Bobin and James J. Bock and Anna Bonaldi and Laura Bonavera and J. Richard Bond and Julian Borrill and François R. Bouchet and F. Boulanger and M. Bridges and Manfred Bucher and C. Burigana and R. C. Butler and Jean-François Cardoso and Andrea Catalano and Anthony D. Challinor and A. Chamballu and Ranga-ram Chary and Xianjue Chen and L. Y. Chiang and H. Cynthia Chiang and Philip R. Christensen and Sarah E. Church and D. L. Clements and St{\'e}phane Colombi and Loris P. L. Colombo and François Couchot and A. Coulais and Brendan Crill and M. Cruz and A. Fernandez Curto and F. Cuttaia and Luigi Danese and Rodney D. Davies and R. J. Davis and Paolo Bernardis and Adriano de Rosa and Gianfranco de Zotti and Jacques Delabrouille and J. M. Delouis and F. X. D'esert and Clive Dickinson and Jose M. Diego and Herve A. Dole and Simona Donzelli and Olivier Dor'e and Marian Douspis and Jo Dunkley and Xavier Dupac and George P. Efstathiou and Torsten A. Ensslin and Hans Kristian Eriksen and E. Falgarone and Fabio Finelli and Olivier Forni and Marco Frailis and Aur'elien A. Fraisse and Enrico Franceschi and S. Galeotta and Kenneth Matthew Ganga and Martin Giard and Giovanna Giardino and Yannick Giraud-H'eraud and Joaquin Gonz'alez-Nuevo and Krzysztof M. G'orski and Steven Gratton and Anna Gregorio and Alessandro Gruppuso and Frode 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 Sergi R. Hildebrandt and E. Hivon and Michael P. Hobson and Warren Albert Holmes and Allan Hornstrup and W. Hovest and Greg Huey and Kevin M. Huffenberger and Tess R. Jaffe and Andrew H. 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 Martin Kunz and Hannu Kurki-Suonio and Guilaine Lagache and Anne Lahteenmaki and J-M. Lamarre and Anthony N. Lasenby and Ren{\'e} J. Laureijs and Charles R. Lawrence and Maude Le Jeune and Samuel M. Leach and J. Patrick Leahy and Rodrigo Leonardi and Julien Lesgourgues and Michele Liguori and Per B. Lilje and M. J. D. Linden-Vornle and Marcos L'opez-Caniego and Philip M. Lubin and Juan Francisco Mac'ias-P'erez and Bruno Maffei and Davide Maino and Nazzareno Mandolesi and Airam Marcos-Caballero and M. Maris and Douglas J. Marshall and P. G. Martin and E. Mart'inez-Gonz'alez and Silvia Masi and S. Matarrese and Frank Matthai and Pasquale Mazzotta and P. Meinhold and Alessandro Melchiorri and Luis Mendes and A. Mennella and Marina Migliaccio and K. Mikkelsen and Supriyo Mitra and Marc-Antoine Miville-Desch{\^e}nes and Andrea Moneti and Laurent Montier and Gianluca Morgante and Daniel J. Mortlock and Adam Moss and Dipak Munshi 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 I. Novikov and Ian O'Dwyer and Shannon Osborne and Carol Anne Oxborrow and Francesco Paci and Luca Pagano and François Pajot and R. 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 P. Platania and Etienne Pointecouteau and Gianluca Polenta and N. Ponthieu and L. A. Popa and Torsti J. Poutanen and Gabriel W. Pratt and Gary Marcel Prezeau and Simon Prunet and J-L. Puget and Jorg P. Rachen and William T. Reach and Rafael Rebolo and Martin Reinecke and Mathieu Remazeilles and C'ecile Renault and Alessandro Renzi and Stefano Ricciardi and Thomas Riller and Isabelle Ristorcelli and Graca M. Rocha and C. Dutruc Rosset and Gael M. Roudier and Michael Rowan-Robinson and Jos'e Alberto Rubino-Mart'in and Ben Rusholme and Emanuele Salerno and M. Sandri and D. Santos and Giorgio Savini and F. Schiavon and Douglas Scott and Michael Dean Seiffert and E. P. S. Shellard and Locke D Spencer and J. L. Starck and Radek Stompor and Rashmikant V. Sudiwala and Rashid Alievich Sunyaev and Florent Sureau and David O. Sutton and A.-S. Suur-Uski and J. -F. Sygnet and Jan Tauber and Daniele Tavagnacco and Luca Terenzi and Luigi Toffolatti and Maurizio Tomasi and Matthieu Tristram and Marco Tucci and Jussi Tuovinen and M. Turler and Grazia Umana and Luca Valenziano and Jussi Valiviita and Bartjan van Tent and Juha Varis and M atteo Viel and Patricio Vielva and Fabrizio Villa and Nicola Vittorio and Lawrence A. Wade and Benjamin D. Wandelt and Ingunn Kathrine Wehus and Althea Wilkinson and Junqing Xia and D. Yvon and Andrea Zacchei and Andrea Zonca},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={571},
  pages={4}
}
Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwave background (CMB) temperature fluctuations over nearly the full sky, as well as new constraints on Galactic foregrounds, including thermal dust and line emission from molecular carbon monoxide (CO). This paper describes the component separation framework adopted by Planck for many cosmological analyses, including CMB… Expand
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Planck 2013 results. XV. CMB power spectra and likelihood
This paper presents the Planck 2013 likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations that accounts for all known relevantExpand
Component separation methods for the PLANCK mission
Context. The PLANCK satellite will map the full sky at nine frequencies from 30 to 857 GHz. The CMB intensity and polarization that are its prime targets are contaminated by foreground emission. Expand
Planck 2013 results - XXIII. Isotropy and statistics of the CMB
We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our results are based mainly on the full PlanckExpand
Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation
The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the distribution ofExpand
Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies
Using Planck maps of six regions of low Galactic dust emission with a total area of about 140 deg 2 , we determine the angular power spectra of cosmic infrared background (CIB) anisotropies fromExpand
Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
We present new measurements of cosmic infrared background (CIB) anisotropies using Planck. Combining HFI data with IRAS, the angular auto- and cross-frequency power spectrum is measured from 143 toExpand
Planck 2013 results. XIII. Galactic CO emission
Rotational transition lines of CO play a major role in molecular radio astronomy as a mass tracer and in particular in the study of star formation and Galactic structure. Although a wealth of dataExpand
Planck 2015 results - XIII. Cosmological parameters
This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. Our results are inExpand
Planck 2013 results. XVII. Gravitational lensing by large-scale structure
On the arcminute angular scales probed by Planck, the cosmic microwave background (CMB) anisotropies are gently perturbed by gravitational lensing. Here we present a detailed study of this e_ect,Expand
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission
The WMAP mission has mapped the full sky to determine the geometry, content, and evolution of the universe. Full sky maps are made in five microwave frequency bands to separate the temperatureExpand
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