Planck 2015 results. IX. Diffuse component separation: CMB maps

@article{Adam2016Planck2R,
  title={Planck 2015 results. IX. Diffuse component separation: CMB maps},
  author={Planck Collaboration R. Adam and P. Ade and N. Aghanim and M. Arnaud and M. Ashdown and J. Aumont and C. Baccigalupi and A. Banday and R. B. Barreiro and J. Bartlett and N. Bartolo and S. Basak and E. Battaner and K. Benabed and A. Benoit 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 M. Bucher and C. Burigana and R. C. Butler and E. Calabrese and J. Cardoso and B. Casaponsa and G. Castex 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 A. Rosa and G. Zotti and J. Delabrouille and F. D'esert and C. Dickinson and J. Diego and H. Dole and S. Donzelli and O. Dor'e and M. Douspis and A. Ducout and X. Dupac and G. Efstathiou and F. Elsner and T. Ensslin and H. Eriksen and E. Falgarone and Y. Fantaye and J. Fergusson 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 J. Gudmundsson 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 S. Hildebrandt and E. Hivon and M. Hobson and W. Holmes and A. Hornstrup and W. Hovest and K. Huffenberger and G. Hurier and A. Jaffe and T. Jaffe and W. Jones and M. Juvela and E. Keihanen and R. Keskitalo and T. Kisner and R. Kneissl and J. Knoche 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. Jeune 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 G. Maggio and D. Maino and N. Mandolesi and A. Mangilli and D. Marshall and P. Martin and E. Mart'inez-Gonz'alez and S. Masi and S. Matarrese and P. Mazzotta and P. McGehee and P. Meinhold and A. Melchiorri and L. Mendes and A. Mennella and M. Migliaccio and S. Mitra and M. Miville-Desch{\^e}nes and D. Molinari 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 C. A. Oxborrow and F. Paci and L. Pagano and F. Pajot and R. Paladini and D. Paoletti 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 G. Pratt and G. Prezeau and S. Prunet and J. Puget and J. Rachen and B. Racine and W. Reach and R. Rebolo and M. Reinecke and M. Remazeilles and C. Renault and A. Renzi and I. Ristorcelli and G. Rocha and C. Rosset and M. Rossetti and G. Roudier and J. Rubino-Mart'in and B. Rusholme and M. Sandri and D. Santos and M. Savelainen and G. Savini and D. Scott and M. Seiffert and E. Shellard 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 T. Trombetti and M. Tucci and J. Tuovinen and L. Valenziano and J. Valiviita and B. Tent and P. Vielva and F. Villa and L. Wade and B. Wandelt and I. Wehus and D. Yvon and A. Zacchei and A. Zonca},
  journal={Astronomy and Astrophysics},
  year={2016},
  volume={594},
  pages={1-42}
}
We present foreground-reduced cosmic microwave background (CMB) maps derived from the full Planck data set in both temperature and polarization. Compared to the corresponding Planck 2013 temperature sky maps, the total data volume is larger by a factor of 3.2 for frequencies between 30 and 70 GHz, and by 1.9 for frequencies between 100 and 857 GHz. In addition, systematic errors in the forms of temperature-to-polarization leakage, analogue-to-digital conversion uncertainties, and very long time… Expand
Planck 2015 results. V. LFI calibration
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Component separation methods for the PLANCK mission
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