Planck intermediate results

  title={Planck intermediate results},
  author={Planck Collaboration Y. Akrami and Mark Ashdown and Carlo Baccigalupi and Mario Ballardini and Anthony J. Banday and Rita Bel{\'e}n Barreiro and Nicola Bartolo and Soumen Basak and Karim Benabed and J-Ph. Bernard and M. Bersanelli and Pawel Bielewicz and J. Richard Bond and Julian Borrill and Carlo Burigana and Erminia Calabrese and Jean-François Cardoso and B. Casaponsa and H. C. Chiang and C{\'e}line Combet and Dagoberto Contreras and Brendan P. Crill and F. Cuttaia and Paolo Bernardis and Alessandra De Rosa and Gianfranco De Zotti and Jacques Delabrouille and Eleonora Di Valentino and Jose M. Diego and Olivier Dor'e and Marian Douspis and Xavier Dupac and Torsten A. Ensslin and Hans Kristian Eriksen and Ra{\'u}l Fern{\'a}ndez-Cobos and Fabio Finelli and Marco Frailis and Enrico Franceschi and Andrei V. Frolov and S. Galeotta and Silvia Galli and Ken Ganga and Ricardo T. G'enova-Santos and Martina Gerbino and Joaquin Gonz'alez-Nuevo and Krzysztof M. G'orski and Alessandro Gruppuso and Jon E. Gudmundsson and W. J. Handley and Diego Herranz and Eric Hivon and Z. Huang and Andrew H. Jaffe and William C. Jones and Elina Keihanen and Reijo Keskitalo and Kimmo Kiiveri and J. Kim and Theodore Kisner and Nicoletta Krachmalnicoff and Martin Kunz and Hannu Kurki-Suonio and J-M. Lamarre and Massimiliano Lattanzi and Charles R. Lawrence and Maude Le Jeune and François L{\'e}vrier and Michele Liguori and Per B. Lilje and V. Lindholm and Marcos L'opez-Caniego and Juan-Fancisco Mac'ias-P'erez and Davide Maino and Nazzareno Mandolesi and Airam Marcos-Caballero and Michele Maris and P. G. Martin and E. Mart'inez-Gonz'alez and S. Matarrese and Nicoletta Mauri and Jason D. McEwen and Aniello Mennella and Marina Migliaccio and Diego Molinari and Andrea Moneti and Ludovic Montier and G. Morgante and Adam Moss and Paolo Natoli and Luca Pagano and Daniela Paoletti and F. Perrotta and Valeria Pettorino and Francesco Piacentini and Gianluca Polenta and Jorg P. Rachen and Martin Reinecke and Mathieu Remazeilles and Alessandro Renzi and Graca M. Rocha and C. Dutruc Rosset and Jos'e Alberto Rubino-Mart'in and Beatriz Ruiz-Granados and Laura Salvati and Matti Savelainen and Douglas Scott and C. Sirignano and G. Sirri and Locke D Spencer and Raelyn M. Sullivan and Rashid Sunyaev and A.-S. Suur-Uski and Jan Tauber and Daniele Tavagnacco and M. Tenti and Luigi Toffolatti and Maurizio Tomasi and Tiziana Trombetti and Jussi Valiviita and Bartjan van Tent and Patricio Vielva and Fabrizio Villa and Nicola Vittorio and Ingunn Kathrine Wehus and Andrea Zacchei and Andrea Zonca},
  journal={Astronomy \& Astrophysics},
The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularly with the Planck satellite. The simplest interpretation of the dipole is that it is due to our motion with respect to the rest frame of the CMB. Since current CMB experiments infer temperature anisotropies from angular intensity variations, the dipole modulates the temperature anisotropies with the same frequency… 

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