# Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove

@article{Aghanim2013Planck2R, title={Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove}, author={Planck Collaboration N. Aghanim and C. Armitage-Caplan and M. Arnaud and M. Ashdown and F. Atrio-Barandela and J. Aumont and A. Banday and R. B. Barreiro and J. Bartlett and K. Benabed and A. Benoit-L{\'e}vy and J. Bernard and M. Bersanelli and P. Bielewicz and J. Bobin and J. Bock and J. Bond and J. Borrill and F. Bouchet and M. Bridges and C. Burigana and R. C. Butler and J. Cardoso and A. Catalano and A. Challinor and A. Chamballu and L. Chiang and H. Chiang and P. Christensen and D. Clements and L. Colombo and F. Couchot and B. Crill 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 J. Diego and S. Donzelli and O. Dor'e and X. Dupac and G. Efstathiou and T. Ensslin and H. Eriksen and F. Finelli and O. Forni and M. Frailis and E. Franceschi and S. Galeotta and K. Ganga and M. Giard and G. Giardino and J. Gonz'alez-Nuevo and K. M. G'orski and S. Gratton and A. Gregorio and A. Gruppuso and F. Hansen and D. Hanson and D. Harrison and G. Helou and S. Hildebrandt and E. Hivon and M. Hobson and W. Holmes and W. Hovest and K. Huffenberger and W. Jones and M. Juvela and E. Keihanen and R. Keskitalo and T. Kisner and J. Knoche and L. Knox and M. Kunz and H. Kurki-Suonio and A. Lahteenmaki and J. Lamarre and A. Lasenby and C. Lawrence and R. Leonardi and A. Lewis 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 M. Maris and D. Marshall and P. Martin and E. Mart'inez-Gonz'alez and S. Masi and S. Matarrese and P. Mazzotta and P. Meinhold and A. Melchiorri and L. Mendes and M. Migliaccio and S. Mitra and A. Moneti and L. Montier and G. Morgante and D. Mortlock and A. Moss and D. Munshi and P. Naselsky and F. Nati and P. Natoli and H. N{\o}rgaard-Nielsen and F. Noviello and D. Novikov and I. Novikov and S. Osborne and C. A. Oxborrow and L. Pagano and F. Pajot and D. Paoletti and F. Pasian and G. Patanchon and O. Perdereau and F. Perrotta and F. Piacentini 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 G. Prezeau and J. Puget and J. Rachen and W. Reach and M. Reinecke and S. Ricciardi and T. Riller and I. Ristorcelli and G. Rocha and C. Rosset and J. Rubino-Mart'in and B. Rusholme and D. Santos and G. Savini and D. Scott and M. Seiffert and E. Shellard and L. Spencer and R. Sunyaev and F. Sureau and A. Suur-Uski and J. Sygnet and J. Tauber and D. Tavagnacco and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and M. Tucci and M. Turler and L. Valenziano and J. Valiviita and B. Tent and P. Vielva and F. Villa and N. Vittorio and L. Wade and B. Wandelt and M. White and D. Yvon and A. Zacchei and J. P. Zibin and A. Zonca}, journal={Astronomy and Astrophysics}, year={2013}, volume={571}, pages={27} }

Our velocity relative to the rest frame of the cosmic microwave background (CMB) generates a dipole temperature anisotropy on the sky which has been well measured for more than 30 years, and has an accepted amplitude of v=c = 1:23 10 3 , or v = 369 km s 1 . In addition to this signal generated by Doppler boosting of the CMB monopole, our motion also modulates and aberrates the CMB temperature fluctuations (as well as every other source of radiation at cosmological distances). This is an order… Expand

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