Planck intermediate results LII. Planet flux densities

  title={Planck intermediate results LII. Planet flux densities},
  author={Planck Collaboration Y. Akrami and M. Ashdown and Jonathan Aumont and Carlo Baccigalupi and Mario Ballardini and Anthony J. Banday and R. B. Barreiro and Nicola Bartolo and Sagarika Basak and Karim Benabed and J. -P. Bernard and M. Bersanelli and Pawel Bielewicz and Laura Bonavera and J. R. Bond and Julian Borrill and François R. Bouchet and Françcois Boulanger and M. Bucher and Carlo Burigana and Rush C. Butler and Erika Calabrese and J. F. Cardoso and Julien Carron and Huan-ching Chiang and Loris P. L. Colombo and Barbara Comis and François Couchot and A. Coulais and B. P. Crill and A. Curto and F. Cuttaia and P. de Bernardis and Alessandra de F{\'a}tima Galv{\~a}o Rosa and Gianfranco de Zotti and Jacques Delabrouille and Eleonora Di Valentino and Clive Dickinson and Javier Diego and Olivier Dor'e and Anne Ducout and Xavier Dupac and Franz Elsner and T. A. Ensslin and Hans Kristian Eriksen and Edith Falgarone and Y. Fantaye and Fabio Finelli and Marco Frailis and Aurelien A. Fraisse and Enrico Franceschi and Andrei V. Frolov and S. Galeotta and S. Galli and Ken Ganga and Ricardo G'enova-Santos and Martina Gerbino and Joaqu{\'i}n Gonz{\'a}lez-Nuevo and Krzysztof G{\'o}rski and Alessandro Gruppuso and Jon Emil Gudmundsson and Frode K. Hansen and George Helou and Sophie Henrot-Versill'e and Diego Herranz and Eric F. Hivon and Andrew H. Jaffe and Walter Clifford Jones and Elina Keihanen and Reijo Keskitalo and Kimmo Kiiveri and Jae-young Kim and T. S. Kisner and Nicoletta Krachmalnicoff and Martin Kunz and Hannu Kurki-Suonio and Guilaine Lagache and J.-M. Lamarre and Anthony Lasenby and Massimiliano Lattanzi and Charles Lawrence and M. Le Jeune and Emmanuel Lellouch and François Levrier and Michele Liguori and Per B. Lilje and Valtteri Lindholm and Marcos L{\'o}pez-Caniego and Y.-Z. Ma and J. F. Mac'ias-P'erez and Gianmarco Maggio and Davide Maino and N. Mandolesi and M. Maris and Peter George Martin and Enrique Martinez-Gonzalez and S. Matarrese and Nicoletta Mauri and Jason D. McEwen and Alessandro Melchiorri and Aniello Mennella and Maurizio Migliaccio and M.-A. Miville-Desch{\^e}nes and Daniele Molinari and Andrea Moneti and Laurent Montier and R. Moreno and Gianluca Morgante and Paolo Natoli and Carol Anne Oxborrow and Daniela L. Paoletti and Bruce Partridge and Guillaume Patanchon and Laura Patrizii and Olivier Perdereau and Francesco Piacentini and St{\'e}phane Plaszczynski and Gianluca Polenta and Jorg P. Rachen and Ben Racine and Martin Reinecke and Mathieu Remazeilles and Alessandro Renzi and Graça Rocha and E. Romelli and Christoph Rosset and Gael M. Roudier and Jos{\'e} Alberto Rubi{\~n}o-Mart{\'i}n and Beatriz Ruiz-Granados and Laura Salvati and Matteo Sandri and Matti Savelainen and Douglas Scott and Gabriele Sirri and Locke D. Spencer and A.-S. Suur-Uski and Joshua A. Tauber and Daniele Tavagnacco and Marco Tenti and L. Toffolatti and Maurizio Tomasi and Matthieu Tristram and Tullio Trombetti and Jussi Valiviita and F. Van Tent and Patricio Vielva and Fabrizio Villa and Ingunn Kathrine Wehus and Andrea Zacchei},
  journal={Astronomy and Astrophysics},
  • Planck Collaboration Y. Akrami, M. Ashdown, +146 authors Andrea Zacchei
  • Published 2016
  • Physics
  • Astronomy and Astrophysics
  • Measurements of flux density are described for five planets, Mars, Jupiter, Saturn, Uranus, and Neptune, across the six Planck High Frequency Instrument frequency bands (100‐857 GHz) and these are then compared with models and existing data. In our analysis, we have also included estimates of the brightness of Jupiter and Saturn at the three frequencies of the Planck Low Frequency Instrument (30, 44, and 70 GHz). The results provide constraints on the intrinsic brightness and the brightness… CONTINUE READING


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