Planck intermediate results LII. Planet flux densities

@article{Akrami2016PlanckIR,
  title={Planck intermediate results LII. Planet flux densities},
  author={Planck Collaboration Y. Akrami and Mark Ashdown and J. Aumont 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 Laura Bonavera and J. Richard Bond and Julian Borrill and Francois R. Bouchet and Francois Boulanger and Manfred Bucher and Carlo Burigana and R. C. Butler and Erminia Calabrese and J.-F. Cardoso and Julien Carron and H. C. Chiang and Loris P. L. Colombo and Barbara Comis and François Couchot and A. Coulais and Brendan P. Crill and A. Fernandez Curto and F. Cuttaia and Paolo Bernardis and Alessandra De Rosa and Gianfranco De Zotti and Jacques Delabrouille and Eleonora Di Valentino and Clive Dickinson and Jose M. Diego and Olivier Dor'e and Anne Ducout and Xavier Dupac and Franz Elsner and Torsten A. Ensslin and Hans Kristian Eriksen and Edith Falgarone and Yabebal T. Fantaye and Fabio Finelli and Marco Frailis and Aur'elien A. Fraisse 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 F. K. Hansen and George Helou and Sophie Henrot-Versill'e and Diego Herranz and Eric Hivon 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 Guilaine Lagache and J-M. Lamarre and Anthony N. Lasenby and Massimiliano Lattanzi and Charles R. Lawrence and Maude Le Jeune and Emmanuel Lellouch and François L{\'e}vrier and Michele Liguori and Per B. Lilje and V. Lindholm and Marcos L'opez-Caniego and Y.-Z. Ma and Juan-Fancisco Mac'ias-P'erez and Gianmarco Maggio and Davide Maino and Nazzareno Mandolesi and Michele Maris and P. G. Martin and E. Mart'inez-Gonz'alez and S. Matarrese and Nicoletta Mauri and Jason D. McEwen and Alessandro Melchiorri and Aniello Mennella and Marina Migliaccio and Marc-Antoine Miville-Desch{\^e}nes and Diego Molinari and Andrea Moneti and Ludovic Montier and Raphael Moreno and G. Morgante and Paolo Natoli and Carol Anne Oxborrow and Daniela 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 Graca M. Rocha and Erik Romelli and C. Dutruc Rosset and Gael M. Roudier and Jos'e Alberto Rubino-Mart'in and Beatriz Ruiz-Granados and Laura Salvati and M. Sandri and Matti Savelainen and Douglas Scott and G. Sirri and Locke D Spencer and A.-S. Suur-Uski and Jan Tauber and Daniele Tavagnacco and M. Tenti and Luigi Toffolatti and Maurizio Tomasi and M. Tristram and Tiziana 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},
  year={2016},
  volume={607},
  pages={1-20}
}
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… 
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References

SHOWING 1-10 OF 103 REFERENCES
Far-infrared photometric observations of the outer planets and satellites with Herschel-PACS
We present all Herschel PACS photometer observations of Mars, Saturn, Uranus, Neptune, Callisto, Ganymede, and Titan. All measurements were carefully inspected for quality problems, were reduced in a
SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: PLANETS AND CELESTIAL CALIBRATION SOURCES
We present WMAP seven-year observations of bright sources which are often used as calibrators at microwave frequencies. Ten objects are studied in five frequency bands (23–94 GHz): the outer planets
The near-millimeter brightness temperature spectra of Uranus and Neptune
We present new photometric measurements of Uranus and Neptune between 0.35 and 2.0 mm. Together with our previous results (Orton et al., 1986, Icarus 67, 289-304), these data have allowed us to
The Herschel-SPIRE submillimetre spectrum of Mars
We have obtained the first continuous disk averaged spectrum of Mars from 450 to 1550 Ghz using the Herschel-SPIRE Fourier-transform spectrometer. The spectrum was obtained at a constant resolution
Long-term observations of Uranus and Neptune at 90 GHz with the IRAM 30 m telescope
Context. The planets Uranus and Neptune with small apparent diameters are primary calibration standards. Aims. We investigate their variability at ∼90 GHz using archived data taken with the IRAM 30 m
THE ATACAMA COSMOLOGY TELESCOPE: BEAM MEASUREMENTS AND THE MICROWAVE BRIGHTNESS TEMPERATURES OF URANUS AND SATURN
We describe the measurement of the beam profiles and window functions for the Atacama Cosmology Telescope (ACT), which operated from 2007 to 2010 with kilopixel bolometer arrays centered at 148, 218,
143 GHz BRIGHTNESS MEASUREMENTS OF URANUS, NEPTUNE, AND OTHER SECONDARY CALIBRATORS WITH BOLOCAM BETWEEN 2003 AND 2010
Bolocam began collecting science data in 2003 as the long-wavelength imaging camera at the Caltech Submillimeter Observatory. The planets, along with a handful of secondary calibrators, have been
Planck 2015 results - X. Diffuse component separation: Foreground maps
Planck has mapped the microwave sky in temperature over nine frequency bands between 30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz in polarization. In this
Planck 2015 results: XXVI. The Second Planck Catalogue of Compact Sources
The Second Planck Catalogue of Compact Sources is a list of discrete objects detected in single-frequency maps from the full duration of the Planck mission and supersedes previous versions. It
...
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