Transiting exoplanets from the CoRoT space mission - XIV. CoRoT-11b: a transiting massive “hot-Jupiter” in a prograde orbit around a rapidly rotating F-type star

@article{Gandolfi2010TransitingEF,
  title={Transiting exoplanets from the CoRoT space mission - XIV. CoRoT-11b: a transiting massive “hot-Jupiter” in a prograde orbit around a rapidly rotating F-type star},
  author={Davide Gandolfi and Guillaume H'ebrard and Roi Alonso and Magali Deleuil and E. W. Guenther and Malcolm Fridlund and Michael Endl and Philipp Eigmuller and Sz. Csizmadia and Mathieu Havel and Suzanne Aigrain and Michel Auvergne and Annie Baglin and Pierre Barge and Aldo S. Bonomo and P. Bord'e and François Bouchy and Hans Bruntt and Jessica Cabrera and Stefania Carpano and Ludmila Carone and William D. Cochran and Hans J. Deeg and Rudolf Dvorak and Jochen Eisloffel and Anders Erikson and Sylvio Ferraz-Mello and J. C. Gazzano and Neale P. Gibson and Micha{\"e}l Gillon and Ph. Gondoin and Tristan Guillot and Michael Hartmann and A. P. Hatzes and Laurent Jorda and Petr Kabath and Alain L'eger and Antoine Llebaria and Helmut Lammer and Phillip J. MacQueen and Michel Mayor and Tsevi Mazeh and Claire Moutou and Marc Ollivier and Martin Patzold and Francesco A. Pepe and Didier Queloz and Heike Rauer and Daniel Rouan and Benjamin Samuel and Jodi Schneider and B. Stecklum and Brandon Tingley and St{\'e}phane Udry and G{\"u}nther Wuchterl},
  journal={Astronomy and Astrophysics},
  year={2010},
  volume={524},
  pages={55}
}
The CoRoT  exoplanet science team announces the discovery of CoRoT-11b, a fairly massive hot-Jupiter transiting a V  = 12.9 mag F6 dwarf star (M ∗  = 1.27 ± 0.05 M ⊙ , R ∗  = 1.37 ± 0.03 R ⊙ , T eff  = 6440 ± 120 K), with an orbital period of P  = 2.994329 ± 0.000011 days and semi-major axis a  = 0.0436 ± 0.005 AU. The detection of part of the radial velocity anomaly caused by the Rossiter-McLaughlin effect shows that the transit-like events detected by CoRoT  are caused by a planet-sized… Expand
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References

SHOWING 1-10 OF 89 REFERENCES
Transiting exoplanets from the CoRoT space mission . VI. CoRoT-Exo-3b: the first secure inhabitant of the brown-dwarf desert
Context. The CoRoT  space mission routinely provides high-precision photometric measurements of thousands of stars that have been continuously observed for months. Aims. The discovery andExpand
Transiting exoplanets from the CoRoT space mission - IX. CoRoT-6b: a transiting “hot Jupiter” planet in an 8.9d orbit around a low-metallicity star
The CoRoT satellite exoplanetary team announces its sixth transiting planet in this paper. We describe and discuss the satellite observations as well as the complementary ground-based observations ‐Expand
Transiting exoplanets from the CoRoT space mission - XI. CoRoT-8b: a hot and dense sub-Saturn around a K1 dwarf
Aims. We report the discovery of CoRoT-8b, a dense small Saturn-class exoplanet that orbits a K1 dwarf in 6.2 days, and we derive its orbital parameters, mass, and radius. Methods. We analyzed twoExpand
Transiting exoplanets from the CoRoT space mission. II. CoRoT-Exo-2b: a transiting planet around an
Context. The CoRoT mission, a pioneer in exoplanet searches from space, has completed its first 150 days of continuous observations of ∼12 000 stars in the galactic plane. An analysis of the raw dataExpand
Transiting exoplanets from the CoRoT space mission. VII. The ``hot-Jupiter''-type planet CoRoT-5b
Aims. The CoRoT space mission continues to photometrically monitor about 12 000 stars in its field-of-view for a series of target fields to search for transiting extrasolar planets ever since 2007.Expand
Transiting exoplanets from the CoRoT space mission. I. CoRoT-Exo-1b: a low-density short-period plan
Context. The pioneer space mission for photometric planet searches, CoRoT, steadily monitors about 12,000 stars in each of its fields of view; it is able to detect transit candidates early in theExpand
Transiting exoplanets from the CoRoT space mission. IV. CoRoT-Exo-4b: a transiting planet in a 9.2 d
CoRoT, the first space-based transit search, provides ultra-high precision light curves with continuous time-sampling over periods, of up to 5 months. This allows the detection of transiting planetsExpand
Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius
Aims. We report the discovery of very shallow (ΔF/F ≈ 3.4× 10 −4 ), periodic dips in the light curve of an active V = 11.7 G9V star observed by the CoRoT satellite, which we interpret as caused by aExpand
Transiting exoplanets from the CoRoT space mission: III. The spectroscopic transit of CoRoT-Exo-2b with SOPHIE and HARPS
We report on the spectroscopic transit of the massive hot-Jupiter CoRoT-Exo-2b observed with the high-precision spectrographs SOPHIE and HARPS. By modeling the radial velocity anomaly occurringExpand
Line-profile tomography of exoplanet transits - II. A gas-giant planet transiting a rapidly rotating A5 star
TLDR
Photometry and time-series spectroscopy through three separate transits are used to confirm the existence of a gas-giant planet with an orbital period of 1.22 d in orbit around HD 15082, and opens the way to studying the formation of planets around a whole new class of young, early-type stars, hence under different physical conditions and generally in an earlier stage of formation than in sharp-lined late- type stars. Expand
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