Transiting exoplanets from the CoRoT space mission XVI. CoRoT-14b: an unusually dense very hot Jupiter

@article{Tingley2011TransitingEF,
  title={Transiting exoplanets from the CoRoT space mission XVI. CoRoT-14b: an unusually dense very hot Jupiter},
  author={Brandon Tingley and Michael Endl and J. C. Gazzano and Roi Alonso and Tsevi Mazeh and Laurent Jorda and Suzanne Aigrain and Jose M. Almenara and Michel Auvergne and Annie Baglin and Pierre Barge and Aldo Stefano Bonomo and P. Bord'e and François Bouchy and Hans Bruntt and J. Cabrera and Stefania Carpano and Ludmila Carone and William D. Cochran and Sz. Csizmadia and Magali Deleuil and Hans J. Deeg and Rudolf Dvorak and Anders Erikson and Sylvio Ferraz-Mello and Malcolm Fridlund and Davide Gandolfi and Micha{\"e}l Gillon and E. W. Guenther and Tristan Guillot and A. P. Hatzes and Guillaume H'ebrard and Alain L'eger and Antoine Llebaria and Helmut Lammer and Christophe Lovis and Phillip J. MacQueen and Claire Moutou and Marc Ollivier and Aviv Ofir and Martin Patzold and Francesco A. Pepe and Didier Queloz and Heike Rauer and Daniel Rouan and Benjamin Samuel and Jodi Schneider and Avi Shporer and G{\"u}nther Wuchterl},
  journal={Astronomy and Astrophysics},
  year={2011},
  volume={528},
  pages={97}
}
In this paper, the CoRoT Exoplanet Science Team announces its 14th discovery. Herein, we discuss the observations and analyses that allowed us to derive the parameters of this system: a hot Jupiter with a mass of 7.6 ± 0.6 Jupiter masses orbiting a solar-type star (F9V) with a period of only 1.5 d, less than 5 stellar radii from its parent star. It is unusual for such a massive planet to have such a small orbit: only one other known higher mass exoplanet orbits with a shorter period. 
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