WASP-38b: a transiting exoplanet in an eccentric, 6.87d period orbit

@article{Barros2010WASP38bAT,
  title={WASP-38b: a transiting exoplanet in an eccentric, 6.87d period orbit},
  author={S. C. C. Barros and Francesca Faedi and Andrew Collier Cameron and Tim A. Lister and J. McCormac and Don Pollacco and Elaine Simpson and Barry Smalley and Rachel A. Street and Ian Todd and A. H. M. J. Triaud and Isabelle Boisse and François Bouchy and Guillaume H{\'e}brard and Claire Moutou and Francesco A. Pepe and Didier Queloz and Alexandre Santerne and Damien S{\'e}gransan and St{\'e}phane Udry and Joao Bento and Oliver Butters and B E Enoch and Carole A. Haswell and Coel Hellier and Francis P. Keenan and Grant R. M. Miller and V. E. Moulds and Andrew J. Norton and Neil R. Parley and Ibm Watson and Richard G. West and Peter J. Wheatley and Queen's University of Belfast and University of St. Andrews and Las Cumbres Observatory Global Telescope Network and Keele University and Observatoire de Geneve and Institut d'Astrophysique de Paris and Observatoire de Haute-Provence and Universit'e d'Aix-Marseille and University of Warwick and University of Leicester and The Open University and Isaac Newton Group},
  journal={Astronomy and Astrophysics},
  year={2010},
  volume={525},
  pages={1-6}
}
Aims. We report the discovery of WASP-38b, a long period transiting planet in an eccentric 6.871815 day orbit. The transit epoch is 2455335.92050�0.00074 (HJD) and the transit duration is 4.663 hours. Methods. WASP-38b’s discovery was enabled due to an upgrade to the SuperWASP-North cameras. We performed a spectral analysis of the host star HD 146389/BD+10 2980 that yielded Te f f = 6150� 80 K, log g= 4.3� 0.1, v sin i=8.6� 0.4 km s −1 , M�= 1.16� 0.04 M� and R�= 1.33�0.03 R�, consistent with a… 

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