arXiv · 0707.0958
Elodie metallicity-biased search for transiting Hot Jupiters IV. Intermediate period planets orbiting the stars HD43691 and HD132406
Abstract
We report here the discovery of two planet candidates as a result of our planet-search programme biased in favour of high-metallicity stars, using the ELODIE spectrograph at the Observatoire de Haute Provence. One of them has a minimum mass m_2\sin{i} = 2.5 M_Jup and is orbiting the metal-rich star HD43691 with period P = 40 days and eccentricity e = 0.14. The other planet has a minimum mass m_2\sin{i} = 5.6 M_Jup and orbits the slightly metal-rich star HD132406 with period P = 974 days and eccentricity e = 0.34. Both stars were followed up with additional observations using the new SOPHIE spectrograph that replaces the ELODIE instrument, allowing an improved orbital solution for the systems.
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R. Da Silva, S. Udry, F. Bouchy, C. Moutou, M. Mayor, J. -L. Beuzit, X. Bonfils, X. Delfosse, M. Desort, T. Forveille, F. Galland, G. Hebrard, A. -M. Lagrange, B. Loeillet, C. Lovis, F. Pepe, C. Perrier, F. Pont, D. Queloz, N. C. Santos, D. Segransan, J. -P. Sivan, A. Vidal-Madjar, S. Zucker. 2007-07-06. Elodie metallicity-biased search for transiting Hot Jupiters IV. Intermediate period planets orbiting the stars HD43691 and HD132406. https://doi.org/10.1051/0004-6361:20077314
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