The 4.5 mm full-orbit phase curve of the hot Jupiter HD 209458b

The 4.5 mm full-orbit phase curve of the hot Jupiter HD 209458b

The hot Jupiter HD 209458b is particularly amenable to detailed study as it is among the brightest transiting exoplanet systems currently known (V-mag = 7.65; K-mag = 6.308) and has a large planet-to-star contrast ratio. HD 209458b is predicted to be in synchronous rotation about its host star with...

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Bibliographic Details
Main Authors: Zellem, Robert T. (Author), Knutson, Heather A. (Author), Griffith, Caitlin A. (Author), Showman, Adam P. (Author), Fortney, Jonathan J. (Author), Cowan, Nicolas B. (Author), Agol, Eric (Author), Burrows, Adam (Author), Charbonneau, David (Author), Deming, Drake (Author), Laughlin, Gregory (Author), Langton, Jonathan (Author), Lewis, Nicole (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-01-12T19:44:06Z.
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