CONFIRMATION OF HOT JUPITER KEPLER-41b VIA PHASE CURVE ANALYSIS

CONFIRMATION OF HOT JUPITER KEPLER-41b VIA PHASE CURVE ANALYSIS

We present high precision photometry of Kepler-41, a giant planet in a 1.86 day orbit around a G6V star that was recently confirmed through radial velocity measurements. We have developed a new method to confirm giant planets solely from the photometric light curve, and we apply this method herein t...

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Main Authors: Quintana, Elisa V. (Author), Rowe, Jason F. (Author), Barclay, Thomas (Author), Howell, Steve B. (Author), Ciardi, David R. (Author), Demory, Brice-Olivier (Contributor), Caldwell, Douglas A. (Author), Borucki, William J. (Author), Christiansen, Jessie L. (Author), Jenkins, Jon M. (Author), Klaus, Todd C. (Author), Fulton, Benjamin J. (Author), Morris, Robert L. (Author), Sanderfer, Dwight T. (Author), Shporer, Avi (Author), Smith, Jeffrey C. (Author), Still, Martin (Author), Thompson, Susan E. (Author)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-01-29T18:27:30Z.
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