Studying the atmosphere of the exoplanet HAT-P-7b via secondary eclipse measurements with EPOXI, Spitzer and Kepler

Studying the atmosphere of the exoplanet HAT-P-7b via secondary eclipse measurements with EPOXI, Spitzer and Kepler

The highly irradiated transiting exoplanet, HAT-P-7b, currently provides one of the best opportunities for studying planetary emission in the optical and infrared wavelengths. We observe six near-consecutive secondary eclipses of HAT-P-7b at optical wavelengths with the EPOXI spacecraft. We place an...

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Bibliographic Details
Main Authors: Seager, Sara, Madhusudhan, Nikku, Christiansen, Jessie L., Ballard, Sarah, Charbonneau, David, Matthew J., Holman, Wellnitz, Dennis D., Deming, Drake, A'Hearn, Michael F., EPOXI team
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: Institute of Physics 2011
Online Access:http://hdl.handle.net/1721.1/60549
https://orcid.org/0000-0002-6892-6948

Internet

http://hdl.handle.net/1721.1/60549
https://orcid.org/0000-0002-6892-6948

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