SPITZER PHASE CURVE CONSTRAINTS FOR WASP-43b AT 3.6 AND 4.5μm

SPITZER PHASE CURVE CONSTRAINTS FOR WASP-43b AT 3.6 AND 4.5μm

Previous measurements of heat redistribution efficiency (the ability to transport energy from a planet's highly irradiated dayside to its eternally dark nightside) show considerable variation between exoplanets. Theoretical models predict a positive correlation between heat redistribution effic...

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Bibliographic Details
Main Authors: Stevenson, Kevin B., Line, Michael R., Bean, Jacob L., Désert, Jean-Michel, Fortney, Jonathan J., Showman, Adam P., Kataria, Tiffany, Kreidberg, Laura, Feng, Y. Katherina
Other Authors: Univ Arizona, Dept Planetary Sci
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
planetary systems
stars: individual (WASP-43)
techniques: photometric
Online Access:http://hdl.handle.net/10150/623051
http://arizona.openrepository.com/arizona/handle/10150/623051

Internet

http://hdl.handle.net/10150/623051
http://arizona.openrepository.com/arizona/handle/10150/623051

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