3.6 AND 4.5 μm SPITZER PHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

We analyze full-orbit phase curve observations of the transiting hot Jupiters WASP-19b and HAT-P-7b at 3.6 and 4.5 mu m, obtained using the Spitzer Space Telescope. For WASP-19b, we measure secondary eclipse depths of 0.485% +/- 0.024% and 0.584% +/- 0.029% at 3.6 and 4.5 mu m, which are consistent...

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Bibliographic Details
Main Authors:	Wong, Ian, Knutson, Heather A., Kataria, Tiffany, Lewis, Nikole K., Burrows, Adam, Fortney, Jonathan J., Schwartz, Joel, Shporer, Avi, Agol, Eric, Cowan, Nicolas B., Deming, Drake, Désert, Jean-Michel, Fulton, Benjamin J., Howard, Andrew W., Langton, Jonathan, Laughlin, Gregory, Showman, Adam P., Todorov, Kamen
Other Authors:	Univ Arizona, Lunar & Planetary Lab
Language:	en
Published:	IOP PUBLISHING LTD 2016
Subjects:	planetary systems stars individual (WASP-19 and HAT-P-7) techniques photometric
Online Access:	http://hdl.handle.net/10150/621241 http://arizona.openrepository.com/arizona/handle/10150/621241

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http://hdl.handle.net/10150/621241
http://arizona.openrepository.com/arizona/handle/10150/621241

3.6 AND 4.5 μm SPITZER PHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

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