153 citations · 884 across the 11 of their papers we have counts for
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3.6 and 4.5 m Phase Curves of the Highly-Irradiated Hot Jupiters WASP-19b and HAT-P-7b
Ian Wong, Heather A. Knutson, Tiffany Kataria +15
We analyze full-orbit phase curve observations of the transiting hot Jupiters WASP-19b and HAT-P-7b at 3.6 and 4.5 m obtained using the Spitzer Space Telescope. For WASP-19b, we…
Inferring Planetary Obliquity Using Rotational & Orbital Photometry
Joel C. Schwartz, Clara Sekowski, Hal M. Haggard +2
The obliquity of a terrestrial planet is an important clue about its formation and critical to its climate. Previous studies using simulated photometry of Earth show that continuou…
3.6 and 4.5 m Phase Curves of the Highly-Irradiated Eccentric Hot Jupiter WASP-14b
Ian Wong, Heather A. Knutson, Nikole K. Lewis +14
We present full-orbit phase curve observations of the eccentric () transiting hot Jupiter WASP-14b obtained in the 3.6 and 4.5 m bands using the \textit{Spitzer Spac…
Balancing the Energy Budget of Short-Period Giant Planets: Evidence for Reflective Clouds and Optical Absorbers
Joel C. Schwartz, Nicolas B. Cowan
We consider fifty transiting short-period giant planets for which eclipse depths have been measured at multiple infrared wavelengths. The aggregate dayside emission spectrum of the…