Figure 5 from High-resolution Spectroscopic Detection of TiO and a Stratosphere in the Day-side of WASP-33b

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High-resolution Spectroscopic Detection of TiO and a Stratosphere in the Day-side of WASP-33b

Authors: Stevanus K. Nugroho, Hajime Kawahara, Kento Masuda, Teruyuki Hirano, Takayuki Kotani, and Akito Tajitsu

2017 The Astronomical Journal 154 221.

Provider: AAS Journals

Caption: Figure 5.

WASP-33b spectrum model using the T/P profile of Haynes et al. (2015). The left panel shows the WASP-33b model spectrum with various VMRs. The vertical axis shows the planet to star flux contrast in the level of 10⁻³. The right panel shows our adopted temperature profile for the WASP-33b atmosphere.

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