Figure 2 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 2.

Relative shifts of the telluric lines compared to those in the first frame in the blue CCD (1) and red CCD (2). Noticeably, the general trend of the shift follows the trend of temperature variation inside the dome (solid red line).

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