Figure 16 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.

Caption: Figure 16.

Q–Q plot of the out-of-trail distribution which shows that the distribution is Gaussian until 4σ.