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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 17.

Significance map after converting from the p-value from Welch’s t-test using the erf function for the most significant detected signal with the H-spec model spectrum of log VMRTiO = −8. The black dashes show the most significant signal, the white dashes show the expected Kp and Vsys, and the color bar grid interval is 1σ, and the white area also represents the 1σ error of the detected signal.

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