Figure 12 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 12.

Standard deviation of the spectrum of each order with their corresponding optimized SYSREM iteration number. The blue cross and the red circle indicate the spectrum in the blue and red CCDs, respectively. The value of the standard deviation represents the amount of telluric and/or stellar line contamination for every order.

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