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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 11.

﹩{S}_{\max }/n﹩ of all orders for various SYSREM iteration numbers. The vertical lines mark the SYSREM iteration number that made the signal strength optimum. The blue circle, yellow asterisk, green diamond, red square, and purple cross are the ﹩{S}_{\max }/n﹩ of the recovered injected signal with sc = [0.2, 0.4, 0.6, 0.8, 1.0], respectively. The number in the white box at the bottom left of each panel represents the order number and the color represents the CCD (blue or red).

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