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 Journal154221.
Provider: AAS Journals
Caption: Figure 10.
S/N of peaks A and B along the SYSREM iteration number, ﹩{N}_{\mathrm{sys}}﹩, for H-spec (log VMR = −8). The blue diamond line is the S/N of peak A and the red circle dotted line is the S/N of peak B.