Extended Data Fig. 5: Signals of Cr+, Sc+, Na, Ni and Ca classified as tentative.
From: Titanium oxide and chemical inhomogeneity in the atmosphere of the exoplanet WASP-189 b

All of these species have previously been observed in other ultra-hot Jupiters19,25. The shaded region indicates the expected 1σ uncertainty. Dashed lines show expected signal strengths, obtained by injecting and recovering the signatures of model spectra, assuming isothermal atmospheres at 2,000 K (red) and 3,000 K (orange) respectively.