Collection of the CCFs of all species searched for in this study, similar to Fig. 4. The CCFs are organized into two pairs of columns, with the K_p-υ_sys diagram on the left, and the one-dimensional CCF extracted at an orbital velocity of 216.0 km/s (gray lines) or at the orbital velocity at which the CCF peaks (black lines), as in Fig. 4. The values in the top-left corner are the peak position. The orange lines indicate the expected signal of a model spectrum without Ti and TiO and a temperature inversion from 2500 K to 3200 K.