Results from cross-correlation with VO (left) and TiO (right) templates, at a log VMR of −6.6 and −7 respectively, for 1500 K. Top row: cross-correlation function time series summed over all echelle orders, showing no visible trace. Middle: cross-correlation maps summed over all echelle orders, showing non-detections for both species: the black dotted lines indicate the expected velocity position for the signal (K_p = 217 km s⁻¹). Bottom: results from injection tests, showing a detection of the injected signal at 6.9σ for VO and 7.2σ for TiO at the expected velocity position. We note that the expected value for v_sys is zero as the spectra have been corrected to the stellar rest frame.