Notes. From left to right: the observing night, the number of observed spectra, the exposure time, the average S/N across the selected spectral range (1082.49–1085.5 nm), the uncertainty on the mid-transit time for the observed transits calculated as ${\sigma }_{{\text{T}}_{\text{c}}}=\sqrt{{\sigma }_{{\text{T}}_0}^2+n^2\ast {\sigma }_{\text{P}}^2}$ (where T₀ and P are the mid-transit time and orbital period in the adopted ephemerids reported in Table A.1 and n is the number of orbits between times T_c and T₀), and flag for significant telluric overlap/possible stellar activity issues. ⁽⁺⁾Beginning of the night.