Properties of the WASP-69 disk-integrated CCFs. Colored circles correspond to the best fit of the CCF in individual exposures (colored in red, blue, and green for NIRPS, HARPS, and HARPS-N, respectively). Contrast and FWHM vary over time and have been normalized to their out-of-transit mean for comparison. Plotted measurements have been binned into black diamonds to highlight the overall shape of the RM anomaly (we note that it may differ between instruments due to the different broadband limb-darkening and local stellar line shapes at optical and near-infrared wavelengths). Vertical dashed lines indicate the transit contacts.