Data for the star GJ 1002, combining ESPRESSO and CARMENES spectroscopy, and SNO V-band photometry. The four upper panels include the V-band photometry data with the best model fit (top left), the periodogram of the data (top right), the residuals after the fit (bottom left) and the periodogram of the residuals. The four lower panels include the FWHM data of ESPRESSO (teal symbols) and CARMENES (purple symbols) with the best model fit (top left), a zoom to the last ESPRESSO campaign (top right), the residuals after the fit (bottom left) and the periodogram of the residuals. The computation of the periodogram uses the offsets and the jitters estimated for model 0-Planets in Table B.1.