Top panel: ESPRESSO and HARPS radial velocities of GJ 1018. The purple solid line indicates the median posterior global model, and the black and gray solid lines indicate the median posterior GP and Keplerian models, respectively. The shaded purple region indicates the 68.7% confidence interval of the global model. Bottom panel: ESPRESSO and HARPS RVs (left) and TESS photometry (right) subtracted from their corresponding GP components and folded to the orbital period of TOI-244 b. The solid lines indicate the median posterior models.