HARPS RVs (left) and TESS photometry (right) subtracted from the linear drift and GP component, and folded to the orbital period of TOI- 5005 b. The black error bars represent the instrument uncertainties and the grey error bars represent the total uncertainties obtained by quadratically adding the corresponding jitter term. The red solid lines indicate the median posterior models. In the HARPS RVs plot we also include 100 random posterior models that illustrate the level of modelling uncertainty.