Ratio between averaged surface density inside the gaps in our hydrodynamical simulations ∑_gap,hydro and the surface density estimated from different criteria ∑_{gap, criterion}. In red are the estimates from Kanagawa et al. (2015), in orange those from Pichierri et al. (2023) and in brown those from Fung et al. (2014). Circles represent the cases where m_p = 0.5 M_J, upward triangles are for m_p = 1 M_J, and downward triangles are for m_p = 5 M_J. We see that the different criteria fail to reproduce our gap depth the further away the planet is located. For the planet located at 10 AU, the criteria fail to reproduce the m_p = 5 M_J case as the planets become eccentric, changing their gap opening.