Comparison of accretion parameters as a function of stellar properties from our X-Shooter sample of Orion Nebula sources and the sample of different nearby SFRs (transparent circles) presented in Manara et al. (2023). The marker scheme for our sample is the same as in Figure 3. Left panel: Accretion luminosity as a function of stellar luminosity as obtained using FRAPPE. The black lines indicate L_acc equal to 1L_⋆, 0.1L_⋆, and 0.01L_⋆. The error bars indicate the typical uncertainties on the stellar and accretion luminosities (∼0.2 dex and 0.25 dex, respectively). Right panel: Mass accretion rate as a function of stellar mass as obtained using FRAPPE. Literature targets with arrows pinpoint upper limits. The error bars indicate the typical uncertainties on the mass accretion rate and stellar mass (∼0.35 dex and 0.1 dex, respectively).