Distribution of accretion luminosities and mass accretion rates derived for YSO H emitters within 500 pc. Different lines trace the quality filters described in Sect. 2.7 (see Fig. 2). The left panels present accretion properties obtained using the GSP-Phot extinction correction and the right panels the ones obtained using the med-GSP-Phot extinction correction (Sect. 2.4). We have added to this plot the accretion luminosities and mass accretion rates presented in Manara et al. (2023) for well-characterised T Tauri stars from higher-resolution spectroscopy. The central panels are cumulative distributions of the accretion properties shown on left panels, using GSP-Phot extinction.