Notes. Columns show the disk type, the distance (d), the spectral type (SpT), the stellar mass (M_*) and luminosity (L_*), the accretion luminosity (L_acc) and the accretion rate onto the central star (${\dot{\mathrm{M}}}_{\text{acc}}$), the X-ray luminosity, and the outer disk inclination (inc.). The last column reports the references for the stellar luminosity, the accretion luminosity, the accretion rates, and the X-ray luminosity. Distances are from Gaia DR2 (Gaia Collaboration 2018). The inclinations of the outer disks are from Francis & van der Marel 2020 and Long et al. (2019). The uncertainty on the stellar luminosity is assumed to be 0.20 dex, based on the typical uncertainty estimated by Wichittanakom et al. (2020).^† The accretion luminosity on these targets is calculated starting from the reported accretion rate and using equation (2) in Wichittanakom et al. (2020), with uncertainties assumed to be 0.25 dex (Manara et al. 2023). ^‡ X-ray luminosities are derived by correcting the fluxes reported in Table 4 in Dionatos et al. 2019 for the distance of each target and assuming a 0.30 dex uncertainty (Güdel et al. 2007). References: 1) Gangi et al. (2022), 2) Harsono et al. (2024), 3) Simon et al. (2016), 4) Ricci et al. (2010), 5) Pascucci et al. (2020) 6) Dionatos et al. 2019, 7) Vioque et al. 2018, 8) Wichittanakom et al. 2020, 9) Francis & van der Marel 2020, 10) Ryspaeva et al. 2023, 11) Herczeg et al. 2023, 12) Varga et al. 2021.