Notes. Columns show the star coordinates; distance, d; spectral type, SpT; stellar mass, M_* ; and luminosity, L_*; accretion luminosity, ; accretion rate onto the central star, Ṁ ; X-ray luminosity; and the outer disk inclination, inc. The last column reports the references for the luminosity, accretion luminosity, accretion rates, and X-ray luminosity. Distances are from Gaia DR2 (Gaia Collaboration 2018). The inclination of the outer disks are from Francis & van der Marel (2020) and their typical uncertainty is in the range of a few degrees. ^(*)The uncertainty on the luminosity for these targets 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 with Eq. (2) in Wichittanakom et al. (2020), with uncertainties assumed to be 0.25 dex (Manara et al. 2023).^(‡) X-ray luminosities derived 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) Vioque et al. (2018), (2) Wichittanakom et al. (2020), (3) Francis & van der Marel (2020), (4) Manara et al. (2023), (5) Dionatos et al. (2019), (6) Ryspaeva et al. (2023).