Notes. The bottom part of the table includes the sources for which the dust height could not be constrained. In the first column (“Name”), we indicate a SIMBAD compatible name (2MASS to be added before the names starting with “J”), while the second column (“Adopted”) shows the adopted name in the next tables. In the R_⋆ column, the symbol ^(*) indicates that the reported R_⋆ value is higher than the direct estimate from the literature. It must however not be considered as the true stellar radius as a higher value was only introduced to ensure significantly optically thin/bright models (see Sect. 3.3). The symbol ^(g) in Haro6-5B implies that T_{e f f} and R_⋆ were assumed because Haro6-5B does not have a direct measurement of these parameters and is a K5 star.

References. (1) Andrews et al. (2018); (2) Huang et al. (2018); (3) Clarke et al. (2018); (4) GRAVITY Collaboration (2023); (5) Donati et al. (2020); (6) Law et al. (2022); (7) Long et al. (2018); (8) Huang et al. (2020); (9) Espaillat et al. (2011); (10) Macías et al. (2018); (11) Simon et al. (2019); (12) Villenave et al. (2020); (13) Cieza et al. (2021); (14) Testi et al. (2022); (15) Villenave et al. (2019); (16) Facchini et al. (2020); (17) Donati et al. (2019); (18) Villenave et al. (2022); (19) van Terwisga et al. (2018); (20) Loomis et al. (2017); (21) Francis & van der Marel (2020); (22) Alcalá et al. (2017); (23) Manara et al. (2023); (24) Pinte et al. (2016); (25) Beck et al. (2010); (26) Stephens et al. (2023); (27) Keppler et al. (2018); (28) Haffert et al. (2019); (29) Ribas et al. (2024); (30) Mendigutía et al. (2011); (31) Mendigutía et al. (2013); (32) Kudo et al. (2018); (33) Hashimoto et al. (2021); (34) Martire et al. (2024)