Notes. Columns list the name of the star, interferometric inner dust radius, distance based on Gaia EDR3 parallaxes, inner dust radius in spatial scale derived combining r_in (mas) and d (pc), stellar luminosity, temperature, radius, and mass. The main references – not indicated with a superscript – are this work (Col. 2 for the first five stars), GRAVITY Collaboration (2019; Col. 2 for the following 23 stars up to V1818 Ori), GD21 (Cols. 3, 5, 7, and 8), and Wichittanakom et al. (2020; Col. 6). Additional references are ⁽¹⁾Eisner et al. (2004), ⁽²⁾Monnier et al. (2005), ⁽³⁾Kraus et al. (2008), ⁽⁴⁾Tatulli et al. (2011), ⁽⁵⁾Davies et al. (2018), ⁽⁶⁾Millan-Gabet et al. (2001), ⁽⁷⁾Benisty et al. (2010), ⁽⁸⁾Setterholm et al. (2018), ⁽⁹⁾Kluska et al. (2018),⁽¹⁰⁾Hone et al. (2019), ⁽¹¹⁾Danchi et al. (2001), ⁽¹²⁾Malbet et al. (2007), ⁽¹³⁾Weigelt et al. (2011), ⁽¹⁴⁾Kraus et al. (2012b), ^(a)Fairlamb et al. (2015), and ^(b)GD21. For the sources with more than one value of r_in available, the most recent estimate is provided when there are not variations within the errorbars (italics), and an averaged value for the rest (parentheses). Errorbars in the latter cases serve to quantify the ranges provided in the literature. The log L_* value for V590 Mon has been re-scaled from the distance in Fairlamb et al. (2015) to the current Gaia EDR3 distance (Sect. 3.1). Distances tagged with ^(†)may be affected by some degree of spuriousness (see text, and GD21 for details).