Notes. For each star in Col. 1, the remaining columns list the metallicity, projected rotational velocity, inclination, rotational period, Hα equivalent width (corrected for photospheric absorption; the nominal error bars are ∼10% for the King (1993) sources (see Table 1) and lower than 0.01 Å for the rest), accretion luminosity, mass accretion rate, Li I equivalent width (corrected for blending with the adjacent Fe I6707.43 transition), Li abundance, and the deviation from local thermodynamical equilibrium (Δ = A(Li)_non-LTE − A(Li)_LTE). The full table is available electronically at the CDS. [Fe/H] and v sin i values were taken from Guzmán-Díaz et al. (2023) and King (1993) when available (see Table 1). References for the inclinations are ¹Hughes et al. (2017), ²Pinilla et al. (2022), ³Long et al. (2019), ⁴Tanii et al. (2012), ⁵Labdon et al. (2023), ⁶Piétu et al. (2006), ⁷Kreplin et al. (2016), ⁸de Boer et al. (2021), ⁹Valegård et al. (2024), ¹⁰Davies et al. (2018b), ¹¹Lazareff et al. (2017), ¹²Ginski et al. (2024), ¹³Benisty et al. (2017), ¹⁴Jamialahmadi et al. (2018), ¹⁵Cazzoletti et al. (2018), ¹⁶Muro-Arena et al. (2020), ¹⁷Weinberger et al. (1999), ¹⁸Davies et al. (2018a), ¹⁹Benisty et al. (2018), ²⁰Chen et al. (2012), ²¹Benisty et al. (2011), ²²Muro-Arena et al. (2018), ²³Bertrang et al. (2018), ²⁴Kokoulina et al. (2021).