Notes. Distances of the source, stellar masses and luminosities are taken from the references listed in Francis & van der Marel (2020), with the exception of CQ Tau (Gaia Collaboration 2021; Vioque et al. 2018), V883 Ori (Furlan et al. 2016), HL Tau (Liu et al. 2017; Yen et al. 2019).^(a) An asterisk beside t_ex indicates that the temperature was assumed, rather then measured via a rotational diagram. ^(b) The first column lists the references from which the methanol column densities and the methanol excitation temperatures are taken from. The second column contains the publications where the DALI models parameters are described. Additionally, other thermochemical models are presented in: HD 100546 (Keyte et al. 2023) and IRS 48 (Bruderer et al. 2014; van der Marel et al. 2016, 2021). No thermochemical model was available for the disk HD 100453.^(c) Due to the detection of just one methanol line in the CQ Tau disk, Booth et al. (2026) report only the value of the integrated CH₃OH line flux.

References. (1) Ilee et al. (2026); (2) Kama et al. (2016); (3) Evans et al. (2025); (4) Leemker et al. (2024); (5) Booth et al. (2023); (6) Keyte et al. (2024); (7) Booth et al. (2025); (8) van der Marel et al. (2021); (9) Leemker et al. (2023); (10) Tobin et al. (2023); (11) Leemker et al. (2021); (12) This work; (13) Leemker et al. (2026);