Notes. Columns are: clumps Galactic name, heliocentric distance (Dist.), bolometric luminosity (L_bol), clump mass (M_clump), the peak H₂ column density [N(H₂)], mean volume density () and mean mass surface density (Σ) at FWHM level (i.e., within the 50% contour), the associations with methanol maser (CH₃OH), water maser (H₂O), and SiO emission. These physical properties are taken from Urquhart et al. (2018) and Urquhart et al. (2022), with uncertainties of a factor of a few. The information of maser associations are from Billington et al. (2020), with the detection levels of 15–167 mJy (1σ) for H₂O (Walsh et al. 2011, 2014) and ~170 mJy (1σ) for CH₃OH maser (Green et al. 2009). The SiO data are collected from the SEDIGISM survey and the literature (Harju et al. 1998; Csengeri et al. 2016; Stroh et al. 2019), with sensitivities of ~ 0.8 K (Schuller et al. 2017), ~0.03–0.07 K (Harju et al. 1998), 15–30 mK (Csengeri et al. 2016), and 14 mJy beam⁻¹ (Stroh et al. 2019). The symbol “Y” means maser detections. − means no measurements, whilst “N” means no detections. Only a small part of the table is presented here with the full version available from CDS.