Notes. The columns are as follows: (1) source name; (2) source designation in the Elia et al. (2021) Hi-GAL catalogue; (3) projected angular separation between the LABOCA 870 µm peak position of our source and the Hi-GAL catalogue position; (4) source distance in the Hi-GAL catalogue (not available for clump A in G1.75-0.08 and clumps A and C in G11.36+0.80); (5) circularised and beam-deconvolved FWHM size measured from the Herschel/SPIRE 250 µm image; (6) total clump mass derived from fitting the source SED, and where a hypothetical distance of 1 kpc was used for sources with unavailable distance; (7) dust temperature derived from the SED fit; and (8) bolometric luminosity derived by integrating the SED from λ = 21 µm to λ = 1.1 mm, where again a distance of 1 kpc was assumed if it was not available.