Comparison between COM abundances with respect to CH₃OH measured towards the Clump and literature values towards L1544 (LMPSC; Vastel et al. 2014; Bizzocchi et al. 2014; Jiménez-Serra et al. 2016; Vastel et al. 2019), TMC-1 (dark clouds; Gratier et al. 2016; Cabezas et al. 2021; Agúndez et al. 2025), I00117-MM2 and G11.11 (high-mass cores and/or IRDCs; Vasyunina et al. 2014; Fontani et al. 2015; Mininni et al. 2021), IRAS 16293B (hot corino) and G32.41+0.31 (hot core; Mininni et al. 2023; López-Gallifa et al. 2024), and the comets 67P∕Churyumov-Gerasimenko and Hale-Bopp (Bockelée-Morvan et al. 2000; Le Roy et al. 2015; Altwegg et al. 2016). The colours are representative of the environment: orange and dark orange for low-mass cores and dark clouds, green and dark green for massive cores/IRDCs, blue and dark blue for more evolved hot cores and corinos, and pink and purple for comets.