Notes. ⁽¹⁾Protocluster name, central position used for the ALMA-IMF observations. Distances and masses are from Motte et al. (2022) and references therein. ⁽²⁾Velocity relative to the local standard of rest extracted from Cunningham et al. (2023). ⁽³⁾Classification of the ALMA-IMF protocluster clouds: Young (Y), Intermediate (I), and Evolved (E) (see Section 4.1 by Motte et al. (2022)). ⁽⁴⁾Central frequencies of observations in Band 6 extracted from Louvet et al. (2024). ⁽⁵⁾Angular resolution in Band 6 extracted from Louvet et al. (2024). ⁽⁶⁾Angular resolution in spw1 Band 6 (217.150 GHz, which includes the SiO (5–4) and DCN (3–2) lines) defined as ${\theta }_{ave}=\sqrt{{\theta }_{maj}\times {\theta }_{min}}$ and extracted from Cunningham et al. (2023). ⁽⁷⁾Angular resolution in spw5 Band 6 (230.530 GHz, which includes the CO(2–1) line) extracted from Cunningham et al. (2023).