ALMAGAL in the context of other interferometric surveys of star-forming regions in terms of number of target clumps vs. evolutionary stage (top), number of detected fragments (middle, from Coletta et al. 2025), and spatial resolution achieved (bottom). The panels show surveys for which the necessary information was immediately available in the papers and for which observations consist of single pointings or relatively small mosaics. For the latter reason, ALMA-IMF is not included in the figure as the program does relatively large maps of 15 star-forming complexes.