Overview of the surroundings of the ALMA-IMF protocluster clouds, ordered by decreasing mass of their central clump (Col. (9) of Table 1): W51-E and W51-IRS2 (panel a), W43-MM1, W43-MM2, and W43-MM3 (panel b), G333.60 (panel c), G338.93 (panel d), G010.62 (panel e), and G008.67 (panel f). ATLASGAL 870 μm emission contours (logarithmically spaced from 0.45 Jy beam⁻¹ to 140 Jy beam⁻¹ with a 19.2″ beam) are overlaid on Spitzer three-color images (red represents MIPS 24 μm, green GLIMPSE 8 μm, and blue GLIMPSE 3.6 μm). The green and red contours outline the primary beam response of the ALMA 12 m array mosaics down to 15% at 3 mm and 1.3 mm, respectively. A 3 pc scale bar is shown in the lower-right corner of each image.