Example of an ALMAGAL target observed from mid-infrared to millimeter. The ALMAGAL ID (AG323.7408-0.2633), its physical parameters (Molinari et al. 2025), and the number of cores detected in ALMAGAL continuum observations (Coletta et al. 2025) are reported in the top-left corner of the figure. Panels a–h: source images (~80″ × 45″) at wavelengths increasing from 24 μm to 1.38 mm. The wavelength in micrometers is reported in the top-right corner of each panel. Panel a: Spitzer-MIPS image of the source (saturated in the center). Panels b and c: Herschel-PACS images. Panels d–f: Herschel-SPIRE images. Panel g: the ATLASGAL image. Panel h: new ALMAGAL image. In this image, 15 fragments were detected by Coletta et al. (2025). Angular resolutions in the different panels are as follows: a: 6″; b: 10.2″ (for this panel and the following four, the resolution value is not the nominal one for Herschel, but rather the one directly measured by Traficante et al. 2011, on Hi-GAL maps, and circularized here); c: 13.5″; d: 23″; e: 30″; f: 42″; g: 19″; and h: 0.5″. Being detected at 70 μm (and also at 24 μm, in this case), this source is classified as star-forming in accordance with the Hi-GAL catalog criteria.