Postage stamps (7″ × 7″) of some ALMA-selected galaxies. From left to right: JWST/NIRCam F322W2 (3.2 μm), F150W2 (1.5 μm), and the MUSE white-light image. For sources that are located outside the MUSE FoV, we report instead the VLT/FORS2 R-band image. The superimposed black contours show the CO(4–3) line emission or, in the case of C08, the 1.2 mm dust continuum (bottom panels). Contours correspond to [ − 2, 2, 3, 2^N]×σ with N, the integer number, >1.