Fig. 1.
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Multi-wavelength data for the galaxy VC875, shown at their native resolutions. From left to right: The first row presents HST/ACS F814W (rest-frame 145 nm), JWST/NIRCam F115W (207 nm), F150W (270 nm), and F277W (499 nm). The second row shows JWST/F444W (800 nm), ALMA dust continuum emission around 157 μm, and ALMA [CII] 158 μm emission. The contours are those of the ALMA [CII] line emission maps starting from 3σ increasing by steps of 2σ. Ellipses in the bottom left corners represent the central lobe of the PSF for HST and JWST images, and the synthesised beam for ALMA images.
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