NIR-to-radio photometry available for our sample. Left panel: multi-band cutouts of our targets. The green text marks the instrument, the observed wavelength in units of μm, and the size of the field of view. Right panel: fits to the SEDs of our galaxies. We do not report the SED of ID1 because it lies in an area of UltraVista that is affected by unreliable flux uncertainties. ID2 is absent from the catalogue of Jin et al. (2018) due to the lack of K_s and VLA 3 GHz priors. The SEDs are fitted with a stellar component (blue curve; Bruzual & Charlot 2003) and an AGN torus component (red curve; Mullaney et al. 2011). The fits where fixed to the grism redshifts derived as in the main text. Upper limits are at 2σ.