VIMOS slit-position and MUSE multiwavelength images of the field of CDF-S XT2. Left panel: JWST-F444W imaging superimposed with the VLT-VIMOS slits (black box) used by Balestra et al. (2010) for determining the redshift of XT2 and the nearby AGN CANDELS #4210. Left-center panel: MUSE collapsed imaging at [OII] emission line (i.e., λ_cen = 6478 Å, width 10 Å) of the field of XT2, where according to Balestra et al. (2010) the line [OII] of XT2’s is detected by VLT-VIMOS. The AGN CANDELS #4210 is clearly detected (consistent with a [OII] line at z = 0.7396). Right-center panel: MUSE white-light image showing the position of the XT2 host and AGN CANDELS #4210. The cyan and red dots depict the position of the XT2 host and AGN CANDELS #4210, respectively. Right panel: MUSE collapsed imaging at the Ly-α emission line (i.e., λ_cen = 1216 Å, width 10 Å) of the field of XT2 at redshift z_spec = 3.4598. At these wavelengths, the XT2 host is not observed. The cyan and red dots depict the position of the XT2 host and AGN CANDELS #4210, respectively.