MUSE spectroscopy of GRB 220627A. Left: white light image resulting from the final MUSE data cube. The GRB afterglow is clearly visible at the centre of the image. Right: telluric-corrected spectrum (black) and error spectrum (grey) of GRB 220627A extracted from the MUSE data cube using an aperture with a radius of 0.6″. We show identified absorption lines at the GRB redshift (z = 3.084) and the intervening system (z = 2.665) in grey and red, respectively. The vertical shaded region is heavily affected by telluric lines.