Fig. A.1.
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Point Spread Function subtraction and aperture masking of the Galactic star located between G1 (southwest) and G2 (east) in a MUSE narrow-band image centred on [O II] emission at z = 1.17. Light in this image may also arise from continuum emission. G2a and G2b refer to the brightest knots within G2. G2c denotes the region of G2 nearest to the stellar core (masked out) where [O II] emission can be detected.
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