Fig. 1.
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Distribution of the continuum S/N for the MUSE spectra of the 84 galaxies included in the down-the-barrel subsample (left panel) and of the 360 galaxies used for the transverse analysis, divided into bins of impact parameter: b ≤ 40 kpc (P1), 40 kpc < b ≤ 65 kpc (P2), 65 kpc < b ≤ 90 kpc (P3), and 90 kpc < b ≤ 110 kpc (P4; right panel).
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