Fig. D.1.
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Same as Fig. 9, for the BLA at z = 0.06805. The VLT/VIMOS FoV spans a square of ∼1.6 Mpc side at this redshift. The VLT/MUSE FoV is smaller, reaching impact parameters of ∼60 kpc from the QSO sightline. One galaxy in our VLT/VIMOS survey lies within 1000 km s−1 from the BLA. The right panel shows a zoom-out of the left panel, using spectroscopic data from the SDSS DR16 survey.
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