Fig. B.1.
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Rest-frame UV luminosity function for the sample of UBR color-selected LBGs. Upper panel: cumulative luminosity function of the LBGs identified within the FoV of MUSE (squares) and FORS2 (triangles), and of those galaxies with spectroscopic redshift within |Δv| ≤ 1000 km s−1 around the central QSO (points). The LBGs’ luminosity functions are corrected for the 1D completeness of the R-band that is used for the detection (see Figure 1). Lower panel: overdensity as a function of the R-band magnitude.
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