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Table 2.

Different KiDS bright galaxy sub-samples considered in this work.

Selection log(L/L0) Ngal z log ( L / L 0 ) $ \log \left (\langle L\rangle /L_0\right ) $
Red (−∞,−0.55] 79584 0.16 −0.74
Red (−0.55,−0.33] 81220 0.21 −0.43
Red (−0.33,−0.16] 82043 0.26 −0.24
Red (−0.16,0.00] 82498 0.31 −0.08
Red (0.00,+∞) 85354 0.36 0.16

ns>2.5 (−∞,−0.55] 50464 0.15 −0.77
ns>2.5 (−0.55,−0.33] 52470 0.21 −0.43
ns>2.5 (−0.33,−0.16] 56212 0.26 −0.24
ns>2.5 (−0.16,0.00] 59040 0.31 0.08
ns>2.5 (0.00,+∞) 65429 0.36 0.16

Red, ns>4 145297 0.28 −0.09
Red, ns<4 203526 0.25 −0.24

Blue 385142 0.22 −0.45
ns<2.5 400786 0.22 −0.42

Density 675724 0.22 −0.42

Notes. Samples are split by colour, morphology, or both. We indicate the selection in luminosity (log(L/L0)), the number of galaxies in each bin (Ngal), the mean redshift of the sub-sample (〈z〉), and the logarithmic mean luminosity of the galaxies in the bin (log(〈L〉/L0)).

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