Fig. 2
The VVDS rest-frame FUV-band luminosity functions from z ≃ 0.1 up to z ≃ 4 (from the thinnest to the thickest curve), fitted with a Schechter functional form parametrised with the Schechter parameters (α, φ∗, M∗) reported in Table 1. Lines are dashed for magnitudes fainter than the LF magnitude bias in each redshift bin (see Sect. 3.1).
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