Notes. (1) VUDS ID; (2) stellar masses (in logM_⊙) and 1σ uncertainties from SED fitting, as described in Sect. 4.1; (3) star formation rates (in log(M_⊙/yr) from Hα or Hβ luminosity assuming Chabrier (2003) IMF and a theoretical ratio Hα/ Hβ = 2.82; uncertainties in SFR account for the propagation of errors in line fluxes and reddening; (4) effective radius (in kpc), derived applying GALFIT to F814W-band ACS-HST images as described in Sect. 4.4. A value of −9.9 is assigned for those cases in which: (a) GALFIT is not applied (VVDS-02h field) or (b) GALFIT returns an error at the end of the fitting procedure. (5) Ratio between the minor and major axis of the ellipse enclosing half of the total luminosity of the galaxy in the F814W filter; (6) and (7) gas surface density (μ_gas, in M_⊙ pc^-2) and gas fraction f_gas, respectively, which were derived from the SFR surface densities assuming a Kennicutt-Schmidt law with exponent 1.4, as described in Sect. 4.4. For μ_gas and f_gas, we should consider an uncertainty of at least 0.2−0.3 dex (~a factor of two), which comes both from the uncertainties of the size and also from the KS law (which has an average dispersion over different types of galaxies of ~0.2 dex). (8) Gas-phase metallicity derived from the code HII-CHI-mistry. The code also returns an error for the estimation; (9) ionization parameter and its uncertainty derived from HII-CHI-mistry; (10) morphological type as follows: 0 = round/nucleated, 1 = tadpole/cometary, 2 = clumpy/Chain, 3 = merger/interacting, 4 = low surface brightness, 5 = unresolved, 6 = not available (see Sect. 4.4 for more details). The entire version of this table for the whole sample is available at the CDS.