VANDELS is an ESO Public Spectroscopic Survey designed to build a sample
of high-signal-to-noise ratio, medium-resolution spectra of galaxies at
redshifts between 1 and 6.5. Here we present the final Public Data
Release of the VANDELS Survey, comprising 2087 redshift measurements. We
provide a detailed description of sample selection, observations, and
data reduction procedures. The final catalogue reaches a target
selection completeness of 40% at iAB = 25. The high
signal-to-noise ratio of the spectra (above 7 in 80% of the spectra) and
the dispersion of 2.5 Å allowed us to measure redshifts with high
precision, the redshift measurement success rate reaching almost 100%.
Together with the redshift catalogue and the reduced spectra, we also
provide optical mid-infrared photometry and physical parameters derived
through fitting the spectral energy distribution. The observed galaxy
sample comprises both passive and star forming galaxies covering a
stellar mass range of 8.3 < Log(M*/M⊙) < 11.7.