  VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of
high signal to noise, medium resolution spectra of galaxies at redshift between
1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey,
comprising 2087 redshift measurements. We give 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{\AA} 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-IR photometry
and physical parameters derived through SED fitting. The observed galaxy sample
comprises both passive and star forming galaxies covering a stellar mass range
8.3< Log(M*/Msolar)<11.7. All catalogues and spectra are accessible through the
survey database (http://vandels.inaf.it) where all information can be queried
interactively, and via the ESO Archive (https://www.eso.org/qi/).
