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We describe the completed VIMOS VLT Deep Survey, and the final data releaseof 35016 galaxies and type-I AGN with measured spectroscopic redshifts up toredshift z~6.7, in areas 0.142 to 8.7 square degrees, and volumes from 0.5x10^6to 2x10^7h^-3Mpc^3. We have selected samples of galaxies based solely on theiri-band magnitude reaching i_{AB}=24.75. Spectra have been obtained with VIMOSon the ESO-VLT, integrating 0.75h, 4.5h and 18h for the Wide, Deep, andUltra-Deep nested surveys. A total of 1263 galaxies have been re-observedindependently within the VVDS, and from the VIPERS and MASSIV surveys. They areused to establish the redshift measurements reliability, to assesscompleteness, and to provide a weighting scheme taking into account the surveyselection function. We describe the main properties of the VVDS samples, andthe VVDS is compared to other spectroscopic surveys. In total we have obtainedspectroscopic redshifts for 34594 galaxies, 422 type-I AGN, and 12430 Galacticstars. The survey has enabled to identify galaxies up to very high redshiftswith 4669 redshifts in 1<=z_{spec}<=2, 561 in 2<=z_{spec}<=3 and 468 withz_{spec}>3, and specific populations like LAE have been identified out toz=6.62. We show that the VVDS occupies a unique place in the parameter spacedefined by area, depth, redshift coverage, and number of spectra. The VVDSprovides a comprehensive survey of the distant universe, covering all epochssince z, or more than 12 Gyr of cosmic time, with a uniform selection, thelargest such sample to date. A wealth of science results derived from the VVDShave shed new light on the evolution of galaxies and AGN, and theirdistribution in space, over this large cosmic time. A final public release ofthe complete VVDS spectroscopic redshift sample is available athttp://cesam.lam.fr/vvds.

The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z~6.7 selected with 17.5<=i_{AB}<=24.7