The VIMOS-VLT Deep Survey (VVDS) currently offers a unique combination of depth, angular size and number of measured galaxies among surveys of the distant Universe: ∼ 11, 000 spectra over 0.5 deg to IAB = 24 (VVDS-Deep), 35, 000 spectra over ∼ 7 deg 2 to IAB = 22.5 (VVDS-Wide). The current “First Epoch” data from VVDS-Deep already allow investigations of galaxy clustering and its dependence on ...