  The Visible InfraRed (VIR) mapping spectrometer onboard Dawn mission has
obtained the spatial distribution of the spectral reflectance of Vesta in the
wavelength ranges between 0.25-1.07 micrometers and 0.95-5.1 micrometers. A
photometric correction allows to characterize the intrinsic variability of the
surface albedo by removing the dependance of the reflectance from the observing
geometry. In this work, we present the photometric correction obtained for
observations from the Survey, HAMO and HAMO 2 mission phases at Vesta in the
whole spectral range investigated by VIR, as well as the surface albedo maps.
