Virgo cluster region mapped by VESTIGE. The complete blind survey covers the inner 104 deg² (green footprint), the same region mapped by NGVS (Ferrarese et al. 2012). The black contours indicate the X-ray emission of the diffuse gas of the cluster obtained by ROSAT (Böhringer et al. 1994), the large red dotted circles indicate the different substructures of the cluster, while the red, green, and blue empty circles indicate early-type galaxies, transition type galaxies, and star-forming systems, respectively, with sizes depending on their stellar mass (big for M_star > 10^9.5 M_⊙, medium for 10^8.5 <M_star ≤ 10^9.5 M_⊙, small for M_star ≤ 10^8.5 M_⊙) as defined in Boselli et al. (2014a).