Belfiore,C.BelfioreBRESCIA, MassimoMassimoBRESCIACapaccioli,M.CapaccioliCaputi,O.CaputiCastiello, G.G.CastielloCORTECCHIA, FaustoFaustoCORTECCHIAFerragina, L.L.FerraginaFIERRO, DavideDavideFIERROFiume, V.V.FiumeMANCINI, DarioDarioMANCINIMancini, G.G.ManciniMarra, G.G.MarraMARTY, LaurentLaurentMARTYMazzola, G.G.MazzolaParisi, L.L.ParisiPellone, L.L.PellonePERROTTA, FrancescoFrancescoPERROTTAPorzio, V.V.PorzioSCHIPANI, PietroPietroSCHIPANISciarretta, G.G.SciarrettaSpirito, G.G.SpiritoValentino, M.M.Valentino2024-02-092024-02-092004981-238-688-2http://hdl.handle.net/20.500.12386/34739The VLT Survey Telescope (VST) is a 2.6 m aperture, wide-field (1°1°), UV to I facility, to be installed at the European Southern Observatory (ESO) on the Cerro Paranal Chile. VST was primarily intended to complement the observing capabilities of VLT with wide-angle imaging for detecting and pre-characterising sources for further observations with the VLT.STAMPAenConference paper10.1142/9789812702999_0036https://www.worldscientific.com/doi/abs/10.1142/9789812702999_0036https://arxiv.org/ftp/astro-ph/papers/0501/0501598.pdf2004otmu.conf..303BFIS/05 - ASTRONOMIA E ASTROFISICA