de Cicco, D.D.de Cicco0000-0002-0501-8256Paolillo, M.M.Paolillo0000-0003-0911-8884Covone, G.G.Covone0000-0001-5008-8619Falocco, S.S.Falocco0000-0003-4210-7693Longo, G.G.Longo0000-0002-3938-692XGRADO, ANIELLOANIELLOGRADO0000-0003-0197-589XLimatola, L.L.Limatola0000-0002-3585-866XBOTTICELLA, MARIA TERESAMARIA TERESABOTTICELLAPignata, G.G.PignataCAPPELLARO, EnricoEnricoCAPPELLAROVaccari, M.M.VaccariTrevese, D.D.TreveseVagnetti, F.F.VagnettiSalvato, M.M.SalvatoRADOVICH, MARIOMARIORADOVICHBrandt, W. N.W. N.BrandtCapaccioli, M.M.CapaccioliNAPOLITANO, NICOLA ROSARIONICOLA ROSARIONAPOLITANOSCHIPANI, PietroPietroSCHIPANI2020-03-262020-03-262015http://hdl.handle.net/20.500.12386/23584The VLT Survey Telescope (VST) is located at Cerro Paranal Observatory; it is a joint venture between the European Southern Observatory (ESO) and the INAF-Osservatorio Astronomico di Capodimonte (OAC) in Napoli. The telescope is 2.65m in diameter and is equipped with the single focal plane detector OmegaCAM: a mosaic of 32 CCD detectors made up of 268 megapixels in total, corresponding to a 26cmx26cm area and a 1°x1° FoV, the resolution being 0.214"/pixel. The VST is dedicated to surveys in the wavelength range 0.3-1.0um. <P />The survey provides data in the g, r, and i bands, with an observing frequency of approximately ten days for the g and i bands and three days for the r band, depending on the various observational constraints. We discuss here the analysis of 28 epochs in the r band, for which we have the best temporal sampling. The observations cover the period from December 2011 to May 2012. <P />(1 data file).enDatabasehttp://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/574/A1122015yCat..35740112DFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation