Falocco, S.S.FaloccoDe Cicco, D.D.De CiccoPaolillo, MaurizioMaurizioPaolilloCovone, G.G.CovoneLongo, G.G.LongoGRADO, ANIELLOANIELLOGRADOLimatola, L.L.LimatolaVaccari, M.M.VaccariBOTTICELLA, MARIA TERESAMARIA TERESABOTTICELLAPignata, G.G.PignataCAPPELLARO, EnricoEnricoCAPPELLAROTrevese, D.D.TreveseVagnetti, F.F.VagnettiSalvato, M.M.SalvatoRADOVICH, MARIOMARIORADOVICHHsu, L.L.HsuBrandt, W. N.W. N.BrandtCapaccioli, M.M.CapaccioliNAPOLITANO, NICOLA ROSARIONICOLA ROSARIONAPOLITANOBARUFFOLO, AndreaAndreaBARUFFOLOCASCONE, EnricoEnricoCASCONESCHIPANI, PietroPietroSCHIPANI2020-07-142020-07-142016978-3-319-19329-81570-6591http://hdl.handle.net/20.500.12386/26436This work makes use of the VST observations to select variable sources. We use also the IR photometry, SED fitting and X-ray information where available to confirm the nature of the AGN candidates. The IR data, available over the full survey area, allow to confirm the consistency of the variability selection with the IR color selection method, while the detection of variability may prove useful to detect the presence of an AGN in IR selected starburst galaxies.STAMPAenConference paper10.1007/978-3-319-19330-4_432-s2.0-84978946318000389802600044https://link.springer.com/chapter/10.1007%2F978-3-319-19330-4_432016ASSP...42..275FFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation