S. Falocco, D. De Cicco, M. Paolillo, G. Covone, G. Longo, A. Grado, L. Limatola, M. Vaccari, M. T. Botticella, G. Pignata, E. Cappellaro, D. Trevese, F. Vagnetti, M. Salvato, M. Radovich, L. Hsu, W. N. Brandt, M. Capaccioli, N. Napolitano, A. Baruffolo, E. Cascone, P. Schipani
Published 2015-07-17Version 1
This 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.
Comments: Refereed Proceeding of the "The Universe of Digital Sky Surveys" conference held at the INAF - Observatory of Capodimonte, Naples, on 25th-28th november 2014, to be published on Astrophysics and Space Science Proceedings, edited by Longo, Napolitano, Marconi, Paolillo, Iodice
SUDARE-VOICE variability-selection of Active Galaxies in the Chandra Deep Field South and the SERVS/SWIRE region
Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
A Large Population of Obscured AGN in Disguise as Low Luminosity AGN in Chandra Deep Field South
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