{ "id": "2001.02560", "version": "v1", "published": "2020-01-08T15:13:42.000Z", "updated": "2020-01-08T15:13:42.000Z", "title": "Extending the variability selection of active galactic nuclei in the W-CDF-S and SERVS/SWIRE region", "authors": [ "M. Poulain", "M. Paolillo", "D. De Cicco", "W. N. Brandt", "F. E. Bauer", "S. Falocco", "F. Vagnetti", "A. Grado", "F. Ragosta", "M. T. Botticella", "E. Cappellaro", "G. Pignata", "M. Vaccari", "P. Schipani", "G. Covone", "G. Longo", "N. R. Napolitano" ], "categories": [ "astro-ph.GA" ], "abstract": "Variability has proven to be a powerful tool to detect active galactic nuclei (AGN) in multi-epoch surveys. The new-generation facilities expected to become operational in the next few years will mark a new era in time-domain astronomy and their wide-field multi-epoch campaigns will favor extensive variability studies. We present our analysis of AGN variability in the second half of the VST survey of the Wide Chandra Deep Field South (W-CDF-S), performed in the r band and covering a 2 sq. deg. area. The analysis complements a previous work, in which the first half of the area was investigated. We provide a reliable catalog of variable AGN candidates, which will be critical targets in future variability studies. We selected a sample of optically variable sources and made use of infrared data from the Spitzer mission to validate their nature by means of color-based diagnostics. We obtain a sample of 782 AGN candidates among which 12 are classified as supernovae, 54 as stars, and 232 as AGN. We estimate a contamination $\\lesssim 20\\%$ and a completeness $\\sim 38\\%$ with respect to mid-infrared selected samples.", "revisions": [ { "version": "v1", "updated": "2020-01-08T15:13:42.000Z" } ], "analyses": { "keywords": [ "servs/swire region", "variability selection", "wide chandra deep field south", "variability studies", "agn candidates" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }