Discovery, identification, and study of variability in gamma-ray point sources

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dc.creatorFiorucci, M.
dc.creatorMarchili, N.
dc.creatorTosti, G.
dc.creatorCiprini, S.
dc.creatorMarcucci, F.
dc.creatorTramacere, A.
dc.date2003-04-10
dc.date.accessioned2026-07-07T02:08:13Z
dc.date.available2026-07-07T02:08:13Z
dc.descriptionWe present preliminary results of a statistical analysis obtained with a sample of blazars observed at the Perugia Astronomical Observatory since 1992. We briefly show how these statistical results can be useful to discriminate faint variable sources against the background noise. This technique, together with the more traditional ones, may be used to discover and identify high-energy point sources.
dc.description4 pages. Poster at the International Workshop "High Energy Blazar Astronomy" celebrating the 50th anniversary of Tuorla Observatory (Tuorla Observatory, Turku, Finland, 17-21 June 2002). Proceedings to be published in the PASP Conference Series, Eds. A. Sillanpaa, L. O. Takalo, and E. Valtaoja
dc.identifierhttps://arxiv.org/abs/astro-ph/0304186
dc.identifierhttp://arxiv.org/abs/astro-ph/0304186
dc.identifierASP Conf.Ser. 299 (2003) 217
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5959
dc.subjectAstrophysics
dc.titleDiscovery, identification, and study of variability in gamma-ray point sources
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