Multi-wavelength data handling in current and future surveys: the possible role of Virtual Observatory

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dc.creatorVignali, C.
dc.creatorFiore, F.
dc.creatorComastri, A.
dc.creatorBrusa, M.
dc.creatorGilli, R.
dc.creatorCappelluti, N.
dc.creatorCivano, F.
dc.creatorZamorani, G.
dc.date2009-02-05
dc.date.accessioned2026-07-07T12:38:51Z
dc.date.available2026-07-07T12:38:51Z
dc.descriptionHere we review some of the main issues related to multi-wavelength source identification and characterization, with particular emphasis on the field of X-ray surveys carried out over the last years. This complex and time-consuming process is going to represent one of the main difficulties over the coming years, when significantly larger surveys, both in area and depth, will be carried out with the new generations of space- and ground-based facilities like e.g. eROSITA, WISE, VISTA, Pan-STARRS, and LSST. The Virtual Observatory can offer a reliable way to approach to a new concept of data handling and multi-wavelength source characterization, provided that uniform and rigorous data analyses and extensive quality checks are performed.
dc.description6 pages, to be published in the Proceedings of the Workshop "Multiwavelength Astronomy and Virtual Observatory", held at ESAC-Madrid, December 1-3, 2008
dc.identifierhttps://arxiv.org/abs/0902.0976
dc.identifierhttp://arxiv.org/abs/0902.0976
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218909
dc.subjectCosmology and Nongalactic Astrophysics
dc.subjectHigh Energy Astrophysical Phenomena
dc.titleMulti-wavelength data handling in current and future surveys: the possible role of Virtual Observatory
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