X-ray and optical followup of gamma-ray (up to TeV) sources

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The imaging capabilities of the INTEGRAL and HESS observatories allow the study of hard X-ray and TeV sources with unprecedented positional accuracy. Here I review the multiwavelength followup studies which are currently being performed on the unidentified sources detected by these facilities in order to unveil their actual nature.
11 pages, 6 figures, ChJAA in press; proceedings of the Frascati Workshop 2007 "Multifrequency behaviour of high energy cosmic sources" (F. Giovannelli & L. Sabau-Graziati eds.). The quality of Fig. 1 was degraded to fit the arXiv uploads size limits

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