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Very high-energy (VHE; E > 100 GeV) gamma-rays have been detected from a widerange of astronomical objects, such as SNRs, pulsars and pulsar wind nebulae,AGN, gamma-ray binaries, molecular clouds, and possibly star-forming regions aswell. At lower energies, sources detected using Large Area Telescope (LAT)aboard Fermi provide a rich set of data which can be used to study the behaviorof cosmic accelerators in the GeV to TeV energy bands. In particular, theimproved angular resolution in both bands compared to previous instrumentssignificantly reduces source confusion and facilitates the identification ofassociated counterparts at lower energies. In this talk, a comprehensive searchfor VHE gamma-ray sources which are spatially coincident with GalacticFermi/LAT bright sources is performed, and the GeV to TeV spectra of selectedcoincident sources are shown. It is found that LAT bright GeV sources arecorrelated to TeV sources, in contrast with previous studies using EGRET data.

A search for VHE counterparts of galactic Fermi sources