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Multi-wavelength studies at radio, infrared, optical, X-ray, and TeVwavelengths have discovered probable counterparts to many Galactic sources ofGeV emission detected by EGRET. These include pulsar wind nebulae, high massX-ray binaries, and mixed morphology supernova remnants. Here we provide anoverview of the observational properties of Galactic sources which emit across19 orders of magnitude in energy. We also present new observations of severalsources.

The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters