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This paper represents a step toward constraining galaxy formation models viaTeV gamm a ray observations. We use semi-analytic models of galaxy formation topredict a spectral distribution for the intergalactic infrared photon field,which in turn yields information about the absorption of TeV gamma rays fromextra-galactic sources. By making predictions for integral flux observations at>200 GeV for several known EGRE T sources, we directly compare our models withcurrent observational upper limits obtained by Whipple. In addition, ourpredictions may offer a guide to the observing programs for the currentpopulation of TeV gamma ray observatories.Comment: 6 pages, 11 figures, to appear in the proceedings of the 6th TeV  Workshop at Snowbird, U

The implications of galaxy formation models for the TeV observations of current detectors