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The detection by the HESS atmospheric Cerenkov telescope of fourteen newsources from the Galactic plane makes it possible to estimate the contributionof unresolved sources like those detected by HESS to the diffuse Galacticemission measured by the Milagro Collaboration. The number-intensity relationand the luminosity function for the HESS source population are investigated. Byevaluating the contribution of such a source population to the diffuse emissionwe conclude that a significant fraction of the TeV energy emission measured bythe Milagro experiment could be due to unresolved sources like HESS sources.Predictions concerning the number of sources which Veritas, Milagro, and HAWCshould detect are also given.

Constraints on the TeV source population and its contribution to the galactic diffuse TeV emission