The contribution of active galaxies to the far-infrared and submillimeter backgrounds

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We present a simple model, developed to estimate the contribution of Active Galactic Nuclei to the far--infrared background, closely linked to the AGN synthesis model for the X-ray background. According to our calculation the AGN contribution is never dominant, ranging from a few to 15 percent between 100 and 850 micron.
5 pages, 2 color figures, to appear in Proceedings of XXI Moriond Conference: "Galaxy Clusters and the High Redshift Universe Observed in X-rays", edited by D. Neumann, F.Durret, & J. Tran Thanh Van

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