The Optical Extragalactic Background Light from Resolved Galaxies

Abstract

We discuss the ultraviolet to near-IR galaxy counts from the deepest imaging surveys, including the northern and southern Hubble Deep Fields. The logarithmic slope of the galaxy number-magnitude relation is flatter than 0.4 in all seven UBVIJHK optical bandpasses at faint magnitudes, i.e. the light from resolved galaxies has converged from the UV to the near-IR. Most of the galaxy contribution to the extragalactic background light (EBL) comes from relatively bright, low-redshift objects (50% at V_AB<21 and 90% at V_AB<25.5). We find a lower limit to the surface brightness of the optical EBL of about 15 nW/m^2/sterad, comparable to the intensity of the far-IR background from COBE data. Diffuse light, lost because of surface brightness selection effects, may add substantially to the EBL.

15 pages, 15 figures. Invited talk at IAU Symposium 204, "The Extragalactic Infrared Background and its Cosmological Implications", Manchester, August 2000, eds. M.Harwit and M.G.Hauser

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