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A new 6-cm survey of almost 0.6 square degrees to a limit of 0.55-mJy/beam(10-sigma) finds 37 isolated radio sources and 7 radio source pairs (notnecessarily physical companions). IRAC counterparts are identified for at least92% of the radio sources within the area of deep IRAC coverage, which includes31 isolated sources and 6 pairs. This contrasts with an identification rate of<74% to R<23.95 in visible light. Eight of the IRAC galaxies have power lawspectral energy distributions, implying that the mid-infrared emission comesfrom a powerful AGN. The remaining 26 IRAC galaxies show stellar emission inthe mid-infrared, probably in most of these galaxies because the stellaremission is bright enough to outshine an underlying AGN. The infrared colorssuggest that the majority of these galaxies are bulge-dominated and haveredshifts between approximately 0.5 and 1.0. Visible spectra from the DEEP2redshift survey, available for 11 galaxies, are consistent with thissuggestion. The IRAC galaxies fall into two distinct groups in acolor-magnitude diagram, one group (the "stripe") includes all the AGN. Theother group (the "blue clump") has blue 3.6 to 8 micron colors and a smallrange of 8 micron magnitudes. This separation should be useful in classifyinggalaxies found in other radio surveys.Comment: Accepted by A

Mid-Infrared Identification of 6 cm Radio-Source Counterparts in the Extended Groth Strip