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Gas surrounding high redshift galaxies has been studied through observationsof absorption line systems toward background quasars for decades. However, ithas proven difficult to identify and characterize the galaxies associated withthese absorbers due to the intrinsic faintness of the galaxies compared to thequasars at optical wavelengths. Utilizing the Atacama LargeMillimeter/Submillimeter Array, we report on detections of [CII] 158 micronline and dust continuum emission from two galaxies associated with two suchabsorbers at a redshift of z~4. Our results indicate that the hosts of thesehigh-metallicity absorbers have physical properties similar to massivestar-forming galaxies and are embedded in enriched neutral hydrogen gasreservoirs that extend well beyond the star-forming interstellar medium ofthese galaxies.

[CII] 158 micron Emission from the Host Galaxies of Damped Lyman Alpha Systems