Baker_ObservationsOfTheInterstellarMediumOfGalaxies

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New radio, millimeter, and submillimeter facilities offer powerful capabilities for studying the "cold" (neutral atomic and molecular) phases of the interstellar medium in galaxies at low and high redshift. I will discuss the use of spectral line observations of these phases as tools for understanding how galaxies grow in mass, how their masses are internally distributed, and how they turn their gas reservoirs into stars.

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