Measuring the [C II]-to-H I connection in high-redshift absorption-selected galaxies
HI neutral gas is the basic building block of galaxies. It dictates the star formation rate and hence the metal enrichment rates within high redshift galaxies. HI neutral gas cannot be directly observed beyond z ≈ 0.38 due to the weakness of the 21 cm transition, therefore alternate methods need to be developed for studying high redshift galaxies. The emission luminosity of [C II]-157.741 μm trans