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UV Diagnostics of Galaxies from the Peak of Star-Formation to the Epoch of Reionization

Published onMay 31, 2019
UV Diagnostics of Galaxies from the Peak of Star-Formation to the Epoch of Reionization
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Abstract

We describe prospects facilitated by giant telescopes in the 2020s to use rest-frame UV spectroscopy to study the properties of massive stellar populations and gas (ionization, metallicity, kinematics, outflows) in and around galaxies from the peak of the cosmic star-formation density (z~3) up in to the epoch of reionization (z > 6).

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