Characterizing the Average Interstellar Medium Conditions of Galaxies at $z\sim$ 5.6-9 with UV and Optical Nebular Lines

Weida Hu, Casey Papovich, Mark Dickinson +30

Ultraviolet (UV; rest-frame $\sim 1200-2000$ A) spectra provide a wealth of diagnostics to characterize fundamental galaxy properties, such as their chemical enrichment, the nature…