The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at <i>z</i> = 1.5–4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-unity Dust Covering Fractions
2026 · The Astrophysical Journal · 0 citations
https://doi.org/10.3847/1538-4357/ae38da