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    • Comparing emission- and absorption-based gas-phase metallicities in GRB host galaxies at z = 2−4 using JWST 

      Schady, P; Yates, R M; Christensen, L; De Cia, A; Rossi, A; D’Elia, V; Heintz, K E; Jakobsson, P; Laskar, T; Levan, A; Salvaterra, R; Starling, R L C; Tanvir, N R; Thöne, C C; Vergani, S; Wiersema, K; Arabsalmani, M; Chen, H -W; De Pasquale, M; Fruchter, A; Fynbo, J P U; García-Benito, R; Gompertz, B; Hartmann, D; Kouveliotou, C; Milvang-Jensen, B; Palazzi, E; Perley, D.A.; Piranomonte, S; Pugliese, G; Savaglio, S; Sbarufatti, B; Schulze, S; Tagliaferri, G; Postigo, A de Ugarte; Watson, D; Wiseman, P (2024-04-15)
      Much of what is known of the chemical composition of the universe is based on emission line spectra from star-forming galaxies. Emission-based inferences are, nevertheless, model-dependent and they are dominated by light ...