Aims. We have devised a model for estimating the ultraviolet (UV) and optical line emission (i.e. CIII] 1909 Å, Hβ, [OIII] 5007 Å, Hα, and [NII] 6583 Å) that traces HII regions in the interstellar medium (ISM) of a subset of galaxies at z ∼ 4-6 from the ALMA large programme ALPINE. The aim is to investigate the combined impact of binary stars...
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December 24, 2024 (v1)Journal articleUploaded on: January 13, 2025
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September 11, 2024 (v1)Journal article
Context. The ultraviolet continuum traces young stars while the near-infrared unveils older stellar populations and dust-obscured regions. Balmer emission lines provide insights into gas properties and young stellar objects but are highly affected by dust attenuation. The near-infrared Paschen lines suffer less dust attenuation and can be used...
Uploaded on: October 15, 2024