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Unveiling the Interstellar Medium in High-Redshift Galaxies

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If you have a question about this talk, please contact Sandro Tacchella.

We have identified approximately 180 galaxies at redshifts z=4-10 through the analysis of optical emission lines in the JWST /NIRSpec data obtained from the three major public spectroscopic programs of ERO , GLASS, and CEERS . Leveraging this extensive high-redshift spectroscopic sample, my talk will discuss the evolution of interstellar medium (ISM) properties, with a specific focus on the chemical enrichment.

This talk is part of the Galaxies Discussion Group series.

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