CORDIS Project
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The PantaRhei project aims to characterize the baryon cycle in galaxies during Cosmic Noon by analyzing gas outflows and their effects on star formation and chemical enrichment. It combines high-resolution spectroscopy with advanced modeling techniques to deepen the understanding of galaxy evolution.
The formation and evolution of galaxies over cosmic time is driven by the continuous flow of gas in and out of systems, known as the "baryon cycle." Current theoretical models suggest that feedback from star formation (SF) and active galactic nuclei (AGN) leads to gas outflows, regulating SF activity and enriching galaxy metal content.
This ejective feedback is believed to be particularly powerful at z=1-2, during the peak of SF and AGN activity, known as Cosmic Noon.
Yet, a comprehensive unders…
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