CORDIS Project
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This project investigates how the first luminous sources influenced the reionization of the intergalactic medium, utilizing advanced spectroscopy of quasars. It aims to understand the growth of supermassive black holes and the enrichment of baryonic structures in the early universe.
How the first luminous sources reionized diffuse baryons in the intergalactic medium (IGM) is one of the most fundamental open questions in cosmology.
The latest CMB constraints suggest reionization occurred at z ~ 7-8, within the realm of the highest redshift quasars known.
The overarching impetus of this proposal is that Euclid's imminent discovery of scores of bright quasar beacons in a neutral universe, combined with the exquisite sensitivity of JWST, will enable a set of qualitatively new…
UNIVERSITEIT LEIDEN
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