The Thermal State of the Intergalactic Medium at Redshift $5<z<6$
Jiren Liu, Lizhi Fang (UA)
TL;DR
This study investigates the thermal properties of the intergalactic medium during the epoch corresponding to redshifts 5 to 6, providing insights into the universe's thermal history during this period.
Contribution
It offers new measurements and analysis of the IGM's temperature at high redshifts, enhancing understanding of cosmic reionization.
Findings
IGM temperature increases with redshift
Evidence supports early reionization models
Constraints on heating mechanisms during reionization
Abstract
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Statistical and numerical algorithms