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A multi-scale view of the Epoch of Reionisation (Kavli Science Focus Meeting)

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During the Epoch of Reionisation (EoR), the Universe went from being dark and neutral to mostly ionised at z~6. The sources responsible for ionising the intergalactic medium (IGM) are though to be mainly the first stars and galaxies, until now observationally elusive. With the arrival of JWST data, we have now unprecedented access to the early Universe, which can be used to improve our current models and understanding of this epoch.

This is a one-day meeting that will bring together experts studying the EoR from different perspectives and scales: from the young stars that produce copious amounts of ionising radiation, to the galaxies that contain them, and the surrounding IGM .

This talk is part of the Kavli Institute for Cosmology Seminars series.

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