CORDIS Project
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The MUSE project develops a new instrument for observing distant galaxies by analyzing Lyman-alpha emissions. It aims to enhance understanding of the interstellar medium and the early universe's reionization through advanced radiation transfer modeling.
MUSE is a second generation instrument for the ESO-VLT being built in Lyon.
This integral field spectrograph is planned to start observing in autumn 2012.
One of the major goals of MUSE is to detect thousands of high redshift galaxies thanks to their Lyman-alpha emission. MCLya is a 3D Lyman-alpha radiation transfer code developed by the applicant.
It has been used to fit a small sample of observed Lyman-alpha lines from high redshift galaxies, constraining the gas and dust content and the star…
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
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