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About Maximilien Franco

My current research focuses on the evolution of the massive high redshift galaxies. I use IR and submm/mm wavelengths to probe the early Universe and understand the transition between star-forming and quenched galaxies.

Detection of fluorine in absorption in a star-forming galaxy at redshift 4.4

Fluorine is a fascinating element in many ways. We report the detection of fluorine (in the form of hydrogen fluoride) in a lensed galaxy at z=4.4, seen as it was 1.3 billion years after the Big Bang. This detection may give valuable clues to the highly debated formation conditions of this element.

Maximilien Franco

Nov 04, 2021

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maximilienfranco.fr
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m.franco@herts.ac.uk

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in/maximilien-franco-77590766

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Research Communities by Springer Nature