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Resolving the nature and putative nebular emission of GS9422: an obscured AGN without exotic stars

By Sandro Tacchella and others
Understanding the sources that power nebular emission in high-redshift galaxies is fundamentally important not only for shedding light onto the drivers of reionisation, but to constrain stellar populations and the growth of black holes. Here we focus on an individual object, GS9422, a galaxy at z_{\rm spec}=5.943 with exquisite data... Show more
April 2, 2024
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Resolving the nature and putative nebular emission of GS9422: an obscured AGN without exotic stars
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