In the MUSE Extremely Deep Field, 32-51% of high-redshift Ly-alpha emitters show double-peaked line profiles, with the fraction depending on luminosity rather than decreasing steeply with redshift once selection effects are considered.
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The MUSE Extremely Deep Field: Classifying the Spectral Shapes of Lya Emitting Galaxies
In the MUSE Extremely Deep Field, 32-51% of high-redshift Ly-alpha emitters show double-peaked line profiles, with the fraction depending on luminosity rather than decreasing steeply with redshift once selection effects are considered.