Witnessing the onset of reionisation via Lyman-$\alpha$ emission at redshift 13
Joris Witstok, Peter Jakobsen, Roberto Maiolino, Jakob M. Helton,, Benjamin D. Johnson, Brant E. Robertson, Sandro Tacchella, Alex J. Cameron,, Renske Smit, Andrew J. Bunker, Aayush Saxena, Fengwu Sun, Stacey Alberts,, Santiago Arribas, William M. Baker, Rachana Bhatawdekar

TL;DR
This paper reports the first detection of Ly$ extalpha$ emission at redshift 13, indicating early galaxy activity and the onset of cosmic reionisation less than 330 million years after the Big Bang.
Contribution
It provides the first spectroscopic evidence of Ly$ extalpha$ emission at such a high redshift, revealing insights into early galaxy properties and reionisation processes.
Findings
Detection of Ly$ extalpha$ emission at z=13
Indication of early reionised regions around galaxies
Evidence of prolific ionising photon production
Abstract
Cosmic Reionisation commenced when ultraviolet (UV) radiation produced in the first galaxies began illuminating the cold, neutral gas that filled the primordial Universe. Recent James Webb Space Telescope (JWST) observations have shown that surprisingly UV-bright galaxies were in place beyond redshift , when the Universe was less than old. Smooth turnovers of their UV continua have been interpreted as damping-wing absorption of Lyman- (Ly), the principal hydrogen transition. However, spectral signatures encoding crucial properties of these sources, such as their emergent radiation field, largely remain elusive. Here we report spectroscopy from the JWST Advanced Deep Extragalactic Survey (JADES) of a galaxy at redshift that reveal a singular, bright emission line unambiguously identified as Ly, in…
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Taxonomy
TopicsScientific Research and Discoveries · Astronomy and Astrophysical Research · Calibration and Measurement Techniques
