A faint M$_{\rm UV} = -14.5$ Lyman-continuum leaker candidate in the epoch of reionization: Unprecedented Ly$\alpha$ properties at z=5.725
M. Messa, E. Vanzella, T. Morishita, M. Stiavelli, T. Treu, P. Bergamini, Z. Liu, A. Zanella, A. Bolamperti, A. Verhamme, T. Garel, C. Grillo, and P. Rosati

TL;DR
This paper reports on the unique Lyα emission properties of a highly metal-poor, low-mass galaxy at z=5.725, suggesting it is a strong candidate for leaking ionizing radiation during reionization.
Contribution
It presents the first detailed Lyα profile analysis of an extremely metal-poor dwarf galaxy at high redshift, indicating potential ionizing photon escape.
Findings
Lyα line is narrow, symmetric, and nearly at systemic velocity.
The galaxy's properties suggest a low neutral hydrogen column density.
AMORE6 is a compelling candidate for Lyman continuum leakage during reionization.
Abstract
We report the unprecedented Ly properties of AMORE6, an extremely metal-poor (), low-mass (), and ultracompact (effective radius pc) dwarf galaxy at , which is gravitationally lensed by the cluster A2744. A prominent, narrow, and nearly symmetric Ly emission line is detected at the systemic redshift (the latter traced by H, from JWST/NIRCam slitless spectroscopy), with a rest-frame equivalent width of \AA, a full width at half maximum of km s, and a slight asymmetry, resulting in a flux excess of in the red wing of the line. The negligible velocity offset from systemic ( km s, uncertainty), together with the sharpness and symmetry of the profile, indicates minimum radiative transfer effects, which implies a…
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