A long time ago in an LAE far, far away: a signpost of early reionization or a nascent AGN at $z=13$?

The JADES survey recently reported the discovery of JADES-GS-z13-1-LA at $z = 13$, the highest redshift Ly$α$ emitter (LAE) ever observed. This observation suggests that either the intergalactic medium (IGM) surrounding JADES-GS-z13-1-LA is highly ionized, or the galaxy's intrinsic Ly$α$ emission properties are extreme. We use radiative transfer simulations of reionization that capture the distribution of ionized gas in the $z = 13$ IGM to investigate the implications of JADES-GS-z13-1-LA for reionization. We find that if JADES-GS-z13-1-LA is a typical star forming galaxy (SFG) with properties characteristic of LAEs at z ~ 6, its detection suggests that the universe is 5% ionized by $z = 13$. We also investigate the possibility that the extreme properties of JADES-GS-z13-1-LA are driven by an AGN. Using a simple analysis based on the fact that AGN are expected to produce more ionizing photons than SFGs, we estimate that the likelihood that JADES-GS-z13-1-LA hosts an AGN is $88%$, $66%$, and $33%$ if the IGM is $< 1%$, ≈ 5% and ≈ 25% ionized, respectively. We also highlight other features in the spectrum of JADES-GS-z13-1-LA that may be indicative of AGN activity, including strong Ly$α$ damping wing absorption extending to ~ 1300 angstroms, and a possible CII*λ1335 emission line. Our findings strongly motivate dedicated follow-up observations of JADES-GS-z13-1-LA to determine whether it hosts an AGN.