Discovery of a gas-enshrouded broad-line AGN at z ∼ 7

The Lyman-alpha (Ly$\alpha$) absorption profile in star-forming galaxies serves as a powerful tracer of the extended, dense neutral hydrogen in their surroundings during the Epoch of Reionization (EoR).
We report a unique galaxy, \galname, at $z\approx 6.87$ gravitationally lensed by the foreground galaxy cluster Abell 2744, which exhibits both moderate Ly$\alpha$ emission and damped Ly$\alpha$ absorption, suggesting the presence of a dense neutral hydrogen environment. Our analysis suggests that %the UV continuum is more likely shaped by a damped Ly$\alpha$ system rather than by nebular emission.
the UV continuum turnover near Ly$\alpha$ is more likely shaped by a damped Ly$\alpha$ system rather than nebular continuum from two photon process.
We analyze the physical properties of \galname with spectroscopic and photometric data from the James Webb Space Telescope (JWST) and the Hubble Space Telescope (HST). The galaxy shows a compact morphology ($r_e \sim 0.3\ {\rm kpc}$) and a broadened H$\alpha$ emission line, suggesting possible AGN activity. The broad component of H$\alpha$ has a FWHM of $2721 \pm 200\ {\rm km\ s^{-1}}$, corresponding to a black hole mass of $M_{\mathrm{BH}}=2.90^{+2.35}_{-1.28}\times 10^7 M_\odot$ and a black hole–to–stellar mass ratio of $\log (M_{\rm BH}/M_{\rm stellar}) = -1.58^{+0.45}_{-0.34}$. The Balmer decrement ($\rm H\alpha/H\beta$) yields a dust attenuation of $\rm A_V \approx 1.15 \pm 0.23$, indicating that this system is less dust-rich than some “little red dots”.
Furthermore, we perform SED fitting using both stellar and AGN models. The results show that the UV and optical wavelengths are dominated by star-forming regions, while the AGN component contributes primarily at longer wavelengths. This work provides new insights into the interplay between star formation, neutral gas, and potential AGN activity in galaxies during the EoR.