Resolving dust and Lyα emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS
arXiv:2512.13778 · doi:10.1051/0004-6361/202558580
Abstract
Lyman emission is highly sensitive to dust and neutral hydrogen and is therefore expected to be strongly suppressed in dusty or gas-rich galaxies during the epoch of reionization (EoR). Nevertheless, numerous moderately dusty Ly emitters (LAEs) are observed at this epoch, suggesting that complex interstellar medium (ISM) geometries and feedback-driven outflows may facilitate Ly escape. We investigate the dust, gas, and stellar properties of the gravitationally lensed LAE HCM 6A at to characterize its multiphase ISM and the physical conditions regulating Ly escape. We combine JWST/NIRISS slitless spectroscopy, HST+JWST/NIRCam imaging, and JWST/NIRSpec slit spectra from the CANUCS program. Using a customized BAGPIPES SED-fitting framework with a flexible attenuation law, we derive stellar, nebular, and dust properties on integrated (kpc), slit-level (0.1 kpc), and pixel-level (25 pc) scales, enabled by strong lensing (-). A Ly map from SLEUTH traces the spatial distribution of Ly emission. We measure an unlensed stellar mass of - and an intrinsic UV magnitude of . The older region (S1) is moderately dusty with consistent stellar and nebular attenuation indicators, implying a uniform ISM geometry, while the youngest region (S3) shows strong discrepancies among dust tracers, indicating a feedback-shaped multiphase ISM. Ly emission arises primarily from S3, where a dust-cleared central clump enables efficient Ly escape. We find Calzetti-like attenuation curves with a UV bump that strengthens with stellar age and decreasing . Our observations provide a uniquely detailed, spatially resolved view of a moderately dusty LAE during the EoR, demonstrating how feedback and multiphase ISM structure govern Ly escape.
13 pages, 6 figures, Accepted for publication in A&A
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