Probing patchy reionisation with JWST: IGM opacity constraints from the Lyman-$\hat{I}\pm$ forest of galaxies in legacy extragalactic fields

Abstract

We present the first characterization of the Gunn-Peterson trough in high-redshift galaxies using public JWST NIRSpec spectroscopy. This enables us to derive the first galaxy-based IGM opacity measurements at the end of reionisation. Using galaxy spectra has several advantages over quasar spectra: it enables measurements of the IGM opacity in any extragalactic field over a continuous redshift range $4\lesssim z\lesssim 7$, as well as measurements of the intrinsic Lyman-${\hat{I}}^2$ opacity. Our novel constraints are in good agreement with state-of-the-art ground-based quasar Lyman-$\hat{I}\pm$ forest observations, and will become competitive as the number of JWST $z>5$ galaxy spectra rapidly increases. We also provide the first constraints on the uncontaminated Lyman-${\hat{I}}^2$ opacity at $5<z<6$. Finally, we demonstrate the power of JWST to connect the ionisation state of the IGM to the sources of reionisation in a single extragalactic field. We show that a previously reported galaxy overdensity and an excess of Lyman-$\hat{I}\pm$ emitters detected with JWST in GOODS-South at $z=5.8-5.9$ coincides with an anomalously low IGM opacity to Lyman-$\hat{I}\pm$ at this redshift. The local photo-ionisation rate excess can be fully accounted for by the cumulative ionising output of $M_{\mathrm{UV}}\lesssim -10$ galaxies in the overdensity, provided they have ${\log }_{10}⟨\hat{I}{¾}_{\mathrm{ion}}{f}_{\mathrm{esc}}/[{\mathrm{erg}}^{-1}\mathrm{Hz}]⟩\simeq 25$ (e.g. ${\log }_{10}\hat{I}{¾}_{\mathrm{ion}}/[{\mathrm{erg}}^{-1}\mathrm{Hz}]=25.4$ and $f_{\mathrm{esc}}=40\%$). Overall, this breakthrough offers a new way to connect the galaxy large-scale structure to the state of the IGM, potentially enabling us to precisely identify the sources of reionisation.

10 pages + appendices. Accepted in MNRAS. Updated to match accepted version