Anatomy of an ionized bubble: NIRCam grism spectroscopy of the $z=6.6$ double-peaked Lyman-$\hat{I}\pm$ emitter COLA1 and its environment

Abstract

The increasingly neutral intergalactic gas at $z>6$ impacts the Lyman-$\hat{I}\pm$ flux observed from galaxies. One luminous galaxy, COLA1, stands out because of its unique double-peaked Ly$\hat{I}\pm$ line at $z=6.6$, unseen in any simulation of reionization. Here we present JWST/NIRCam wide-field slitless spectroscopy in a 21 arcmin${}^2$ field centered on COLA1. We find 141 galaxies spectroscopically-selected through the [OIII]($\lambda 4969,5008$) doublet at $5.35<z<6.95$, with 40 of these sources showing H${\hat{I}}^2$. For COLA1 we additionally detect [OIII]${}_{4363}$ and H${\hat{I}}^3$. We measure a systemic redshift of $z=6.5917$ for COLA1, confirming the double-peak nature of the Ly$\hat{I}\pm$ profile. This implies that it resides in a highly ionized bubble and that it is leaking ionizing photons with a high escape fraction $f_{\mathrm{esc}}(\mathrm{LyC})=20$-$50$%, making it a prime laboratory to study Lyman continuum escape in the Epoch of Reionization. COLA1 shows all the signs of a prolific ionizer with a Ly$\hat{I}\pm$ escape fraction of $81\pm 5\%$, Balmer decrement indicating no dust, a steep UV slope (${\hat{I}}_{\mathrm{UV}}^2=-3.2\pm 0.4$), and a star-formation surface density $\gtrsim 10\times$ that of typical galaxies at similar redshift. We detect 5 galaxies in COLA1's close environment ($\hat{I}”z<0.02$). Exploiting the high spectroscopic completeness inherent to grism surveys, and using mock simulations that mimic the selection function, we show the that number of detected companions is very typical for a similarly UV-bright ($M_{\mathrm{UV}}\sim -21.3$) galaxy; that is, the ionized bubble around COLA1 is unlikely due to an excessively large over-density. Instead, the measured ionizing properties suggest that COLA1 by itself might be powering the bubble required to explain its double-peaked Ly$\hat{I}\pm$ profile ($R_{\mathrm{ion}}\approx 0.7$ pMpc), with minor contribution from detected neighbours ($-17.5>M_{\mathrm{UV}}>-19.5$).

15 pages, 13 figures. Accepted for publication in A&A. Main figs. 1, 2, 10 (SFR surface density), 11 (spectra and positions of galaxies in the bubble). Corrected error in escape fraction estimate from SFR surface density