The topology of reionization and the environments where galaxies efficiently produce ionizing photons are key open questions. For the first time, we investigate the trend between ionizing photon production efficiency, $\xi_{ \rm ion}$, and galaxy overdensity, $\log(1+\delta)$. We analyze the ionizing properties of 79 galaxies between $1.0 < z < 5.2$ using JWST NIRSpec medium-resolution spectra from the Systematic Mid-infrared Instrument (MIRI) Legacy Extragalactic Survey (SMILES) program. Among these, 67 galaxies have H$\alpha$ coverage, spanning $1.0 < z < 3.1$. The galaxy overdensity, $\log(1+\delta)$, is measured using the JADES photometric catalog, which covers the SMILES footprint. For the subset with H$\alpha$ coverage, we find that $\log\xi_{ \rm ion}$ is positively correlated with $\log(1+\delta)$, with a slope of $0.94_{ -0.46}^{ +0.46}$. Additionally, the mean $\xi_{ \rm ion}$ for galaxies in overdense regions ($\log(1+\delta) > 0.1$) is 2.43 times that of galaxies in lower density regions ($\log(1+\delta) < 0.1$). This strong trend is found to be independent of redshift evolution. Furthermore, our results confirm the robust correlations between $\xi_{ \rm ion}$ and the rest-frame equivalent widths of the [O III] or H$\alpha$ emission lines. Our results suggest that galaxies in high-density regions are efficient producers of ionizing photons.
Categories: astro-ph.GA astro-ph.CO