The <scp>thesan</scp> project: environmental drivers of Local Group reionization

Abstract The timing of cosmic reionization across Local Group (LG) analogues provides insights into their early histories and surrounding large-scale structure. Using the radiation-hydrodynamic simulation thesan-1 and its dark matter-only counterpart thesan-dark-1, we track the reionization histories of all haloes, including 224 LG analogues within the proximity of any of the 20 Virgo-like clusters with halo masses above 1014 M⊙ at z = 0 and their environments. The statistically controlled samples quantify how the reionization redshift (zreion) correlates with halo mass, local overdensity, and present-day pair properties. Even at fixed mass, haloes in denser regions ionize earlier, and increasing the overdensity smoothing scale systematically suppresses small-scale structure, including local variations and environmental gradients in zreion. Virgo-like clusters accelerate reionization in their surroundings out to ~5–10 cMpc, beyond which local overdensity again becomes the dominant factor. Within LG pairs, reionization timing offsets reach up to ~150 Myr and correlate with present-day halo separation, reflecting sensitivity to large-scale structure rather than mass ratio in driving asynchronous reionization. The results support an extreme inside-out picture where clustered sources rapidly ionize their immediate neighborhoods, while lower-density regions self-ionize later and voids wait for external homogenization. These links between environment and reionization timing explain the influence of protoclusters and help interpret fossil records in LG dwarfs around the Milky Way. For Milky Way analogues, we find a reionization redshift as early (late) as $z_{\rm reion} = 12.7^{+2.0}_{-1.7}$ ($8.88^{+0.66}_{-0.70}$) when considered on 125 ckpc (500 ckpc) scales, with LG analogues following an inside-out reionization picture.