Hanwen Sun, Tao Wang, E. Daddi, Qiaoyang Hao, Ke Xu, D. Elbaz, Luwenjia Zhou, H. J. Mo, Huiyuan Wang, Longyue Chen, Yangyao Chen, Shuowen Jin, Yipeng Lyu, Nikolaj B. Sillassen, Kai Wang, Tiancheng Yang
Abstract Protoclusters, galaxy clusters’ high-redshift progenitors, hold the key to understanding the formation and evolution of clusters and their member galaxies. However, their cosmological distances and spatial extensions (tens of Mpc) have inhibited complete mapping of their structure and constituent galaxies, which is key to robustly linking protoclusters to their descendants. Here we report the discovery of the Bigfoot, a tridimensional structure at z = 3.98 including 11 subgroups traced by 55 (700) spectroscopic (photometric) redshifts with JWST, extending over 15 × 37 × 49 cMpc 3 in the PRIMER-UDS field. Bigfoot’s large-scale and mass function of member galaxies closely match constrained simulations’ predictions for the progenitors of today’s most massive clusters ( M 0 > 10 15 M ⊙ ). All subgroups with M h > 10 12.5 M ⊙ exhibit enhanced fractions of massive galaxies (>10 10.0 M ⊙ ) compared to lower-mass halos and fields, demonstrating the accelerated formation of massive galaxies in massive halos. The presence of this massive protocluster with a large central halo (10 13.0 M ⊙ ) in a JWST deep field bears important cosmological implication that favors high σ 8 of PLANCK cosmology over low-redshift probes.