Galaxy clusters trace the largest structures of the Universe and provide ideal laboratories for studying galaxy evolution and cosmology1,2. Clusters with extended X-ray emission have been discovered at redshifts of up to z ≈ 2.5 (refs 3,4,5,6,7). Meanwhile, there has been growing interest in hunting for protoclusters, the progenitors of clusters, at higher redshifts8,9,10,11,12,13,14. It is, however, very challenging to find the largest protoclusters at early times, when they start to assemble. Here, we report a giant protocluster of galaxies at z ≈ 5.7, when the Universe was only one billion years old. This protocluster occupies a volume of about 353 cubic comoving megaparsecs. It is embedded in an even larger overdense region with at least 41 spectroscopically confirmed, luminous Lyα-emitting galaxies (Lyα emitters, or LAEs), including several previously reported LAEs9. Its LAE density is 6.6 times the average density at z ≈ 5.7. It is the only one of its kind in an LAE survey in 4 deg2 on the sky. Such a large structure is also rarely seen in current cosmological simulations. This protocluster will collapse into a galaxy cluster with a mass of (3.6 ± 0.9) × 1015 solar masses, comparable to those of the most massive clusters or protoclusters known so far.
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We acknowledge support from the National Key R&D Program of China (2016YFA0400703 and 2016YFA0400702) and from the National Science Foundation of China (grant 11533001). G.A.B. is supported by CONICYT/FONDECYT, Programa de Iniciacion, Folio 11150220. E.W.O. acknowledges support from the NSF from grant AST1313006. We thank R. de Grijs and M. Ouchi for discussions. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. Australian access to the Magellan Telescopes was supported through the National Collaborative Research Infrastructure Strategy of the Australian Federal Government.
The authors declare no competing interests.
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Jiang, L., Wu, J., Bian, F. et al. A giant protocluster of galaxies at redshift 5.7. Nat Astron 2, 962–966 (2018). https://doi.org/10.1038/s41550-018-0587-9