Lessons on early structure formation from a mature galaxy cluster observed at cosmic noon

作者: Boyuan Liu , Anna T P Schauer , Volker Bromm

DOI: 10.1093/MNRAS/STAA1307

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摘要: We demonstrate a new approach of indirectly constraining both early star and structure formation via mature galaxy clusters at cosmic noon (z~2), using the cluster XLSSC 122 as an example. With standard Press Schechter formalism, we infer rapid evolution efficiency (the ratio stellar to halo mass) from 10^-4 0.01 during z~20-13, based on age distribution stars in post-starburst galaxies 122, measured by HST photometry assuming no dust extinction. Here, consider all low-mass haloes, including minihaloes, that host first (5*10^5 Msun 13 122. Our exploratory results are consistent with existing constraints. More comprehensive will be obtained if our is extended large sample or field noon, improved modelling populations.

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