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• W4385436314 abstract "Motivated by spectroscopic confirmation of three overdense regions in the COSMOS field at $zsim3.35$, we analyze the uniquely deep multi-wavelength photometry and extensive spectroscopy available in the field to identify any further related structure. We construct a three dimensional density map using the Voronoi tesselation Monte Carlo method and find additional regions of significant overdensity. Here we present and examine a set of six overdense structures at $3.20<z<3.45$ in the COSMOS field, the most well characterized of which, PCl~J0959+0235, has 80 spectroscopically confirmed members and an estimated mass of $1.35times 10^{15}$~M$_odot$, and is modeled to virialize at $zsim1.5-2.0$. These structures contain ten overdense peaks with $>5sigma$ overdensity separated by up to 70 cMpc, suggestive of a proto-supercluster similar to the Hyperion system at $zsim2.45$. Upcoming photometric surveys with JWST such as COSMOS-Web, and further spectroscopic follow-up will enable more extensive analysis of the evolutionary effects that such an environment may have on its component galaxies at these early times." @default.
• W4385436314 created "2023-08-01" @default.
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• W4385436314 date "2023-07-27" @default.
• W4385436314 modified "2023-10-16" @default.
• W4385436314 title "Elent'ari: A $zsim3.3$ Proto-Supercluster in COSMOS" @default.
• W4385436314 doi "https://doi.org/10.48550/arxiv.2307.15113" @default.
• W4385436314 hasPublicationYear "2023" @default.
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