Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation

We use the TNG-Cluster simulation to investigate how stellar mass and star formation rate (SFR) incompleteness affect the identification of density peaks within galaxy protoclusters at different redshifts. Our analysis focuses on a sample of 352 protoclusters, defined as the progenitor populations o...

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Detalhes bibliográficos

Principais autores:	Devontae C. Baxter, Alison L. Coil, Ethan O. Nadler, Dylan Nelson, Annalisa Pillepich, Ben Forrest, Finn Giddings, Emmet Golden-Marx, Brian C. Lemaux, Derek Sikorski
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
Colecção:	The Astrophysical Journal
Assuntos:	High-redshift galaxy clusters Galaxy formation Galaxy evolution Galaxy environments Large-scale structure of the universe Hydrodynamical simulations
Acesso em linha:	https://doi.org/10.3847/1538-4357/adf644
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