The Mass and Redshift Dependence of Halo Star Clustering
We adopt the two-point correlation function (2PCF) as a statistical tool to quantify the spatial clustering of halo stars for galaxy systems spanning a wide range in host halo virial mass ( $11.25\lt {\mathrm{log}}_{10}{M}_{200c}/{M}_{\odot }\lt 15$ ) and redshifts (0 < z < 1.5) from the Illus...
| Prif Awduron: | , , , , , , , |
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| Fformat: | Erthygl |
| Iaith: | English |
| Cyhoeddwyd: |
IOP Publishing
2024-01-01
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| Cyfres: | The Astrophysical Journal |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/1538-4357/ad834a |