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- W2962778574 abstract "In preparation for deep extragalactic imaging with the James Webb Space Telescope, we explore the clustering of massive halos at z = 8 and 10 using a large N-body simulation. We find that halos with masses of 109–1011 h−1 M⊙, which are those expected to host galaxies detectable with JWST, are highly clustered with bias factors ranging from 5 to 30 depending strongly on mass, as well as on redshift and scale. This results in correlation lengths of 5–10 h−1 Mpc, similar to those of today's galaxies. Our results are based on a simulation of 130 billion particles in a box of size 250 h−1 Mpc using our new high-accuracy Abacus simulation code, the corrections to cosmological initial conditions of Garrison et al., and the Planck 2015 cosmology. We use variations between sub-volumes to estimate the detectability of the clustering. Because of the very strong interhalo clustering, we find that a medium-sized survey with a transverse size of the order of 25 h−1 comoving Mpc (about 13') may be able to detect the clustering of z = 8–10 galaxies with only 500–1000 survey objects if the galaxies indeed occupy the most massive dark matter halos." @default.
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- W2962778574 date "2019-04-24" @default.
- W2962778574 modified "2023-09-26" @default.
- W2962778574 title "Testing the Detection Significance on the Large-scale Structure by a <i>JWST</i> Deep Field Survey" @default.
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- W2962778574 doi "https://doi.org/10.3847/1538-4357/ab1268" @default.
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