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Tracking Halo Orbits and Their Mass Evolution around Large-scale Filaments

  • Authors: Hannah Jhee, Hyunmi Song, Rory Smith, Jihye Shin, Inkyu Park, Clotilde Laigle

Hannah Jhee et al 2022 The Astrophysical Journal 940 .

  • Provider: AAS Journals

Caption: Figure 6.

Phase-space distributions at z = 0 of halos subsampled by time since first crossing: [0, 1), [1, 2.5), [2.5, 6), and [6, 13.5) Gyr from left to right. The number of halos in each panel is 498, 491, 470, and 219, respectively. The color map is according to the mean time since first crossing (〈t FC〉) of halos in a given hexagonal bin.

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