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Spin Parity of Spiral Galaxies. VI. A Search for Dynamical Memory in the Spin Distribution of Galaxies in HSC WIDE Survey Regions

  • Authors: Masanori Iye, Masafumi Yagi

Masanori Iye and Masafumi Yagi 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 4.

(Upper panel) Observed cumulative distribution function OCDF for Cube Set S1. In this case, the observed OCDF extends beyond the range covered by 1000 Monte Carlo simulations. The discontinuity at pS = 0.5 in the theoretical distribution is less pronounced due to the large number of galaxies nall ≥ 300 in the cubes selected for this set. (Lower panel) OCDFs for Cube Set S127 (see Table 4). The observed distribution (red), the theoretical binomial expectation (black), and the results from 1000 Monte Carlo simulations (cyan) are shown. The observed OCDF lies well within the range spanned by the Monte Carlo simulations.

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