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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 5.

The solid curve shows the theoretical two-sided binomial cumulative distribution function TCDF(p) for a cube set with R = 100 in Array 7. The probability of obtaining an asymmetry equal to or larger than that observed for this set is given by pfrac = TCDF(p). The dashed line represents the corresponding TCDF for the normal distribution. In the binomial case, the curve deviates from the normal distribution due to its discrete and finite nature.

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