Large-scale asymmetry in the distribution of galaxy spin directions -- analysis and reproduction
Lior Shamir

TL;DR
This study critically examines previous claims of galaxy spin direction asymmetry, reproduces their analyses, and concludes that observed preferred directions are consistent with a cosmological-scale dipole axis, influenced by observational and internal galaxy factors.
Contribution
It provides a detailed reproduction and analysis of prior studies, clarifying the role of experimental design and internal galaxy structure in observed asymmetries.
Findings
Data supports a preferred galaxy spin direction from Earth.
Previous studies' results are influenced by experimental design choices.
Observed asymmetry may be due to internal galaxy structure, not large-scale anomalies.
Abstract
Recent independent observations using several different telescope systems an analysis methods have provided evidence of parity violation between the number of galaxies that spin in opposite directions. On the other hand, other studies argued that no parity violation can be identified. This paper provides detailed analysis, statistical inference, and reproduction of previous reports that show no preferred spin direction. Code and data used for the reproduction are publicly available. The results show that the data used in all of these studies agrees with the observation of a preferred direction as observed from Earth. In some of these studies the datasets were too small, or the statistical analysis was incomplete. In other papers the results were impacted by experimental design decisions that lead directly to show non-preferred direction. In some of these cases these decisions are not…
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