Abstract
We perform a Bayesian analysis of anisotropy in binary galaxy spin directions in the Hyper-Suprime Cam Data Release 3 catalog, in response to a recent claim that it exhibits a dipole. We find no significant evidence for anisotropy, or for a direction-independent spin probability that differs from 0.5. These results are unchanged allowing for a quadrupole or simply searching for a fixed anisotropy between any two hemispheres, and the Bayes factor indicates decisive evidence for the isotropic model. Our principled method contrasts with the statistic employed by Shamir, which lacks a strong theoretical foundation.
| Original language | English |
|---|---|
| Article number | 281 |
| Number of pages | 3 |
| Journal | Research Notes of the AAS |
| Volume | 8 |
| Issue number | 11 |
| DOIs | |
| Publication status | Published - 1 Nov 2024 |
Keywords
- Galaxies
- Large-scale structure of the universe
- Bayesian statistics
- Astrostatistics
- UKRI
- STFC
- ST/X508664/1
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