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Symmetry in Hyper Suprime-Cam Galaxy Spin Directions

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. Our code is available at ✎.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/2515-5172/ad8fb1

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Institution:
University of Oxford
Division:
HUMS
Department:
Asian and Middle Eastern Studies
Sub department:
Astrophysics
Role:
Author
ORCID:
0000-0002-0986-314X
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Role:
Author
ORCID:
0000-0003-0685-9791


Publisher:
American Astronomical Society
Journal:
Research Notes of the American Astronomical Society More from this journal
Volume:
8
Issue:
11
Article number:
281
Publication date:
2024-11-11
Acceptance date:
2024-11-06
DOI:
EISSN:
2515-5172


Language:
English
Keywords:
Source identifiers:
2411929
Deposit date:
2024-11-11
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