  The paper shows an analysis of the large-scale distribution of galaxy spin
directions of 739,286 galaxies imaged by DES. The distribution of the spin
directions of the galaxies exhibits a large-scale dipole axis. Comparison of
the location of the dipole axis to a similar analysis with data from SDSS,
Pan-STARRS, and DESI Legacy Survey shows that all sky surveys exhibit dipole
axes within 52$^o$ or less from each other, well within 1$\sigma$ error. While
non-random distribution is unexpected, the findings are consistent across all
sky surveys, regardless of the telescope or whether the data were annotated
manually or automatically. Possible errors that can lead to the observation are
discussed. The paper also discusses previous studies showing opposite
conclusions,and analyzes the decisions that led to these results. Although the
observation is provocative, and further research will be required, the existing
evidence justifies to consider the contention that galaxy spin directions as
observed from Earth are not necessarily randomly distributed. Possible
explanations can be related to mature cosmological theories, but also to the
internal structure of galaxies.

Cosmology and Nongalactic Astrophysics;Astrophysics of Galaxies