Planes of satellite galaxies: when exceptions are the rule
Marius Cautun (1), Sownak Bose (1), Carlos S. Frenk (1), Qi Guo (2),, Jiaxin Han (1), Wojciech A. Hellwing (1,3), Till Sawala (1), Wenting Wang, (1), ((1) ICC Durham (2) NAO Beijing (3) ICM Warsaw)

TL;DR
This study shows that planar satellite galaxy structures are common in $ ext{Λ}$CDM simulations, and the observed MW and M31 planes are not as exceptional as previously thought, emphasizing the importance of statistical context.
Contribution
It demonstrates that satellite planes are prevalent in simulations and that the apparent discrepancy with observations is due to misinterpretation and statistical effects.
Findings
Approximately 10% of $ ext{Λ}$CDM haloes have prominent satellite planes.
Satellite planes exhibit large diversity in properties.
Correcting for the look-elsewhere effect reduces the perceived significance of observed planes.
Abstract
The detection of planar structures within the satellite systems of both the Milky Way (MW) and Andromeda (M31) has been reported as being in stark contradiction to the predictions of the standard cosmological model (CDM). Given the ambiguity in defining a planar configuration, it is unclear how to interpret the low incidence of the MW and M31 planes in CDM. We investigate the prevalence of satellite planes around galactic mass haloes identified in high resolution cosmological simulations. We find that planar structures are very common, and that ~10% of CDM haloes have even more prominent planes than those present in the Local Group. While ubiquitous, the planes of satellite galaxies show a large diversity in their properties. This precludes using one or two systems as small scale probes of cosmology, since a large sample of satellite systems is needed to…
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