Correlated orientations of the axes of large quasar groups on Gpc scales
Tracey Friday, Roger G. Clowes, Gerard M. Williger

TL;DR
This study finds large-scale correlated orientations of quasar groups, suggesting intrinsic alignments that challenge current cosmological models and potentially explain quasar polarisation and radio jet alignments.
Contribution
It provides the first evidence of correlated orientations among large quasar groups on Gpc scales, revealing alignments larger than those predicted by standard cosmology.
Findings
LQG position angles are non-uniformly distributed.
LQGs show bimodal orientation distribution near quasar polarisation angles.
Significant alignment observed at ~30° separation, over 1.6 Gpc scales.
Abstract
Correlated orientations of quasar optical and radio polarisation, and of radio jets, have been reported on Gpc scales, possibly arising from intrinsic alignment of spin axes. Optical quasar polarisation appears to be preferentially either aligned or orthogonal to the host large-scale structure, specifically large quasar groups (LQGs). Using a sample of 71 LQGs at redshifts , we investigate whether LQGs themselves exhibit correlated orientation. We find that LQG position angles (PAs) are unlikely to be drawn from a uniform distribution (-values ). The LQG PA distribution is bimodal, with median modes at , remarkably close to the mean angles of quasar radio polarisation reported in two regions coincident with our LQG sample. We quantify the degree of alignment in the PA data, and find…
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