Fig. 1

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Lensing geometry and notation near the north pole. The sky curvature is suppressed for clarity. The deflection vector lies in the plane tangent to the observed coordinate
at latitude θ and longitude φ, and points toward the unlensed coordinate
, lying a distance
away along the great circle generated by α. The lensing remapping for parallel-transported spin-weighted fields like the dashed green vector or ellipse receives a phase correction eis(β−β′) from the rotation of the local θ and φ basis axes.
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