Weak lensing goes bananas: What flexion really measures
Peter Schneider (AIfA Bonn), Xinzhong Er (AIfA & MPIfR)

TL;DR
This paper investigates the measurement of flexion in weak gravitational lensing, deriving the relevant equations, analyzing biases, and exploring the decomposition of flexion into components, revealing fundamental limitations of the formalism.
Contribution
It derives the reduced flexion lens equation, quantifies biases in estimators, and decomposes flexion into shear-related and non-shear components, highlighting formalism limitations.
Findings
Flexion measures higher-order image distortions in weak lensing.
Biases in shear and flexion estimators depend on source size and flexion.
Multiple images form when reduced flexion times source size exceeds a threshold.
Abstract
In weak gravitational lensing, the image distortion caused by shear measures the projected tidal gravitational field of the deflecting mass distribution. To lowest order, the shear is proportional to the mean image ellipticity. If the image sizes are not small compared to the scale over which the shear varies, higher-order distortions occur, called flexion. For ordinary weak lensing, the observable quantity is not the shear, but the reduced shear, owing to the mass-sheet degeneracy. Likewise, the flexion itself is unobservable. Rather, higher-order image distortions measure the reduced flexion, i.e., derivatives of the reduced shear. We derive the corresponding lens equation in terms of the reduced flexion and calculate the resulting relation between brightness moments of source and image. Assuming an isotropic distribution of source orientations, estimates for the reduced shear and…
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