Testing Shear Recovery with Field Distortion
Jun Zhang, Fuyu Dong, Hekun Li, Xiangchong Li, Yingke Li, Dezi Liu,, Wentao Luo, Liping Fu, Guoliang Li, Zuhui Fan

TL;DR
This paper introduces a novel method to test and calibrate shear recovery accuracy in cosmic shear measurements using field distortion effects in real images, eliminating the need for simulations.
Contribution
The study demonstrates a new calibration technique leveraging field distortion to assess shear measurement biases directly from observational data.
Findings
Multiplicative biases are below 0.04 in specified shear ranges.
Minor additive biases (~5E-4) are identified in CFHTLenS data.
Fourier_Quad pipeline reduces biases compared to official catalogs.
Abstract
The tilt, rotation, or offset of each CCD with respect to the focal plane, as well as the distortion of the focal plane itself, cause shape distortions to the observed objects, an effect typically known as field distortion (FD). We point out that FD provides a unique way of quantifying the accuracy of cosmic shear measurement. The idea is to stack the shear estimators from galaxies that share similar FD-induced shape distortions. Given that the latter can be calculated with parameters from astrometric calibrations, the accuracy of the shear estimator can be directly tested on real images. It provides a way to calibrate the multiplicative and additive shear recovery biases within the scientific data itself, without requiring simulations or any external data sets. We use the CFHTLenS images to demonstrate the accuracy of the Fourier_Quad shear recovery method. We highlight some details in…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
