Elliptical Weighted HOLICs for Weak Lensing Shear Measurement. part1:Definitions and isotropic PSF correction
Yuki Okura, Toshifumi Futamase

TL;DR
This paper introduces the E-HOLICs method, using elliptical weight functions and a zero plane concept to improve gravitational shear measurement accuracy in weak lensing, especially under complex PSF conditions.
Contribution
The paper presents a novel shear estimation method with elliptical weights and a zero plane concept, enhancing accuracy and systematic error reduction over traditional approaches.
Findings
E-HOLICs accurately estimates shear for highly elliptical images.
The method reduces systematic errors compared to KSB in simulations.
Shear estimation simplifies to solving a polynomial in distortion magnitude.
Abstract
We develop a new method to estimate gravitational shear by adopting an elliptical weight function to measure background galaxy images. In doing so, we introduce a new concept of "zero plane" which is an imaginal source plane where shapes of all sources are perfect circles, and regard the intrinsic shear as the result of an imaginal lensing distortion. This makes the relation between the observed shear, the intrinsic shear and lensing distortion more simple and thus higher-order calculation more easy. The elliptical weight function allows us to measure the mutiplemoment of shape of background galaxies more precisely by weighting highly to brighter parts of image and moreover to reduce systematic error due to insufficient expansion of the weight function in the original approach of KSB. Point Spread Function(PSF) correction in E-HOLICs methods becomes more complicated than those in KSB…
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.
