A Hierarchical PSF Reconstruction Method
Pedro Alonso, Jun Zhang, Cong Liu

TL;DR
This paper introduces a multi-layer PSF reconstruction method that leverages data from multiple exposures to effectively remove complex PSF residuals, significantly reducing systematic errors in shear measurements in astronomy.
Contribution
The paper presents a novel multi-layer PSF reconstruction approach that utilizes all available exposures to improve PSF modeling accuracy and mitigate residual patterns affecting shear analysis.
Findings
Successfully eliminates most PSF residuals in Hyper Suprime-Cam data.
Reduces shear biases by removing systematic errors linked to PSF residuals.
Enhances the accuracy of shear measurements in weak lensing studies.
Abstract
Reconstruction of the point spread function (PSF) plays an important role in many areas of astronomy, including photometry, astrometry, galaxy morphology, and shear measurement. The atmospheric and instrumental effects are the two main contributors to the PSF, both of which may exhibit complex spatial features. Current PSF reconstruction schemes typically rely on individual exposures, and its ability of reproducing the complicated features of the PSF distribution is therefore limited by the number of stars. Interestingly, in conventional methods, after stacking the model residuals of the PSF ellipticities and (relative) sizes from a large number of exposures, one can often observe some stable and nontrivial spatial patterns on the entire focal plane, which could be quite detrimental to, e.g., weak lensing measurements. These PSF residual patterns are caused by instrumental effects as…
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Taxonomy
TopicsFatigue and fracture mechanics · Engineering Applied Research
