English

The Point Spread Function Reconstruction by Using Moffatlets - I

Instrumentation and Methods for Astrophysics 2016-09-28 v1 Astrophysics of Galaxies

Abstract

The shear measurement is a crucial task in the current and the future weak lensing survey projects. And the reconstruction of the point spread function(PSF) is one of the essential steps. In this work, we present three different methods, including Gaussianlets, Moffatlets and EMPCA to quantify their efficiency on PSF reconstruction using four sets of simulated LSST star images. Gaussianlets and Moffatlets are two different sets of basis functions whose profiles are based on Gaussian and Moffat functions respectively. Expectation Maximization(EM) PCA is a statistical method performing iterative procedure to find principal components of an ensemble of star images. Our tests show that: 1) Moffatlets always perform better than Gaussianlets. 2) EMPCA is more compact and flexible, but the noise existing in the Principal Components (PCs) will contaminate the size and ellipticity of PSF while Moffatlets keeps them very well.

Keywords

Cite

@article{arxiv.1604.07126,
  title  = {The Point Spread Function Reconstruction by Using Moffatlets - I},
  author = {Baishun Li and Guoliang Li and Jun Cheng and John Peterson and Wei Cui},
  journal= {arXiv preprint arXiv:1604.07126},
  year   = {2016}
}

Comments

19 pages,17 figures,Accepted for publication in RAA

R2 v1 2026-06-22T13:39:47.140Z