How to Coadd Images. II. Anti-aliasing and PSF Deconvolution

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Lei Wang, Huanyuan Shan, Lin Nie, Dezi Liu, Zhaojun Yan, Guoliang Li, Cheng Cheng, Yushan Xie, Han Qu, Wenwen Zheng, Xi Kang
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引用次数: 0

Abstract

We have developed a novel method for co-adding multiple under-sampled images that combines the iteratively reweighted least squares and divide-and-conquer algorithms. Our approach not only allows for the anti-aliasing of the images but also enables Point-Spread Function (PSF) deconvolution, resulting in enhanced restoration of extended sources, the highest peak signal-to-noise ratio, and reduced ringing artefacts. To test our method, we conducted numerical simulations that replicated observation runs of the China Space Station Telescope/ the VLT Survey Telescope (VST) and compared our results to those obtained using previous algorithms. The simulation showed that our method outperforms previous approaches in several ways, such as restoring the profile of extended sources and minimizing ringing artefacts. Additionally, because our method relies on the inherent advantages of least squares fitting, it is more versatile and does not depend on the local uniformity hypothesis for the PSF. However, the new method consumes much more computation than the other approaches.
如何添加图像。II.抗锯齿和 PSF 解卷积
我们开发了一种新方法,将迭代再加权最小二乘法和分而治之算法结合起来,共同添加多个欠采样图像。我们的方法不仅可以对图像进行抗锯齿处理,还能实现点扩散函数(PSF)解卷,从而增强对扩展源的还原,获得最高的峰值信噪比,并减少振铃伪影。为了测试我们的方法,我们进行了数值模拟,复制了中国空间站望远镜/VLT巡天望远镜(VST)的观测运行,并将我们的结果与使用以前算法得到的结果进行了比较。模拟结果表明,我们的方法在多个方面优于以前的方法,如恢复扩展源的轮廓和最小化振铃伪影。此外,由于我们的方法依赖于最小二乘法拟合的固有优势,因此通用性更强,而且不依赖于 PSF 的局部均匀性假设。不过,与其他方法相比,新方法的计算量要大得多。
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来源期刊
Research in Astronomy and Astrophysics
Research in Astronomy and Astrophysics 地学天文-天文与天体物理
CiteScore
3.20
自引率
16.70%
发文量
2599
审稿时长
6.0 months
期刊介绍: Research in Astronomy and Astrophysics (RAA) is an international journal publishing original research papers and reviews across all branches of astronomy and astrophysics, with a particular interest in the following topics: -large-scale structure of universe formation and evolution of galaxies- high-energy and cataclysmic processes in astrophysics- formation and evolution of stars- astrogeodynamics- solar magnetic activity and heliogeospace environments- dynamics of celestial bodies in the solar system and artificial bodies- space observation and exploration- new astronomical techniques and methods
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