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Elimination of Thermally Generated Charge in Charged Coupled Devices Using Bayesian Estimator

机译:使用贝叶斯估计器消除带电耦合器件中的热产生电荷

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摘要

This paper deals with advanced methods for elimination of thermally generated charge in astronomical images, which were acquired by a Charged Coupled Device (CCD) sensor. There exist a number of light images acquired by telescope, which were not corrected by dark frame. The reason is simple: the dark frame doesn’t exist, because it was not acquired. This situation may for instance come when sufficient memory space is not available. Correction methods based on the modeling of the light and dark image in the wavelet domain will be discussed. As the model for the dark frame image and for the light image the generalized Laplacian was chosen. The model parameters were estimated using moment method, whereas an extensive measurement on an astronomical camera was proposed and done. This measurement simplifies estimation of the dark frame model parameters. Finally a set of astronomical testing images was corrected and then the objective criteria for an image quality evaluation based on the aperture photometry were applied.
机译:本文讨论了消除天文学图像中热生成电荷的先进方法,这些方法是由电荷耦合器件(CCD)传感器获得的。望远镜存在大量的光图像,没有被暗框校正。原因很简单:暗框不存在,因为它没有被获取。例如,当没有足够的存储空间可用时,可能会出现这种情况。将讨论基于小波域中明暗图像建模的校正方法。作为暗框图像和亮图像的模型,选择了广义拉普拉斯算子。使用矩量法估算了模型参数,而提出并完成了在天文相机上的广泛测量。该测量简化了暗框模型参数的估计。最后,校正了一组天文测试图像,然后应用了基于孔径光度法的图像质量评估的客观标准。

著录项

  • 作者

    Svihlik J.; Pata P.;

  • 作者单位
  • 年度 2008
  • 总页数
  • 原文格式 PDF
  • 正文语种 en
  • 中图分类

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