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Optimal image subtraction method: Summary derivations, applications, and publicly shared application using IDL

机译:最佳图像减法:使用IDL的摘要派生,应用程序和公共共享的应用程序

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To detect objects that vary in brightness or spatial coordinates over time, C. Alard and R. H. Lupton in 1998 proposed an "optimal image subtraction" (OIS) method that constructs a convolution kernel from a set of matching stars distributed across the two images to be subtracted. Using multivariable least squares, the kernel is derived and can be designed to vary by pixel coordinates across the convolved image. Local effects in the optics, including aberrations or other spatially sensitive perturbations to a perfect image, can be mitigated. This paper presents the specific systems of equations that originate from the OIS method. Also included is a complete description of the Gaussian components basis vectors used by Alard & Lupton to construct the convolution kernel. An alternative set of basis vectors, called the delta function basis, is also described. Important issues are addressed, including the selection of the matching stars, differential background correction, constant photometric flux, contaminated pixel masking, and alignment at the subpixel level. Computer algorithms for the OIS method were developed, written using the Interactive Data Language (IDL), and applications demonstrating these algorithms are presented.
机译:为了检测随时间变化的亮度或空间坐标的对象,C。Alard和RH Lupton在1998年提出了一种“最佳图像减法”(OIS)方法,该方法根据分布在两幅图像上的一组匹配星来构造卷积核。减去。使用多变量最小二乘法,可以导出内核,并且可以将其设计为根据卷积图像上的像素坐标而变化。可以减轻光学器件中的局部影响,包括像差或对理想图像的其他空间敏感扰动。本文介绍了源自OIS方法的特定方程组。还包括对Alard&Lupton用于构造卷积核的高斯分量基向量的完整描述。还描述了另一组基础矢量,称为增量函数基础。解决了重要问题,包括选择匹配的星星,差分背景校正,恒定的光度通量,受污染的像素蒙版以及子像素级别的对齐。开发了用于OIS方法的计算机算法,使用交互式数据语言(IDL)编写,并演示了演示这些算法的应用程序。

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