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An efficient guide stars classification algorithm via support vector machines

机译:通过支持向量机的高效导星分类算法

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The purpose of this study is to obtain an approximate even guide stars catalog (GSC) applied in star trackers,thus a guide stars selection algorithm via support vector machines (SVM) is presented.Using combination of the number of stars and Boltzmann entropy within circular region centered at every star of original catalog(OC)as feature vector,the local density and uniformity of each star from OC is characterized preferably,which distinguishes guide stars and non-guide stars meeting structural risk minimization (SRM).The SVM algorithm is implemented by generating the GSC for a star tracker with an 8°×8°squared field of view (FOV).To validate the GSC generated by SVM,statistics of guide stars number inside the FOV is compared between SVM and magnitude filtering method(MFM) using 10,000 random boresight directions.Results clearly show the volume of GSC created by the SVM algorithm is approximately 34% and the standard deviation is 22% accounting for that of MFM satisfying four guide stars inside the FOV.Consequently, the proposed algorithm makes a great progress relative to MFM in capacity and uniformity of GSC.
机译:这项研究的目的是获得应用在恒星追踪器中的近似均匀的恒星目录(GSC),从而提出一种通过支持向量机(SVM)进行的恒星选择算法。以原始目录(OC)的每颗恒星为中心的区域作为特征向量,较好地表征了OC中每颗恒星的局部密度和均匀性,以区分满足结构风险最小化(SRM)的引导星和非引导星。为生成具有8°×8°平方视场(FOV)的恒星跟踪器的GSC实现。为验证SVM生成的GSC,比较了SVM和幅度滤波方法(MFM)将FOV内的导星数量统计),使用10,000个随机视轴方向。结果清楚地表明,由SVM算法创建的GSC的体积约为34%,标准偏差为22%(考虑了MFM)该算法满足了FOV内部的四颗导星。因此,相对于MFM,GSC的容量和均匀性都取得了很大的进步。

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