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机构地区:[1]中国科学院国家天文台,北京100012 [2]山东大学威海分校机电与信息工程学院,山东威海264209 [3]中国科学院研究生院,北京100049
出 处:《光谱学与光谱分析》2012年第2期510-513,共4页Spectroscopy and Spectral Analysis
基 金:国家自然科学基金项目(10973021;11078013)资助
摘 要:提出一种适用于在郭守敬望远镜海量光谱中自动、快速筛选激变变星的方法。利用已证认的激变变星光谱作为模板,通过随机森林分类训练,得到一个分类模型,该模型给出了各个波长对应流量的重要性排序,可根据该排序进行降维并用于激变变星判别,结果作为反馈进一步丰富模板库。实验中共发现了16个新的激变变星候选体,表明了该方法的可行性。An automatic and efficient method for cataclysmic variables candidates is presented in the present paper.The identified CVs were selected as templates.A model was constructed by random forest algorithm with templates and random selected spectra.Wavelength ranking was described by the model and the classifier was constructed afterwards.Most of the non-candidates were excluded by the method.Template matching strategy was used to identify the final candidates which were analyzed to complement the templates as feedback.16 new CVs candidates were found in the experiment that shows that our approach to finding special celestial bodies can be feasible in LAMOST.
分 类 号:TP29[自动化与计算机技术—检测技术与自动化装置]
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