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Introducing hidden Markov models to LAMOST automatic data processing

机译:将隐藏的马尔可夫模型引入Lamost自动数据处理

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The LAMOST1,2 telescope is expected to have its first light in later of 2007. The 4-meter aperture and 4000-fiber feeding ablility will make it a powerful spectra sky survey instrument, as well a challenge to the mission of data processing and analysis. So far several statistical methods, mainly based on PCA, have been developed for spectra automatic classification and red shift measurement by a team of LAMOST3. Statistical methods of Hidden Markov Modelling have become popular in many area since 1990s, which are rich in mathematical structure and can form the theoretical basis for use in a wide range of applications, e.g. speech recognition and pattern recognition. No doubt they are prospective implements for automatic spectra processing and analysis. In this paper, I attempt to briefly introduce the theoretical aspects of this type of statistical modelling and show the possible applications in automatic spectra data processing and analysis.
机译:Lamost1,2望远镜预计将在2007年后的第一盏灯。4米的孔径和4000纤维饲料的可能性将使它成为一个强大的光谱天空调查仪器,也是对数据处理和分析的使命的挑战。到目前为止,几种统计方法主要基于PCA,已经开发了一个Lamost3团队的Spectra自动分类和红移测量。自20世纪90年代以来,隐马尔可夫建模的统计方法在许多地区变得流行,这富有数学结构,可以形成在各种应用中使用的理论基础,例如,语音识别和模式识别。毫无疑问,他们是自动光谱处理和分析的前瞻性工具。在本文中,我试图简要介绍这种类型的统计建模的理论方面,并在自动光谱数据处理和分析中显示可能的应用。

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