Study of Star/Galaxy Classification Based on the XGBoost Algorithm     

《Chinese Astronomy and Astrophysics》2019,43(4):539-548

Machine learning has achieved great success in many areas today. The lifting algorithm has a strong ability to adapt to various scenarios with a high accuracy, and has played a great role in many fields. But in astronomy, the application of lifting algorithms is still rare. In response to the low classification accuracy of the dark star/galaxy source set in the Sloan Digital Sky Survey (SDSS), a new research result of machine learning, eXtreme Gradient Boosting (XGBoost), has been introduced. The complete photometric data set is obtained from the SDSS-DR7, and divided into a bright source set and a dark source set according to the star magnitude. Firstly, the ten-fold cross-validation method is used for the bright source set and the dark source set respectively, and the XGBoost algorithm is used to establish the star/galaxy classification model. Then, the grid search and other methods are used to adjust the XGBoost parameters. Finally, based on the galaxy classification accuracy and other indicators, the classification results are analyzed, by comparing with the models of function tree (FT), Adaptive boosting (Adaboost), Random Forest (RF), Gradient Boosting Decision Tree (GBDT), Stacked Denoising AutoEncoders (SDAE), and Deep Belief Nets (DBN). The experimental results show that, the XGBoost improves the classification accuracy of galaxies in the dark source classification by nearly 10% as compared to the function tree algorithm, and improves the classification accuracy of sources with the darkest magnitudes in the dark source set by nearly 5% as compared to the function tree algorithm. Compared with other traditional machine learning algorithms and deep neural networks, the XGBoost also has different degrees of improvement.  相似文献   

Relation of Velocity Distribution and Mass for DA White Dwarfstwo     

Xiao-bo Gong  Li-fang Li 《Chinese Astronomy and Astrophysics》2018,42(2):202-212

White dwarfs are the evolutionary endpoint of the low-and-medium mass stars. In the studies of white dwarfs, the mass of white dwarf is an important physical parameter. In this paper, we give an analysis about the velocity distribution of DA white dwarfs in the Sloan Digital Sky Survey (SDSS), and hope to find the relation between mass and velocity distribution of white dwarfs. We get the radial velocity and tangential velocity of every DA white dwarf according to their proper motion and spectral shift. Through analyzing the velocity distribution of DA white dwarfs, we find that the small-mass white dwarfs, which are produced from the single-star evolution channel, have a relatively large velocity dispersion.  相似文献   

Integration of Penman approach with complementary principle for evaporation research          下载免费PDF全文

Songjun Han  Fuqiang Tian 《水文研究》2018,32(19):3051-3058

Natural evaporation occurs with water transportation from an unsaturated land surface into an unsaturated atmosphere. The subprocesses at the land surface and in the atmosphere are one‐sidedly emphasized in the Penman approach and the complementary principle, in which the ratio of actual evaporation to the Penman potential evaporation is expressed as a function of the wetness state of the land surface and the atmosphere, respectively. The Penman approach and complementary principle can be integrated for completely conceptualizing the evaporation process, by expressing the evaporation ratio as a function of both the land surface and atmospheric wetness. The integrated approach has the potential to increase the accuracy of evaporation estimation while reducing the burdens of parameterization.  相似文献   

一种海洋混合层深度的智能识别方法研究     

张康  郭双喜  黄鹏起  屈玲  鲁远征  岑显荣  于璐莎  周伟东  周生启 《热带海洋学报》2019,38(5):32-41

文章提出了一种识别混合层深度的人工智能方法。该方法在温度(密度)与压强(或深度)间建立线性模型, 并且将其系数和方差做成一组表征廓线特征的统计量。初始时为模型设定一个主观的先验分布, 在一个自海表向下移动的窗口内通过贝叶斯链式法则和最小描述长度原理学习新数据, 得到系数均值的最大后验概率估计。用F-检验识别系数发生突变的位置, 以此确定混合层的存在性及其深度。通过2017年2月太平洋海域的地转海洋学实时观测阵(Array for Real-time Geostrophic Oceanography, ARGO)数据进行测试, 并且以质量因子(Quality Index, QI)值作为判断识别混合层深度结果准确性的依据, 发现该方法相比于梯度法、阈值法、混合法、相对变化法、最大角度法和最优线性插值法在识别结果上具备更大的QI值。表明该方法能够准确识别混合层深度。  相似文献   

对基础测绘"十四五"规划的若干思考     

阮于洲  王晨阳 《测绘通报》2019,(11):153-155

着眼于明确机构改革后基础测绘在自然资源管理业务格局中的职责定位、工作重点，以及如何按照新《测绘法》更好地履行"为经济建设、国防建设、社会发展和生态保护服务"的法定要求，分析了"十四五"基础测绘发展的基本形势，据此提出"十四五"规划工作的基本思路和主要遵循，明确了工作重点和相关措施，相关观点已经在"十四五"基础测绘规划编制工作中得到体现。  相似文献   

方程误差系统的多新息辨识方法     

丁锋 《南京气象学院学报》2015,7(5):385-407

多新息方法可以用于线性系统和非线性系统的自适应滤波、参数估计、自校正控制、自适应故障检测与诊断等.线性系统包括两种基本类型:方程误差类系统和输出误差类系统.本文将多新息辨识应用到方程误差滑动平均(EEMA)系统(即CARMA系统),研究多新息增广随机梯度算法和多新息增广最小二乘算法,应用到方程误差自回归滑动平均(EEARMA)系统(即CARARMA系统),提出基于分解的多新息广义增广随机梯度算法和基于分解的多新息广义增广最小二乘算法,以及基于滤波的多新息广义增广随机梯度算法和基于滤波的多新息广义增广最小二乘算法.  相似文献   

船舶自动气象站分类标准及仪器布设原则     

张玉洁  安忠亮  高林  涂爱琴  宋传经 《山东气象》2015,35(3):40-43

本文在研究分析各类船舶的基础上,对船舶自动气象站(船舶站)的基本构成和采集要素进行了分类,提出了船舶站构成的分类标准,解决了不同船舶选取安装不同要素自动站选择依据不足的问题,详述了船舶站的构成。以典型船舶站为例,详述了温、压、湿、风、降水、能见度、辐射等观测要素的安装位置选择,为船舶站的设计和安装提供参考依据。  相似文献   

城镇地籍基础地理数据建库方法探讨     

蔡素真 《福建地质》2011,30(1):67-73

通过对第二次全国土地调查城镇地籍调查数据建库标准的分析,提出一套基于大比例尺城镇地形图开展基础地理数据建库的方法,探讨利用数据建库成果地形图图式的符号化回放,既满足城镇地形图的出图效果又满足基础地理数据GIS方法管理的需求.  相似文献   

新疆孔雀河流域下游平原灌区土壤盐碱化改良的原则与治理措施研究     

郭健  郭琳  张兵 《地下水》2011,(4):46-48

根据孔雀河流域下游平原灌区自然地理特征,分析盐碱地形成的原因,探讨实施治理盐碱地改良利用应遵守的原则,提出以水利土壤改良为先导,配以农艺改良和生物改良等治理综合措施。以期达到盐碱地标本兼治的目的,从而实现农业可持续发展。  相似文献   

煤田地质钻探中“真烧假脱断”事故的处理     

杜贵亭 《中国煤炭地质》2011,(2):68-70

＂真烧假脱断＂事故在煤田地质钻探施工中比较常见,容易误判为钻具脱扣或折断的烧钻事故。该事故多发生在夜班,以零时至凌晨5时为事故的多发时段;事故产生的主要原因是钻具接箍密封不严,水龙头堵塞,泥浆泵故障和其它因素引起的泥浆不能正常输送到孔底而产生。针对事故的特点,在实践中总结出＂存疑求原、解释合理、逐一破劲、砸反结合＂的处理原则和＂稳、准、静、决＂的处理步骤。郏县王集勘探区某孔和登封某勘探区某孔的处理结果表明,该处理原则和步骤切实可行,对指导同类事故的处理有一定的借鉴意义。  相似文献