利用基于机器学习的周期分析有效检测可变天体

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
N. Chihara , T. Takata , Y. Fujiwara , K. Noda , K. Toyoda , K. Higuchi , M. Onizuka
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引用次数: 0

摘要

本文研究了亮度随时间周期性变化的变天体的有效探测问题。这个问题对于研究宇宙的演化和结构以及解释物理现象至关重要。Sesar等人的方法是利用天体时间序列的统计数据,如固有变率σ和χ2等,来检测可变天体的常用方法之一。然而,由于统计数据是天体时间序列的集合,以往的方法没有利用周期性这一可变天体的固有特性;它不能有效地发现多变的天体。为了解决这一问题,我们提出了一种利用周期分析来探测可变天体的方法。由于天体时间序列通常是稀疏的,稀疏建模可以有效地从稀疏时间序列中获得天体的周期性,因此我们的方法使用稀疏建模作为周期分析。利用天体的周期性作为特征,对某一天体进行二元分类,判断该天体是否为可变天体。为了证明我们方法的有效性,我们使用Hyper SuprimeCam (HSC) PDR2数据集对我们的方法进行了评估,我们确认了我们方法的AUC为0.939,而之前方法的AUC为0.750;我们的方法可以更有效地探测到多变的天体。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Effective detection of variable celestial objects using machine learning-based periodic analysis

This paper tackles the problem of effectively detecting variable celestial objects whose brightness periodically changes over time. This problem is crucial in studying the evolution and structure of the universe and elucidating physical phenomena. The method by Sesar et al. is one of the popular approaches used in detecting variable celestial objects that uses statistical data of celestial time series, such as intrinsic variability σ and χ2, etc. However, since statistical data is an aggregation of celestial time series, the previous approaches do not take advantage of the periodicity, which is the inherent characteristic of variable celestial objects; it fails to find variable celestial objects effectively. To solve such a problem, we propose an approach to detecting variable celestial objects using periodic analysis. Our approach uses sparse modeling as periodic analysis since celestial time series is typically sparse and sparse modeling can effectively obtain periodicities of the celestial objects from sparse time series. By exploiting the periodicities of the celestial objects as features, we perform binary classification to estimate whether a celestial object is a variable celestial object. To show the effectiveness of our approach, we evaluated our approach using Hyper SuprimeCam (HSC) PDR2 dataset, and we confirmed that AUC of our approach is 0.939 while AUC of the previous approach is 0.750; our approach can more effectively detect variable celestial objects.

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来源期刊
Astronomy and Computing
Astronomy and Computing ASTRONOMY & ASTROPHYSICSCOMPUTER SCIENCE,-COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
CiteScore
4.10
自引率
8.00%
发文量
67
期刊介绍: Astronomy and Computing is a peer-reviewed journal that focuses on the broad area between astronomy, computer science and information technology. The journal aims to publish the work of scientists and (software) engineers in all aspects of astronomical computing, including the collection, analysis, reduction, visualisation, preservation and dissemination of data, and the development of astronomical software and simulations. The journal covers applications for academic computer science techniques to astronomy, as well as novel applications of information technologies within astronomy.
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