A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey
文献类型：期刊论文
| 作者 | Wang JL(王锦良)1,2,3,4 ; Ding X(丁旭)1,2,3,4; Li JJ(李佳佳)1,2,3,4; Xiong JP(熊建萍)4; Cheng QY(程其原)1,2,3,4; Ji KF(季凯帆)1,2,3,4
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| 刊名 | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
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| 出版日期 | 2024-08-01 |
| 卷号 | 273期号:2 |
| ISSN号 | 0067-0049 |
| DOI | 10.3847/1538-4365/ad5953 |
| 产权排序 | 第1完成单位 |
| 文献子类 | Article |
| 英文摘要 | With the continuous development of large optical surveys, a large number of light curves of late-type contact binary systems (CBs) have been released. Deriving parameters for CBs using the the Wilson-Devinney program and the PHOEBE program poses a challenge. Therefore, this study developed a method for rapidly deriving light curves based on the Neural Networks model combined with the Hamiltonian Monte Carlo (HMC) algorithm (NNHMC). The neural network was employed to establish the mapping relationship between the parameters and the pregenerated light curves by the PHOEBE program, and the HMC algorithm was used to obtain the posterior distribution of the parameters. The NNHMC method was applied to a large contact binary sample from the Catalina Sky Survey, and a total of 19,104 late-type contact binary parameters were derived. Among them, 5172 have an inclination greater than 70 degrees and a temperature difference less than 400 K. The obtained results were compared with the previous studies for 30 CBs, and there was an essentially consistent goodness-of-fit (R 2) distribution between them. The NNHMC method possesses the capability to simultaneously derive parameters for a vast number of targets. Furthermore, it can provide an extremely efficient tool for the rapid derivation of parameters in future sky surveys involving large samples of CBs. |
| 学科主题 | 天文学 ; 恒星与银河系 |
| URL标识 | 查看原文 |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| WOS关键词 | MASS-RATIO ; LIGHT CURVES ; PERIOD ; STATISTICS ; EVOLUTION ; LYRAE |
| 资助项目 | Natural Science Foundation of China[12103088]; Natural Science Foundation of China[12303106]; National Aeronautics and Space Administration[NNG05GF22G]; US National Science Foundation[AST-0909182]; US National Science Foundation[AST-1313422]; US National Science Foundation[AST-1413600]; US National Science Foundation[AST-1518308] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001281165000001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | Natural Science Foundation of China[12103088, 12303106] ; National Aeronautics and Space Administration[NNG05GF22G] ; US National Science Foundation[AST-0909182, AST-1313422, AST-1413600, AST-1518308] |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/27511]  |
| 专题 | 天文技术实验室 云南天文台_大样本恒星演化研究组 云南天文台_丽江天文观测站（南方基地） 云南天文台_中国科学院天体结构与演化重点实验室 |
| 作者单位 | 1.University of the Chinese Academy of Sciences, Yuquan Road 19#, Shijingshan Block, 100049 Beijing, People's Republic of China 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China; 3.Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P.O. Box 110, 650216 Kunming, People's Republic of China; 4.Yunnan Observatories, Chinese Academy of Sciences (CAS), P.O. Box 110, 650216 Kunming, People's Republic of China; dingxu@ynao.ac.cn; |
| 推荐引用方式 GB/T 7714 | Wang JL,Ding X,Li JJ,et al. A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2024,273(2). |
| APA | 王锦良,丁旭,李佳佳,熊建萍,程其原,&季凯帆.(2024).A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,273(2). |
| MLA | 王锦良,et al."A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 273.2(2024). |
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