Investigation of stellar magnetic activity using variational autoencoder based on low-resolution spectroscopic survey
文献类型:期刊论文
作者 | Xiang Y(项越)2,3; Gu SH(顾盛宏)1,2,3; Cao DT(曹东涛)2,3 |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
出版日期 | 2022-07-06 |
卷号 | 514期号:4页码:4781-4793 |
ISSN号 | 0035-8711 |
关键词 | methods: data analysis techniques: spectroscopic stars: activity stars: chromospheres |
DOI | 10.1093/mnras/stac1693 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | We apply the variational autoencoder (VAE) to the LAMOST-K2 low-resolution spectra to detect the magnetic activity of the stars in the K2 field. After the training on the spectra of the selected inactive stars, the VAE model can efficiently generate the synthetic reference templates needed by the spectral subtraction procedure, without knowing any stellar parameters. Then, we detect the peculiar spectral features, such as chromospheric emissions, strong nebular emissions, and lithium absorptions, in our sample. We measure the emissions of the chromospheric activity indicators, H alpha and Ca ii infrared triplet (IRT) lines, to quantify the stellar magnetic activity. The excess emissions of H alpha and Ca ii IRT lines of the active stars are correlated well to the rotational periods and the amplitudes of light curves derived from the K2 photometry. We degrade the LAMOST spectra to simulate the slitless spectra of the China Space Station Telescope (CSST) and apply the VAE to the simulated data. For cool active stars, we reveal a good agreement between the equivalent widths of H alpha line derived from the spectra with two resolutions. The result indicates the ability of identifying the magnetically active stars in the future CSST survey, which will deliver an unprecedented large data base of low-resolution spectra as well as simultaneous multiband photometry of stars. |
学科主题 | 天文学 ; 恒星与银河系 |
URL标识 | 查看原文 |
出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
WOS关键词 | RELATIVE FLUX CALIBRATION ; DIGITAL SKY SURVEY ; 1ST DATA RELEASE ; LAMOST OBSERVATIONS ; X-RAY ; CHROMOSPHERIC EMISSION ; VARIABLE-STARS ; H-ALPHA ; SPECTRA ; I. |
资助项目 | China Manned Space Project[CMS-CSST-2021-B07] ; National Natural Science Foundation of China[10373023] ; National Natural Science Foundation of China[10773027] ; National Natural Science Foundation of China[U1531121] ; National Natural Science Foundation of China[11603068] ; National Natural Science Foundation of China[11903074] ; National Development and Reform Commission ; NASA Science Mission directorate |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000821228400008 |
资助机构 | China Manned Space Project[CMS-CSST-2021-B07] ; National Natural Science Foundation of China[10373023, 10773027, U1531121, 11603068, 11903074] ; National Development and Reform Commission ; NASA Science Mission directorate |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/25284] |
专题 | 云南天文台_系外行星研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Xiang Y(项越); Gu SH(顾盛宏) |
作者单位 | 1.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 101408, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China; 3.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China; |
推荐引用方式 GB/T 7714 | Xiang Y,Gu SH,Cao DT. Investigation of stellar magnetic activity using variational autoencoder based on low-resolution spectroscopic survey[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2022,514(4):4781-4793. |
APA | Xiang Y,Gu SH,&Cao DT.(2022).Investigation of stellar magnetic activity using variational autoencoder based on low-resolution spectroscopic survey.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,514(4),4781-4793. |
MLA | Xiang Y,et al."Investigation of stellar magnetic activity using variational autoencoder based on low-resolution spectroscopic survey".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 514.4(2022):4781-4793. |
入库方式: OAI收割
来源:云南天文台
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。