On the Origin of the Strong Optical Variability of Emission-line Galaxies | |
Lin, Ruqiu5,6; Zheng, Zhen-Ya6; Hu, Weida4; Jiang, Chunyan6; Pan, Xiang3; Yang, Chenwei3; Yuan, Fang-Ting6; Rahna, P. T.6; Wang JG(王建国)1,2; Wang, Yibo4 | |
刊名 | ASTROPHYSICAL JOURNAL |
2022-11-01 | |
卷号 | 940期号:1 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ac9232 |
产权排序 | 第5完成单位 |
文献子类 | Article |
英文摘要 | Emission-line galaxies (ELGs) are crucial for understanding the formation and evolution of galaxies, while little is known about their variability. Here we report on the optical variability of a sample of ELGs selected in the COSMOS field, which has narrowband observations in two epochs separated by ?12 yr. This sample was observed with the Suprime-Cam (SC) and Hyper Suprime-Cam (HSC) on the Subaru telescope in NB816 and bands, respectively. After carefully removing the wing effect of a narrowband filter, we check the optical variability in a sample of 181 spectroscopically confirmed ELGs. We find that 0 (0/68) H alpha emitters, 11.9% (5/42) [O iii] emitters, and 0 (0/71) [O ii] emitters show significant variability (|delta m(NB)| >= 3 sigma delta m(NLAGN)) in the two-epoch narrowband observations. We investigate the presence of active galactic nuclei (AGN) in this variable ELG (var-ELG) sample with three methods, including X-ray luminosity, mid-infrared activity, and radio excess. We find zero bright AGN in this var-ELG sample but cannot rule out the contribution from faint AGN. We find that supernovae explosions (SNe) could also dominate the variability of the var-ELG sample. The merger morphology shown in the HST/F814W images of the entire var-ELG sample is in agreement with the enhancement of star formation, i.e., the SNe activity. |
学科主题 | 天文学 ; 星系与宇宙学 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
资助项目 | National Science Foundation of China[12022303] ; China-Chile Joint Research Fund (CCJRF)[1906] ; CAS Pioneer Hundred Talents Program ; NSFC[U1931131] ; Funds for Key Programs of Shanghai Astronomical Observatory ; Natural Science Foundation of Shanghai[21ZR1474300] ; CAS President's International Fellowship Initiative (PIFI)[E085201009] ; China Manned Space Project[CMS-CSST-2021-A07] ; Japanese Cabinet Office ; Ministry of Education, Culture, Sports, Science and Technology (MEXT) ; Japan Society for the Promotion of Science (JSPS) ; Japan Science and Technology Agency (JST) ; Toray Science Foundation ; NAOJ ; Kavli IPMU ; KEK ; ASIAA ; Princeton University ; TAP member institutes ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; National Natural Science Foundation of China ; National Aeronautics and Space Administration |
WOS关键词 | ACTIVE GALACTIC NUCLEI ; EVOLUTION SURVEY COSMOS ; STAR-FORMATION RATE ; DIGITAL SKY SURVEY ; WIDE-FIELD SURVEY ; H-ALPHA ; LEGACY SURVEY ; DATA RELEASE ; 1ST RELEASE ; CLASSIFICATION |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP Publishing Ltd |
WOS记录号 | WOS:000886927900001 |
资助机构 | National Science Foundation of China[12022303] ; China-Chile Joint Research Fund (CCJRF)[1906] ; CAS Pioneer Hundred Talents Program ; NSFC[U1931131] ; Funds for Key Programs of Shanghai Astronomical Observatory ; Natural Science Foundation of Shanghai[21ZR1474300] ; CAS President's International Fellowship Initiative (PIFI)[E085201009] ; China Manned Space Project[CMS-CSST-2021-A07] ; Japanese Cabinet Office ; Ministry of Education, Culture, Sports, Science and Technology (MEXT) ; Japan Society for the Promotion of Science (JSPS) ; Japan Science and Technology Agency (JST) ; Toray Science Foundation ; NAOJ ; Kavli IPMU ; KEK ; ASIAA ; Princeton University ; TAP member institutes ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; National Natural Science Foundation of China ; National Aeronautics and Space Administration |
内容类型 | 期刊论文 |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/25656] |
专题 | 云南天文台_丽江天文观测站(南方基地) |
通讯作者 | Zheng, Zhen-Ya |
作者单位 | 1.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming, 650216, People's Republic of China 2.Yunnan Observatories (YNAO), Chinese Academy of Sciences, Kunming 650216, People's Republic of China; 3.Key Laboratory for Polar Science, MNR, Polar Research Institute of China, 451 Jinqiao Road, Shanghai, 200136, People's Republic of China; 4.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, Anhui 230026, People's Republic of China; 5.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, People's Republic of China; 6.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, People's Republic of China; zhengzy@shao.ac.cn; |
推荐引用方式 GB/T 7714 | Lin, Ruqiu,Zheng, Zhen-Ya,Hu, Weida,et al. On the Origin of the Strong Optical Variability of Emission-line Galaxies[J]. ASTROPHYSICAL JOURNAL,2022,940(1). |
APA | Lin, Ruqiu.,Zheng, Zhen-Ya.,Hu, Weida.,Jiang, Chunyan.,Pan, Xiang.,...&Zhu, Shuairu.(2022).On the Origin of the Strong Optical Variability of Emission-line Galaxies.ASTROPHYSICAL JOURNAL,940(1). |
MLA | Lin, Ruqiu,et al."On the Origin of the Strong Optical Variability of Emission-line Galaxies".ASTROPHYSICAL JOURNAL 940.1(2022). |
个性服务 |
查看访问统计 |
相关权益政策 |
暂无数据 |
收藏/分享 |
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。
修改评论