Detection of two TeV gamma-ray outbursts from NGC 1275 by LHAASO
文献类型:期刊论文
作者 | Cao, Zhen1,2,3; Aharonian, F.4,5; Axikegu6; Bai, Y. X.1,3; Bao, Y. W.7; Bastieri, D.8; Bi, X. J.1,2,3; Bi, Y. J.1,3; Bian, W.9; Bukevich, A. V.10 |
刊名 | Monthly Notices of the Royal Astronomical Society
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出版日期 | 2025-06-01 |
卷号 | 540期号:2页码:1860-1869 |
关键词 | methods: data analysis methods: statistical galaxies: active galaxies: jets gamma rays: general |
ISSN号 | 0035-8711 |
DOI | 10.1093/mnras/stae2512 |
产权排序 | 第30完成单位 |
文献子类 | Journal article (JA) |
英文摘要 | The Water Cherenkov Detector Array (WCDA) is one of the components of Large High Altitude Air Shower Observatory (LHAASO) and can monitor any sources over two-thirds of the sky for up to 7 h per day with >98 per cent duty cycle. In this work, we report the detection of two outbursts of the Fanaroff–Riley I radio galaxy NGC 1275 that were detected by LHAASO-WCDA between 2022 November and 2023 January with statistical significance of 5.2σ and 8.3σ. The observed spectral energy distribution in the range from 500 GeV to 3 TeV is fitted by a power law with the best-fitting spectral index of α = −3.37 ± 0.52 and −3.35 ± 0.29, respectively. The outburst flux above 0.5 TeV was (4.55 ± 4.21) × 10−11 cm−2 s−1 and (3.45 ± 1.78) × 10−11 cm−2 s−1, corresponding to 60 per cent and 45 per cent of Crab Nebula flux, respectively. Variation analysis reveals the variability time-scale of days at the TeV energy band. A simple test by one-zone synchrotron self-Compton model reproduces the data in the gamma-ray band well. © 2024 The Author(s). |
学科主题 | 天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学 |
URL标识 | 查看原文 |
资助项目 | National Natural Science Foundation of China[12173039];National Natural Science Foundation of China[12173066];National Natural Science Foundation of China[12175121];National Natural Science Foundation of China[12393813];National Natural Science Foundation of China[12393851];National Natural Science Foundation of China[12393852];National Natural Science Foundation of China[12393853];National Natural Science Foundation of China[12393854] |
语种 | 英语 |
资助机构 | National Natural Science Foundation of China[12173039, 12173066, 12175121, 12393813, 12393851, 12393852, 12393853, 12393854] |
源URL | [http://ir.ynao.ac.cn/handle/114a53/28374] ![]() |
专题 | 星系类星体研究组 |
作者单位 | 1.Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China; 2.University of Chinese Academy of Sciences, Beijing, 100049, China; 3.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China; 4.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2, Dublin, Ireland; 5.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, D-69029, Germany; 6.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China; 7.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China; 8.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China; 9.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China; 10.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia; |
推荐引用方式 GB/T 7714 | Cao, Zhen,Aharonian, F.,Axikegu,et al. Detection of two TeV gamma-ray outbursts from NGC 1275 by LHAASO[J]. Monthly Notices of the Royal Astronomical Society,2025,540(2):1860-1869. |
APA | Cao, Zhen.,Aharonian, F..,Axikegu.,Bai, Y. X..,Bao, Y. W..,...&Stepanov, V..(2025).Detection of two TeV gamma-ray outbursts from NGC 1275 by LHAASO.Monthly Notices of the Royal Astronomical Society,540(2),1860-1869. |
MLA | Cao, Zhen,et al."Detection of two TeV gamma-ray outbursts from NGC 1275 by LHAASO".Monthly Notices of the Royal Astronomical Society 540.2(2025):1860-1869. |
入库方式: OAI收割
来源:云南天文台
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