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Triggering the Untriggered: The First Einstein Probe-detected Gamma-Ray Burst 240219A and Its Implications
Yin, Yi-Han Iris1,2; Zhang, Bin-Bin1,2,3; Yang, Jun1,2; Sun, Hui4; Zhang, Chen4; Shao, Yi-Xuan1,2; Hu, You-Dong5; Zhu, Zi-Pei4; Xu, Dong4; An, Li6,7; Gao, He6,7; Wu, Xue-Feng3; Zhang, Bing8,9; Castro-Tirado, Alberto Javier5,10; Pandey, Shashi B.11; Rau, Arne12; Lei, Weihua13; Xie, Wei14; Ghirlanda, Giancarlo15,16; Piro, Luigi17; O'Brien, Paul18; Troja, Eleonora19,20; Jonker, Peter21; Yu, Yun-Wei22; An, Jie4; Chen, Run-Chao1,2; Chen, Yi-Jing1; Dong, Xiao-Fei1,2; Eyles-Ferris, Rob18; Fan, Zhou4; Fu, Shao-Yu4; Fynbo, Johan P. U.23,24; Gao, Xing25; Huang, Yong-Feng1,2; Jiang, Shuai-Qing4; Jiang, Ya-Hui1; Julakanti, Yashaswi18; Kuulkers, Erik26; Lao, Qing-Hui1; Li, Dongyue4; Ling, Zhi-Xing4; Liu, Xing4; Liu, Yuan4; Mou, Jia-Yu1; Pan, Xin4; Wei, Daming3; Wu, Qinyu4; Yadav, Muskan19; Yang, Yu-Han19; Yuan, Weimin4; Zhang, Shuang-Nan27
2024-11-01
Source PublicationASTROPHYSICAL JOURNAL LETTERS
ISSN2041-8205
Volume975Issue:2Pages:L27
Contribution Rank25
AbstractThe Einstein Probe (EP) achieved its first detection and localization of a bright X-ray flare, EP240219a, on 2024 February 19, during its commissioning phase. Subsequent targeted searches triggered by the EP240219a alert identified a faint, untriggered gamma-ray burst (GRB) in the archived data of Fermi Gamma-ray Burst Monitor (GBM), Swift Burst Alert Telescope (BAT), and Insight-HXMT/HE. The EP Wide-field X-ray Telescope (WXT) light curve reveals a long duration of approximately 160 s with a slow decay, whereas the Fermi/GBM light curve shows a total duration of approximately 70 s. The peak in the Fermi/GBM light curve occurs slightly later with respect to the peak seen in the EP/WXT light curve. Our spectral analysis shows that a single cutoff power-law (PL) model effectively describes the joint EP/WXT-Fermi/GBM spectra in general, indicating coherent broad emission typical of GRBs. The model yielded a photon index of similar to-1.70 +/- 0.05 and a peak energy of similar to 257 +/- 134 keV. After detection of GRB 240219A, long-term observations identified several candidates in optical and radio wavelengths, none of which was confirmed as the afterglow counterpart during subsequent optical and near-infrared follow-ups. The analysis of GRB 240219A classifies it as an X-ray-rich GRB (XRR) with a high peak energy, presenting both challenges and opportunities for studying the physical origins of X-ray flashes, XRRs, and classical GRBs. Furthermore, linking the cutoff PL component to nonthermal synchrotron radiation suggests that the burst is driven by a Poynting flux-dominated outflow.
DOI10.3847/2041-8213/ad8652
Indexed BySCI
Language英语
WOS KeywordFLASHES ; MAGNETIZATION ; LUMINOSITY ; COMPONENTS ; EFFICIENT ; BEPPOSAX ; LAGS
Funding ProjectNational Key Research and Development Programs of China[2022YFF0711404] ; National Key Research and Development Programs of China[2022SKA0130102] ; National Key Research and Development Programs of China[2021YFA0718500] ; National SKA Program of China[2022SKA0130100] ; National Natural Science Foundation of China[11833003] ; National Natural Science Foundation of China[U2038105] ; National Natural Science Foundation of China[U1831135] ; National Natural Science Foundation of China[12121003] ; National Natural Science Foundation of China[12393811] ; National Natural Science Foundation of China[13001106] ; China Manned Space Project[CMS-CSST-2021-B11] ; Fundamental Research Funds for the Central Universities[D050102] ; Fundamental Research Funds for the Central Universities[HA 1850/28-1]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001347485800001
PublisherIOP Publishing Ltd
Funding OrganizationNational Key Research and Development Programs of China ; National SKA Program of China ; National Natural Science Foundation of China ; China Manned Space Project ; Fundamental Research Funds for the Central Universities
Citation statistics
Cited Times:10[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7121
Collection中国科学院新疆天文台
Corresponding AuthorZhang, Bin-Bin; Zhang, Chen
Affiliation1.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China
2.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210023, Peoples R China
3.Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China
4.Chinese Acad Sci, R P China, Beijing 550001, Peoples R China
5.Inst Astrofis Andalucia IAA CSIC, Glorieta Astron S-N, E-18008 Granada, Spain
6.Beijing Normal Univ, Beijing, Peoples R China
7.Beijing Normal Univ, Inst Frontier Astron & Astrophys, Beijing, Peoples R China
8.Univ Nevada Vegas, Las Vegas, NV USA
9.Univ Nevada Las Vegas, Dept Phys & Astron, Las Vegas, NV USA
10.Univ Malaga, Dept Ingn Sistemas & Automati, C Dr Ortiz Ramos Sn, Malaga, Spain
11.Aryabhatta Res Inst Observat Sci ARIES, Naini Tal, India
12.Max Planck Inst Extraterr Phys, Gieenbachstr, Garching, Germany
13.Huazhong Univ Sci & Technol, Sch Phys, Dept Astron, Wuhan 430074, Hubei, Peoples R China
14.Guizhou Normal Univ, Sch Phys & Elect Sci, Dept Astron, Guiyang 550001, Peoples R China
15.INAF Osservatorio Astron Brera, Via E Bianchi 46, Merate, LC, Italy
16.INFN, Sez Milano Bicocca, Piazza Sci 3, Milan, MI, Italy
17.INAF Ist Astrofis & Planetol Spaziali, Via Fosso del Cavaliere 100, Rome, Italy
18.Univ Leicester, Sch Phys & Astron, Univ Rd, Leicester LE1 7RH, England
19.Univ RomeTor Vergata, Dept Phys, Via Ric Sci 1, I-00133 Rome, Italy
20.INAF, Via Parco del Mellini, Rome, Italy
21.Radboud Univ Nijmegen, Dept Astrophys, IMAPP, NL-6500 GL Nijmegen, Netherlands
22.Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China
23.Cosm Dawn Ctr DAWN, DK-2200 Copenhagen, Denmark
24.Univ Copenhagen, Niels Bohr Inst, DK-2200 Copenhagen, Denmark
25.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
26.ESTEC, European Space Agcy, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands
27.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
Recommended Citation
GB/T 7714
Yin, Yi-Han Iris,Zhang, Bin-Bin,Yang, Jun,et al. Triggering the Untriggered: The First Einstein Probe-detected Gamma-Ray Burst 240219A and Its Implications[J]. ASTROPHYSICAL JOURNAL LETTERS,2024,975(2):L27.
APA Yin, Yi-Han Iris.,Zhang, Bin-Bin.,Yang, Jun.,Sun, Hui.,Zhang, Chen.,...&Zhang, Shuang-Nan.(2024).Triggering the Untriggered: The First Einstein Probe-detected Gamma-Ray Burst 240219A and Its Implications.ASTROPHYSICAL JOURNAL LETTERS,975(2),L27.
MLA Yin, Yi-Han Iris,et al."Triggering the Untriggered: The First Einstein Probe-detected Gamma-Ray Burst 240219A and Its Implications".ASTROPHYSICAL JOURNAL LETTERS 975.2(2024):L27.
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