NAOC Open IR
A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data
Guidorzi, C.1,2,3; Marongiu, M.1; Martone, R.1; Nicastro, L.3; Xiong, S. L.4; Liao, J. Y.4; Li, G.4; Zhang, S. N.4,5; Amati, L.3; Frontera, F.1,3; Orlandini, M.3; Rosati, P.1,2,3; Virgilli, E.1; Zhang, S.4; Bu, Q. C.4; Cai, C.4,5; Cao, X. L.4; Chang, Z.4; Chen, G.4; Chen, L.6; Chen, T. X.4; Chen, Y. B.7; Chen, Y. P.4; Cui, W.8; Cui, W. W.4; Deng, J. K.7; Dong, Y. W.4; Du, Y. Y.4; Fu, M. X.7; Gao, G. H.4,5; Gao, H.4,5; Gao, M.4; Ge, M. Y.4; Gu, Y. D.4; Guan, J.4; Guo, C. C.4,5; Han, D. W.4; Huang, Y.4; Huo, J.4; Jia, S. M.4; Jiang, L. H.4; Jiang, W. C.4; Jin, J.4; Jin, Y. J.9; Kong, L. D.4,5; Li, B.4; Li, C. K.4; Li, M. S.4; Li, T. P.4,5,8; Li, W.4; Li, X.4; Li, X. B.4; Li, X. F.4; Li, Y. G.4; Li, Z. W.4; Liang, X. H.4; Liu, B. S.4; Liu, C. Z.4; Liu, G. Q.7; Liu, H. W.4; Liu, X. J.4; Liu, Y. N.9; Lu, B.4; Lu, F. J.4; Lu, X. F.4; Luo, Q.4; Luo, T.4; Ma, R. C.4,5; Ma, X.4; Meng, B.4; Nang, Y.4,5; Nie, J. Y.4; Ou, G.10; Qu, J. L.4; Sai, N.4,5; Shang, R. C.7; Song, L. M.4,5; Song, X. Y.4; Sun, L.4; Tan, Y.4; Tao, L.4; Tuo, Y. L.4; Wang, C.5,11; Wang, G. F.4; Wang, J.4; Wang, W. S.10; Wang, Y. S.4; Wen, X. Y.4; Wu, B. Y.4,5; Wu, B. B.4; Wu, M.4; Xiao, G. C.4,5; Xiao, S.4,5; Xu, Y. P.4,5; Yang, J. W.4; Yang, S.4; Yang, Y. J.4; Yi, Q. B.4,12; Yin, Q. Q.4; You, Y.4,5; Zhang, A. M.4; Zhang, C. M.4; Zhang, F.4; Zhang, H. M.10; Zhang, J.4; Zhang, T.4; Zhang, W. C.4; Zhang, W.4,5; Zhang, W. Z.6; Zhang, Y.4; Zhang, Y. F.4; Zhang, Y. J.4; Zhang, Z.7; Zhang, Z. L.4; Zhang, H. S.4; Zhang, X. F.4,5; Zheng, S. J.4; Zhou, D. K.4,5; Zhou, J. F.9; Zhu, Y. X.4,13; Zhu, Y.4; Zhuang, R. L.9
2020-05-15
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume637Pages:13
AbstractContext. No robust detection of prompt electromagnetic counterparts to fast radio bursts (FRBs) has yet been obtained, in spite of several multi-wavelength searches having been carried out so far. Specifically, X/gamma-rays counterparts are predicted by some models. Aims. We aim to search for prompt gamma-ray counterparts in the Insight-Hard X-ray Modulation Telescope (Insight-HXMT) data, taking advantage of the unique combination of the large effective area in the keV-MeV energy range, and of sub-ms time resolution. Methods. We selected 39 FRBs that were promptly visible from the High-Energy (HE) instrument aboard Insight-HXMT. After calculating the expected arrival times at the location of the spacecraft, we searched for a significant excess in both individual and cumulative time profiles over a wide range of time resolutions, from several seconds down to sub-ms scales. Using the dispersion measures in excess of the Galactic terms, we estimated the upper limits on the redshifts. Results. No convincing signal was found, and for each FRB we constrained the gamma-ray isotropic-equivalent luminosity and the released energy as a function of emission timescale. For the nearest FRB source, the periodic repeater FRB 180916.J0158+65, we find L-gamma,L-& x2006;iso & x2004;< & x2004;5.5 x 10(47) erg s(-1) over 1 s, whereas L-gamma,L-& x2006;iso & x2004;< & x2004;10(49) - 10(51) erg s(-1) for the bulk of FRBs. The same values scale up by a factor of similar to 100 for a ms-long emission. Conclusions. Even on a timescale comparable with that of the radio pulse itself, no keV-MeV emission is observed. A systematic association with either long or short GRBs is ruled out with high confidence, except for sub-luminous events, as is the case for the core-collapse of massive stars (long) or binary neutron star mergers (short) viewed off axis. Only giant flares from extragalactic magnetars at least ten times more energetic than Galactic siblings are ruled out for the nearest FRB.
Keywordradiation mechanisms non-thermal radio continuum stars gamma-ray burst general
Funding OrganizationNational Program on Key Re-search and Development Project ; National Program on Key Re-search and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration (CNSA) ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF ; ASI-INAF ; National Program on Key Re-search and Development Project ; National Program on Key Re-search and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration (CNSA) ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF ; ASI-INAF ; National Program on Key Re-search and Development Project ; National Program on Key Re-search and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration (CNSA) ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF ; ASI-INAF ; National Program on Key Re-search and Development Project ; National Program on Key Re-search and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration (CNSA) ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF ; ASI-INAF
DOI10.1051/0004-6361/202037797
WOS KeywordSYNCHROTRON MASER EMISSION ; CURVATURE RADIATION ; LUMINOSITY FUNCTION ; POPULATION ; MAGNETAR ; SUPERNOVA ; GRB-060218 ; REDSHIFT ; ORIGINS ; FLARE
Language英语
Funding ProjectNational Program on Key Re-search and Development Project[2016YFA0400800] ; National Natural Science Foundation of China[11733009] ; National Natural Science Foundation of China[U1838201] ; National Natural Science Foundation of China[U1838202] ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF[2017-14-H.0]
Funding OrganizationNational Program on Key Re-search and Development Project ; National Program on Key Re-search and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration (CNSA) ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF ; ASI-INAF ; National Program on Key Re-search and Development Project ; National Program on Key Re-search and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration (CNSA) ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF ; ASI-INAF ; National Program on Key Re-search and Development Project ; National Program on Key Re-search and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration (CNSA) ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF ; ASI-INAF ; National Program on Key Re-search and Development Project ; National Program on Key Re-search and Development Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration (CNSA) ; China National Space Administration (CNSA) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; Universita di Ferrara through grant FIR 2018 "A Broad-band study of Cosmic Gamma-ray Burst Prompt and Afterglow Emission" ; ASI-INAF ; ASI-INAF
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000536554100008
PublisherEDP SCIENCES S A
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/54761
Collection中国科学院国家天文台
Corresponding AuthorGuidorzi, C.
Affiliation1.Univ Ferrara, Dept Phys & Earth Sci, Via Saragat 1, I-44122 Ferrara, Italy
2.Ist Nazl Fis Nucl, Sez Ferrara, Via Saragat 1, I-44122 Ferrara, Italy
3.INAF Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy
4.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, 19B Yuquan Rd, Beijing 100049, Peoples R China
5.Chinese Acad Sci, Univ Chinese Acad Sci, Beijing 100049, Peoples R China
6.Beijing Normal Univ, Dept Astron, Beijing 100088, Peoples R China
7.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
8.Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China
9.Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China
10.Chinese Acad Sci, Inst High Energy Phys, Comp Div, 19B Yuquan Rd, Beijing 100049, Peoples R China
11.Chinese Acad Sci, Natl Astron Observ, Key Lab Space Astron & Technol, Beijing 100012, Peoples R China
12.Xiangtan Univ, Sch Phys & Optoelect, Xiangtan 411105, Hunan, Peoples R China
13.Jilin Univ, Coll Phys, 2699 Qianjin St, Changchun 130012, Peoples R China
Recommended Citation
GB/T 7714
Guidorzi, C.,Marongiu, M.,Martone, R.,et al. A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data[J]. ASTRONOMY & ASTROPHYSICS,2020,637:13.
APA Guidorzi, C..,Marongiu, M..,Martone, R..,Nicastro, L..,Xiong, S. L..,...&Zhuang, R. L..(2020).A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data.ASTRONOMY & ASTROPHYSICS,637,13.
MLA Guidorzi, C.,et al."A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data".ASTRONOMY & ASTROPHYSICS 637(2020):13.
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