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Yi-Zhong Fan
Researcher at Chinese Academy of Sciences
Publications - 375
Citations - 13754
Yi-Zhong Fan is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Gamma-ray burst & Afterglow. The author has an hindex of 55, co-authored 334 publications receiving 12158 citations. Previous affiliations of Yi-Zhong Fan include Niels Bohr Institute & University of Science and Technology of China.
Papers
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Journal ArticleDOI
Physical Processes Shaping Gamma-Ray Burst X-Ray Afterglow Light Curves: Theoretical Implications from the Swift X-Ray Telescope Observations
Bing Zhang,Yi-Zhong Fan,Yi-Zhong Fan,J. Dyks,Shiho Kobayashi,Shiho Kobayashi,Peter Mészáros,David N. Burrows,John A. Nousek,Neil Gehrels +9 more
TL;DR: In this article, the authors systematically analyze the possible physical processes that shape the properties of the early X-ray afterglow light curves and use the data to constrain various models.
Journal ArticleDOI
Physical processes shaping GRB X-ray afterglow lightcurves: theoretical implications from the Swift XRT observations
Bing Zhang,Yi-Zhong Fan,Jaroslaw Dyks,Shiho Kobayashi,Peter Mészáros,David N. Burrows,John A. Nousek,Neil Gehrels +7 more
TL;DR: In this paper, the authors systematically analyze the possible physical processes that shape the properties of the early X-ray afterglow lightcurves, and use the data to constrain various models.
Journal ArticleDOI
Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger
Elena Pian,P. D'Avanzo,Stefano Benetti,M. Branchesi,Enzo Brocato,Sergio Campana,Enrico Cappellaro,Stefano Covino,Valerio D'Elia,Johan P. U. Fynbo,Fedor Getman,G. Ghirlanda,Gabriele Ghisellini,A. Grado,G. Greco,Jens Hjorth,Chryssa Kouveliotou,Andrew J. Levan,Luca Limatola,D. Malesani,Paolo A. Mazzali,Paolo A. Mazzali,A. Melandri,Per Møller,Luciano Nicastro,Eliana Palazzi,S. Piranomonte,Andrea Rossi,Om Sharan Salafia,Om Sharan Salafia,Jonatan Selsing,G. Stratta,Masaomi Tanaka,Nial R. Tanvir,L. Tomasella,Darach Watson,Sheng Yang,Sheng Yang,Lorenzo Amati,Louis Antonelli,S. Ascenzi,S. Ascenzi,M. G. Bernardini,M. Boer,F. Bufano,Andrea Bulgarelli,Massimo Capaccioli,Piergiorgio Casella,A. J. Castro-Tirado,E. Chassande-Mottin,Riccardo Ciolfi,Chris M. Copperwheat,M. Dadina,G. De Cesare,A. Di Paola,Yi-Zhong Fan,Bruce Gendre,G. Giuffrida,Antonio Giunta,L. K. Hunt,G. L. Israel,Zhi-Ping Jin,Mansi M. Kasliwal,S. Klose,M. Lisi,Francesco Longo,Elisabetta Maiorano,Michela Mapelli,N. Masetti,N. Masetti,L. Nava,B. Patricelli,Daniel A. Perley,A. Pescalli,A. Pescalli,Tsvi Piran,A. Possenti,L. Pulone,M. Razzano,Ruben Salvaterra,Pietro Schipani,Mario Spera,Antonio Stamerra,Luigi Stella,Gianpiero Tagliaferri,Vincenzo Testa,Eleonora Troja,Massimo Turatto,S. D. Vergani,S. D. Vergani,D. Vergani +90 more
TL;DR: The spectral identification and physical properties of a bright kilonova associated with the gravitational-wave source GW170817 and γ-ray burst GRB 170817A associated with a galaxy at a distance of 40 megaparsecs from Earth are described.
Journal ArticleDOI
Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons
G. Ambrosi,Q. An,R. Asfandiyarov,P. Azzarello,P. Bernardini,B. Bertucci,M. S. Cai,Jin Chang,Donghong Chen,H. S. Chen,Jialong Chen,Wangli Chen,M. Y. Cui,T. S. Cui,A. D'Amone,A. De Benedittis,I. De Mitri,M. Di Santo,J.N. Dong,Tie-Kuang Dong,Y. F. Dong,Z. X. Dong,Giacinto Donvito,D. Droz,Kai-Kai Duan,Jinglai Duan,M. Duranti,D. D'Urso,R. R. Fan,Yi-Zhong Fan,Fang Fang,C. Q. Feng,Luzhao Feng,P. Fusco,V. Gallo,F. J. Gan,Min Gao,Shan-Shan Gao,F. Gargano,S. Garrappa,K. Gong,Y. Z. Gong,Dong Ya Guo,Jun-jun Guo,Y. M. Hu,Guangshun Huang,Y. Y. Huang,Maria Ionica,Dan Jiang,Wei Jiang,Xian-Min Jin,Jie Kong,Shi-Jun Lei,S.X. Li,X. X. Li,W. Li,Y. Li,Y. F. Liang,YM Liang,N. H. Liao,H. Liu,Jie Liu,S. B. Liu,Wei Liu,Yujuan Liu,F. Loparco,Michael Ma,Peng-Xiong Ma,S. Y. Ma,Tianxiao Ma,X.Q. Ma,X. Y. Ma,G. Marsella,M. N. Mazziotta,D. Mo,Niu Xiaoyang,X. Y. Peng,W. X. Peng,R. Qiao,J. N. Rao,M. M. Salinas,G. Z. Shang,W. H. Shen,Z.-Q. Shen,Z. T. Shen,Ju-Xian Song,H. Su,Meng Su,Zhi-Yu Sun,A. Surdo,X. J. Teng,X.B. Tian,Andrii Tykhonov,Valerio Vagelli,S. Vitillo,Chi Wang,Huaguang Wang,Haiqiong Wang,J. Z. Wang,L. G. Wang,Qian Wang,S. Wang,Xixian Wang,X. L. Wang,Y. F. Wang,Yaping Wang,Yu-Sa Wang,S. C. Wen,Zheng Wang,D. M. Wei,J. J. Wei,Y. F. Wei,Di Wu,Jinfei Wu,Lihui Wu,Shumei Wu,Xin Wu,K. Xi,Z. Q. Xia,Y.L. Xin,H. T. Xu,Z. Xu,Z. Z. Xu,G. F. Xue,Yang Haibo,Peidong Yang,Yifan Yang,Zhongjie Yang,Huijun Yao,Y. H. Yu,Qiuju Yuan,Chuan Yue,J. J. Zang,Chao Zhang,D.L. Zhang,Fengtao Zhang,Jie Zhang,Jindan Zhang,Jindong Zhang,Laiyu Zhang,Pengchao Zhang,Shengxia Zhang,W. Zhang,Y. Zhang,Y. J. Zhang,Yun-Zhi Zhang,Yugang Zhang,Yaohui Zhang,Zhihua Zhang,Zhoubin Zhang,Hong Yun Zhao,Huan Zhao,Xin-Fu Zhao,Chengrui Zhou,Yali Zhou,Xi Zhu,Yu-Xuan Zhu,Stephan Zimmer +157 more
TL;DR: The direct detection of a spectral break at about 0.9 teraelectronvolts confirms the evidence found by previous indirect measurements, clarifies the behaviour of the CRE spectrum at energies above 1 terAElectronvolt and sheds light on the physical origin of the sub-teraelectronsvolt CREs.
Journal ArticleDOI
A possible macronova in the late afterglow of the long-short burst GRB 060614
Bin Yang,Zhi-Ping Jin,Xiang Li,Stefano Covino,Xian-Zhong Zheng,Kenta Hotokezaka,Yi-Zhong Fan,Tsvi Piran,Da-Ming Wei +8 more
TL;DR: The discovery of near-infrared bump that is significantly above the regular decaying afterglow is reported, which is inconsistent with even the weakest known supernova.