partially supported by the Natural Science Foundation of Yunnan Province(grant No.202101AU070006);the Young and Middle-Aged Academic and Technical Reserve Talents of Yunnan Province(202205AC160087)。
Gamma-ray bursts(GRBs)exhibit powerful radiation and relativistic jets similar to blazars.However,the central engine of GRBs remains unknown.In this paper,we use the fundamental plane to analyze a sample of GRBs with ...
the National Natural Science Foundation of China(Nos.11773036 and 11533003);the Strategic Pioneer Program on Space Science,Chinese Academy of Sciences(Nos.XDA 15052600 and XDA 15016500);the Natural Science Foundation of Guangxi(2018GXNSFGA281007);by Bagui Young Scholars Program;support from the National Key Research and Development Project of China(No.2020YFE0202100)。
Rapid spectroscopy of GRB afterglows is an important and hard task.Based on the archival XSGRB spectral database,we here perform a pilot study on the afterglow's spectroscopy in the forthcoming SVOM era in two aspects...
supported by the National Basic Research Program of China (973 program, Grant Nos. 2012CB821800 and 2009CB824800);the National Natural Science Foundation of China(Grant Nos. 11225314, 11103026 and 10935001)
We analyze the emission plateaus in the X-ray afterglow light curves of gamma-ray bursts (GRBs) and those in the optical light curves of type Ⅱ plateau su- pernovae (SNe Ⅱ-P) in order to study whether they have ...
supported by the Open Research Program of the Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences
It is expected that there should be a spectral cutoff at the high energy end of emission from a prompt gamma-ray burst (GRB), due to, e.g. γγ absorption and/or a high energy cutoff in the electron distribution. We...
supported by the National Natural Science Foundation of China(Grant No.11073057)
The optical emission of GRB 110205A is distinguished by two flares. We examine two possible scenarios for the optical afterglow emission. In the first scenario, the first optical flare is the reverse shock emission of...
supported by the National Natural Science Foundation of China (Grant Nos. 10873009 and 11033002);the National Basic Research Program of China (973 Program;No. 2007CB815404)
We present broadband (radio, optical, X-ray and GeV) fits to the afterglow light curves and spectra of three long-duration gamma-ray bursts (GRBs 080916C, 090902B, and 090926A) detected by the Gamma-Ray Burst Moni...
supported by DGAPA-UNAM(Mexico) Project No.IN101409;Conacyt project No.103520(SS);supported by NASA NNX09AO94G;NSF AST0908362(BZ)
In the collapsar scenario of the long duration Gamma-Ray Bursts (GRBs), multi-TeV neutrino emission is predicted as the jet makes its way through the stellar envelope. Such a neutrino signal is also expected for mor...