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Fermi/LAT observations of GRB 110625A
Tam, P.H.T. ; Kong, A.K.H. ; Fan, Y.-Z.
2013
Source PublicationEAS Publications Series
ISSN1633-4760
Volume61Pages:83-85
Corresponding AuthorTam, P.H.T. (Institute of Astronomy and Department of Physics, National Tsing Hua University, Hsinchu 30013, Taiwan)
AbstractWe report γ-ray afterglow observations of GRB 110625A using Fermi's Large Area Telescope (LAT) above 100 MeV. Gamma-ray emission was clearly detected using data taken between 180 s and 580 s after the burst. The GeV light curve differs from a power-law decay, and probably consists of two emission periods. Simultaneous Swift/XRT observations did not show flaring behaviors, distinguishing its origin of the extended GeV emission from the case of GRB 100728A. © EAS, EDP Sciences 2013.(5 refs)
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/9790
Collection暗物质和空间天文实验室
Recommended Citation
GB/T 7714
Tam, P.H.T.,Kong, A.K.H.,Fan, Y.-Z.. Fermi/LAT observations of GRB 110625A[J]. EAS Publications Series,2013,61:83-85.
APA Tam, P.H.T.,Kong, A.K.H.,&Fan, Y.-Z..(2013).Fermi/LAT observations of GRB 110625A.EAS Publications Series,61,83-85.
MLA Tam, P.H.T.,et al."Fermi/LAT observations of GRB 110625A".EAS Publications Series 61(2013):83-85.
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