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Cited article:
Yi-Ping Qin, Guang-Zhong Xie, En-Wei Liang, Xue-Tang Zheng
A&A, 369 2 (2001) 537-543
Published online: 2001-04-15
This article has been cited by the following article(s):
Distributions of the hardness ratio of short and long gamma-ray bursts in different time intervals within the first two seconds
Yun-Ming Dong and Yi-Ping Qin
Monthly Notices of the Royal Astronomical Society 358 (4) 1267 (2005)
DOI: 10.1111/j.1365-2966.2005.08746.x
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Average Curves of Emissivity of the Highest Pulses in Long and Short Gamma-Ray Bursts
En-Wei Liang, Guang-Zhong Xie and Cheng-Yue Su
Publications of the Astronomical Society of Japan 54 (1) 1 (2002)
DOI: 10.1093/pasj/54.1.1
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Are short Gamma Ray Bursts similar to long ones?
G. Ghirlanda, M.G. Bernardini, G. Calderone and P. D'Avanzo
Journal of High Energy Astrophysics 7 81 (2015)
DOI: 10.1016/j.jheap.2015.04.002
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Fluence–Hardness Correlation in Gamma-Ray Bursts
En-Wei Liang and Guang-Zhong Xie
Publications of the Astronomical Society of Japan 54 (3) 359 (2002)
DOI: 10.1093/pasj/54.3.359
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On the spectral lags of the short gamma-ray bursts
T. Yi, E. Liang, Y. Qin and R. Lu
Monthly Notices of the Royal Astronomical Society 367 (4) 1751 (2006)
DOI: 10.1111/j.1365-2966.2006.10083.x
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How Sample Completeness Affects Gamma‐Ray Burst Classification
Jon Hakkila, Timothy W. Giblin, Richard J. Roiger, et al.
The Astrophysical Journal 582 (1) 320 (2003)
DOI: 10.1086/344568
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Relation between the hardness ratio and time in the first two seconds for compatible samples of short and long gamma-ray bursts
Yi-Ping Qin and Yun-Ming Dong
Monthly Notices of the Royal Astronomical Society 358 (4) 1320 (2005)
DOI: 10.1111/j.1365-2966.2005.08794.x
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Sequences in the Hardness Ratio-Peak Energy Plane of Gamma-Ray Bursts
Xiao-Hong Cui, En-Wei Liang and Rui-Jing Lu
Chinese Journal of Astronomy and Astrophysics 5 (2) 151 (2005)
DOI: 10.1088/1009-9271/5/2/005
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Optical Photometric Observations of γ-Ray Loud Blazars
Jun-Hui Fan, O. M. Kurtanidze, M. G. Nikolashvili, et al.
Chinese Journal of Astronomy and Astrophysics 4 (2) 133 (2004)
DOI: 10.1088/1009-9271/4/2/133
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