Ukwatta, T. N. 2010 暴源系中的时延-光度统计关系
主要内容:
有红移,对Swift暴做的,100-200keV和300-400keV(但BAT不是这个波段呀?)
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Title: | The lag-luminosity relation in the gamma-ray burst source-frame | |
Authors: | Ukwatta, T. N.; Dhuga, K. S.; Stamatikos, M.; Sakamoto, T.; Parke, W. C.; Barthelmy, S. D.; Gehrels, N. | |
Publication: | eprint arXiv:1003.0229 | |
Publication Date: | 02/2010 | |
Origin: | ARXIV | |
Keywords: | Astrophysics - High Energy Astrophysical Phenomena | |
Comment: | Accepted to be published in the Proceedings of "The Shocking Universe - Gamma-Ray Bursts and High Energy Shock Phenomena", Venice (Italy), September 14-18, 2009 | |
Bibliographic Code: | 2010arXiv1003.0229U |
Abstract
We have investigated the empirical lag-luminosity relation in the Gamma-ray Burst (GRB) source-frame. We selected two energy bands (100-200 keV and 300-400 keV) in the GRB source-frame, which after redshift correction, lie in the observer-frame energy range of the Swift Burst Alert Telescope (BAT). The spectral lags between these energy channels are then presented as a function of the isotropic peak luminosity of the GRBs in the sample.Bibtex entry for this abstract Preferred format for this abstract (see Preferences)
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