伽玛暴(Gamma-Ray Burst)笔记。记录有关伽玛暴的新文章,另外也包括看的老文章、自己的想法、以及跟天文相关的一些东西。 Feel free to leave me a message by comments or by email.

星期四, 八月 26, 2010

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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文章信息:
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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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