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首页> 外文期刊>Advances in Astronomy >Systematic Spectral Lag Analysis of Swift Known-zGRBs
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Systematic Spectral Lag Analysis of Swift Known-zGRBs

机译:Swift已知zGRB的系统谱滞后分析

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摘要

The difference of photon arrival time, which is known as spectral lag, is well known characteristics ofgamma-ray bursts (GRBs). In particular, long duration GRBs show a soft lag which means that high energy photonsarrive earlier than soft photons. The lag-luminosity relation is the empirical relationship between the isotropic peak luminosity and the spectral lag. We calculated the spectral lags for 40 known redshift GRBs observed bySwiftaddition to the previous 31 GRB samples. We confirmed that most of our samples follow the lag-luminosity relation. However, we noticed that there are some GRBs which show a significant scatter from the relation. We also confirm that the relationship between the break time and the luminosity of the X-ray afterglow (so-called Dainotti relation) extends up to the lag-luminosity relation.
机译:光子到达时间的差异(称为光谱滞后)是伽马射线猝发(GRB)的众所周知的特征。特别是,长时间GRB显示出软滞后现象,这意味着高能光子比软光子更早到达。滞后-光度关系是各向同性峰值光度与光谱滞后之间的经验关系。我们通过对之前31个GRB样本的快速加法计算得出了40个已知的红移GRB的光谱滞后。我们确认我们的大多数样本都遵循滞后-亮度关系。但是,我们注意到有些GRB从该关系中显示出很大的分散。我们还证实,断裂时间与X射线余辉的发光度之间的关系(所谓的Dainotti关系)一直延伸到滞后发光度关系。

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