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Spectral Cross-Calibration of Fermi-GBM and INTEGRAL-ISGRI using Gamma-Ray Bursts

机译:使用伽马射线爆发的Fermi-GBM和ISGRI的光谱交叉校准

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We present an extended cross-calibration study between the Fermi Gamma-Ray Burst Monitor (GBM) and the INTEGRAL Soft Gamma-Ray Imager ISGRI. A previous sample contained 4 GRBs; GRB081226B; GRB090107B; GRB090625B and GRB090704. A long burst detected by both instruments, GRB090817, provides us with the opportunity to further test the agreement between the previous sample and the new data. GRB090817 contains significant telemetry gaps in the ISGRI data set and methods were devised to account for these gaps. The combined datasets from both instruments for GRB090817 were fit with 3 separate spectral models - a Power Law (PL), Cut-Off Power Law (COPL) and a Band model. The best fit joint spectral model is shown for the time averaged and time resolved joint spectral fits. As a measure of relative flux between the two instruments, a normalisation constant was calculated from the joint spectral fitting.
机译:我们在Fermi Gamma射线突发监视器(GBM)和积分软伽马射线成像仪Isgri之间呈现了一个扩展的交叉校准研究。以前的样本包含4个GRB; grb081226b; grb090107b; GRB090625B和GRB090704。仪器GRB090817检测到的长突发,为我们提供了进一步测试先前样本与新数据之间的协议的机会。 GRB090817包含ISGri数据集中的重要遥测间隙,并设计了方法以占这些差距。来自GRB090817的两个仪器的组合数据集适用于3个单独的光谱型号 - 动力法(PL),截止电源法(COPL)和带模型。显示最佳拟合接合光谱模型的时间平均和时间分辨的接合谱配合。作为两种仪器之间的相对磁通量的衡量标准,从联合光谱配件计算归一化常数。

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