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Fermi/GBM Observations of SGR J0501+4516

机译:Fermi / GBM SGR J0501 + 4516的观察

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The magnetar candidate SGR J0501+4516 was discovered when it became active for about 13 days from August 22 to September 3, 2008. During this period, the Gamma-ray Burst Monitor (GBM) onboard Fermi detected over 30 bursts. We present here our results on the temporal and spectral analysis of the 29 bursts for which high spectral and time resolution data is available. We find that the T_(90) durations of the bursts follow a log-normal distribution with a mean value of approx123 ms. We fit the time-integrated spectrum of each burst with several models: a black body function, optically thin thermal brehmsstrahlung, a power law with an exponential cut-off, two black body functions, and the combination of a black body and a power law. We discuss our results in the context of the spectral properties of other magnetar bursts and we also present some correlations between the spectral parameters of the best fit models for all bursts. Finally, we present the results of our time-resolved spectral analysis of the five brightest bursts and discuss how they compare with our time-integrated results.
机译:当它在2008年8月22日至9月3日起,它发生了大约13天的磁场候选SGR J0501 + 4516。在此期间,伽马射线爆发监测器(GBM)船上费米检测到30多个突发。我们在这里展示我们的结果对29个突发的时间和光谱分析,其中有哪些高频和时间分辨率数据。我们发现突发的T_(90)持续时间遵循对数正常分布,平均值为约123ms。我们适合每个突发的时间集成频谱,具有多种型号:黑色体功能,光学薄的热Brehmsstrahlung,一种具有指数截止的动力法,两个黑色身体功能,以及黑体和动力法的组合。我们在其他磁铁突发的光谱特性的背景下讨论我们的结果,并且我们还在所有突发的最佳拟合模型的光谱参数之间存在一些相关性。最后,我们展示了我们的时间 - 解决了五个最亮突发的频谱分析的结果,并讨论了它们与我们的时间综合结果进行比较。

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