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Ground Calibration of the Silicon Drift Detectors for NICER

机译:硅漂移探测器的地面校准

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The Neutron star Interior Composition ExploreR (NICER) is set to be deployed on the International Space Station (ISS) in early 2017. It will use an array of 56 Silicon Drift Detectors (SDDs) to detect soft X-rays (0.2 - 12 keV) with 100 nanosecond timing resolution. Here we describe the effort to calibrate the detectors in the lab primarily using a Modulated X-ray Source (MXS). The MXS that was customized for NICER provides more than a dozen emission lines spread over the instrument bandwidth, providing calibration measurements for detector gain and spectral resolution. In addition, the fluorescence source in the MXS was pulsed at high frequency to enable measurement of the delay due to charge collection in the silicon and signal processing in the detector electronics. A second chamber, designed to illuminate detectors with either ~(55)Fe, an optical LED, or neither, provided additional calibration of detector response, optical blocking, and effectiveness of background rejection techniques. The overall ground calibration achieved total operating time that was generally in the range of 500-1500 hours for each of the 56 detectors.
机译:中子星形内部成分探险家(更好)将在2017年初部署在国际空间站(ISS)上。它将使用56个硅漂移探测器(SDDS)阵列来检测软X射线(0.2 - 12 Kev )具有100个纳秒时序分辨率。在这里,我们描述了努力主要使用调制的X射线源(MXS)来校准实验室中的探测器。这是定制的NICER MXS提供十几发射线分布在仪器带宽,检测器增益和光谱分辨率提供校准测量。另外,MXS中的荧光源以高频率脉冲,以便在硅中的电荷收集和检测器电子设备中的信号处理来实现由于电荷收集而导致的延迟的测量。第二腔室,设计用于用〜(55)Fe,光学LED或既不提供〜(55)FE,光学LED,光学阻塞和背景抑制技术有效性的额外校准的探测器。整体地校准实现了56个探测器中的每一个通常在500-1500小时范围内的总操作时间。

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