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CCD detector development for the eROSITA space telescope

机译:eROSITA太空望远镜的CCD检测器开发

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The German X-ray telescope eROSITA is the core instrument on the Russian satellite Spectrum-Roentgen-Gamma (SRG). Its scientific goal is the exploration of the X-ray Universe in the energy band from about 0.3 keV up to 10 keV with excellent energy, time and spatial resolution and large effective telescope area. The launch of the SRG satellite is scheduled for 2013. The observational program divides the planned mission duration of seven years into an all-sky survey and pointed observations. For detection of the single X-ray photons with high resolution, adequate frame transfer pnCCDs and the associated front-end electronics have been developed. The back-illuminated, 450 μm thick and fully depleted pnCCDs with a 3 cm × 3 cm large image area have been produced in the MPI Halbleiterlabor in the course of further development of the XMM-Newton X-ray pnCCDs. By means of the concept of back-illumination and full depletion of the chip thickness, high quantum efficiency is obtained over the entire energy band of interest. The performance of each eROSITA CCD was tested on chip level using a so-called ‘cold chuck probe station’. A special feature of this setup is that it allows spectroscopic measurements with a 55Fe source. Based on these results, we will select the seven best CCDs for the eROSITA focal plane cameras. An analog signal processor with 128 parallel channels has been developed for readout of the pnCCD signals. This ASIC permits fast and low-noise signal filtering. For a detailed characterization of the CCD detectors an appropriate control, supply and data acquisition electronics system was developed. We achieve a read noise of 2 electrons rms and an energy resolution of 135 eV FWHM for photons with energy of 5.9 keV. Even at the low X-ray energy of 280 eV, we measure a spectrum of Gaussian shape with a FWHM of 52 eV. However, the energy resolution will degrade during the seven years in space due to radiation damage caused --by protons. The radiation damage effect was studied and quantified for the eROSITA CCDs in an experiment. After successful development and verification of the CCD and its signal processor chip, we have started to assemble a flight-like eROSITA camera.
机译:德国X射线望远镜eROSITA是俄罗斯Spectrum-Roentgen-Gamma(SRG)卫星的核心仪器。它的科学目标是在从0.3 keV到10 keV的能带中探索X射线宇宙,它具有出色的能量,时间和空间分辨率以及较大的有效望远镜面积。 SRG卫星计划于2013年发射。观测计划将计划的七年任务持续时间分为全天候调查和有针对性的观测。为了检测具有高分辨率的单个X射线光子,已经开发了足够的帧传输pnCCD和相关的前端电子设备。在XMM-Newton X射线pnCCD的进一步开发过程中,MPI Halbleiterlabor生产了具有3 cm×3 cm大图像面积的背照式,厚度为450μm的,完全耗尽的pnCCD。通过背照和芯片厚度完全耗尽的概念,可以在整个感兴趣的能带上获得高量子效率。每个eROSITA CCD的性能都是使用所谓的“冷卡盘探针台”在芯片级上进行测试的。此设置的一个特殊功能是它允许使用 55 Fe源进行光谱测量。基于这些结果,我们将为eROSITA焦平面相机选择七种最佳CCD。已经开发出具有128个并行通道的模拟信号处理器,用于读取pnCCD信号。该ASIC允许快速和低噪声的信号过滤。为了详细描述CCD检测器,开发了适当的控制,供应和数据采集电子系统。对于能量为5.9 keV的光子,我们获得了2个电子均方根值的读取噪声和135 eV FWHM的能量分辨率。即使在280 eV的低X射线能量下,我们也能以52 eV的FWHM测量高斯形状的光谱。但是,由于造成的辐射损伤,在太空中的能量分辨率将在7年内下降- -- 由质子。在实验中对eROSITA CCD的辐射损伤效应进行了研究和量化。在成功开发并验证了CCD及其信号处理器芯片之后,我们已经开始组装类似飞行的eROSITA相机。

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