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CALIBRATION OF THE MEGA PROTOTYPE

机译:Mega原型的校准

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Calibration measurements of the MEGA (Medium Energy Gamma-ray Astronomy) prototype have been performed with radioactive lab sources and at the High Intensity Gamma-ray Source (HIGS) at the Free Electron Laser Laboratory (FELL) of Duke University, Durham, NC. MEGA is a combined Compton scatter and pair creation telescope. It consists of two main detector units, the tracker and the calorimeter. Doublesided Silicon strip detectors form the tracker, which is surrounded by the pixelated CsI(Tl) blocks of the calorimeter. A prerequisite for successful data analysis is a calibration of each individual readout channel. This work is still ongoing. The performance of the detector units will be therefore presented as currently known. The encountered problems and the resulting (single detector) calibration methods will be described briefly. Since we aim at an energy range of 0.3 - 50 MeV, the HIGS — a Compton back-scattering source — with beams of mono-energetic, fully linearly polarized photons in the range of 0.7 - 50 MeV was a good match for the MEGA calibration. Measurements at various energies and for different incidence angles have been performed. Some preliminary results will be presented.
机译:Mega(中等能源伽马射线天文学)原型的校准测量已经通过放射性实验室来源和在Duke大学的自由电子激光实验室(下跌)的高强度伽马射源(HIG)进行了校准测量。 Mega是一个康普顿散落和配对创建望远镜。它由两个主探测器单元,跟踪器和量热计组成。双层硅条探测器形成跟踪器,其被热量计的像素化CSI(TL)块包围。成功数据分析的先决条件是每个单独的读数通道的校准。这项工作仍在继续。因此,检测器单元的性能将被呈现为当前已知的。将简要描述遇到的问题和所得到的(单检测器)校准方法。由于我们的目标是0.3 - 50 MeV的能量范围,HIGS - 康普顿背散射源 - 用0.7-50mev的范围内的单能级,完全线性极化光子的光束是Mega校准的良好匹配。已经进行了各种能量和不同入射角的测量。将提出一些初步结果。

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