13 / 2024-06-14 15:55:25
Calibration for the SAMPA ASIC in HERD transition radiation detector front-end electronics
HERD,TRD detector,SAMPA,Calibration
摘要录用
Jieyu Zhu / Institute of modern physics, Chinese Academy of Sciences
Haibo Yang / Institute of modern physics, Chinese Academy of Sciences
Yangzhou Su / Institute of modern physics, Chinese Academy of Sciences
The High Energy cosmic-Radiation Detection facility (HERD) is a part of the Chinese Cosmic Lighthouse Program in China’s Space Station, which will be launched in 2027. HERD is expected to work 10 years in orbit and will indirectly detect dark matter, measure cosmic rays and observe high-energy gamma rays. As a sub-detector of HERD, the transition radiation detector's (TRD) main scientific goal is to calibrate the electromagnetic Calorimeter (CALO) at the TeV energy range, improve the measurement accuracy of the CALO, and detect astronomical phenomena of high-energy gamma rays. The front-end readout electronic (FEE) of the prototype of TRD uses four SAMPA ASICs for 128 signals of anode, realizing a high-speed, low-power, and high-reliability data acquisition system. In this work, we completed the calibrations of the gain and shaping time in the unsupported modes of SAMPA to achieve adjustable dynamic range on orbit. The effect of the different fitting algorithm on the test results is also discussed under different modes of operation.

 
重要日期
  • 会议日期

    10月13日

    2024

    10月18日

    2024

  • 10月18日 2024

    报告提交截止日期

  • 10月31日 2024

    初稿截稿日期

  • 01月31日 2025

    注册截止日期

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University of Science and Technology of China
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