Accurate identification of X-ray single photons using multi-dimensional features and positive-unlabeled learning

IF 2.9 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Zhihui Lyu, Shuai Jia, Fei Wei, Songwu Peng
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引用次数: 0

Abstract

Traditional thresholding for X-ray astronomical detection faces challenges in balancing low-energy photon detection efficiency and noise suppression. This paper proposes an innovative algorithm based on multidimensional feature engineering and positive-unlabeled (PU) learning. The algorithm constructs morphological features of photon events, greatly enhancing the ability to distinguish photons from noise. By combining the PU learning framework with an adaptive threshold, the algorithm addresses the identification of low-energy photons. Experimental results show that its ability to distinguish photons from noise (d’ value of 1489.49) far surpasses the upper limit of conventional methods (maximum d’ value of 11.13). The algorithm accurately recovers the low-energy spectrum, which traditional methods severely distort. This leads to more than an order of magnitude improvement in spectrum recovery accuracy (NMSE). The algorithm demonstrates excellent performance in single-photon identification, providing key technology for realizing the potential of CMOS detectors in space exploration.

Abstract Image

利用多维特征和正无标记学习精确识别x射线单光子
传统的x射线天文探测阈值方法面临着低能量光子探测效率与噪声抑制平衡的挑战。本文提出了一种基于多维特征工程和正无标签学习的创新算法。该算法构建了光子事件的形态特征,大大提高了分辨光子和噪声的能力。该算法将PU学习框架与自适应阈值相结合,解决了低能光子的识别问题。实验结果表明,该方法分辨光子和噪声的能力(d′值为1489.49)远远超过常规方法的上限(最大d′值为11.13)。该算法准确地恢复了传统方法严重失真的低能谱。这使得光谱恢复精度(NMSE)提高了一个数量级以上。该算法在单光子识别方面表现出优异的性能,为实现CMOS探测器在空间探索中的潜力提供了关键技术。
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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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