The first cut is the cheapest: optimizing Athena/X-IFU-like TES detectors resolution by filter truncation

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
M. Teresa Ceballos, Nicolás Cardiel, Beatriz Cobo, Stephen J. Smith, Michael C. Witthoeft, Philippe Peille, Malcolm S. Durkin
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引用次数: 0

Abstract

The X-ray Integral Field Unit (X-IFU) instrument on the future ESA mission Athena X-ray Observatory is a cryogenic micro-calorimeter array of Transition Edge Sensor (TES) detectors designed to provide spatially-resolved high-resolution spectroscopy. The onboard reconstruction software provides energy, spatial location and arrival time of incoming X-ray photons hitting the detector. A new processing algorithm based on a truncation of the classical optimal filter and called 0-padding, has been recently proposed aiming to reduce the computational cost without compromising energy resolution. Initial tests with simple synthetic data displayed promising results. This study explores the slightly better performance of the 0-padding filter and assess its final application to real data. The goal is to examine the larger sensitivity to instrumental conditions that was previously observed during the analysis of the simulations. This 0-padding technique is thoroughly tested using more realistic simulations and real data acquired from NASA and NIST laboratories employing X-IFU-like TES detectors. Different fitting methods are applied to the data, and a comparative analysis is performed to assess the energy resolution values obtained from these fittings. The 0-padding filter achieves energy resolutions as good as those obtained with standard filters, even with those of larger lengths, across different line complexes and instrumental conditions. This method proves to be useful for energy reconstruction of X-ray photons detected by the TES detectors provided proper corrections for baseline drift and jitter effects are applied. The finding is highly promising especially for onboard processing, offering efficiency in computational resources and facilitating the analysis of sources with higher count rates at high resolution.

Abstract Image

第一刀最便宜:通过滤波器截断优化 Athena/X-IFU-like TES 探测器的分辨率
欧空局未来飞行任务雅典娜 X 射线天文台上的 X 射线积分场单元(X-IFU)仪器是一个由过渡边缘传感器(TES)探测器组成的低温微量子计阵列,旨在提供空间分辨的高分辨率光谱。机载重建软件可提供射入探测器的 X 射线光子的能量、空间位置和到达时间。最近提出了一种基于经典最优滤波器截断的新处理算法,称为 "0-填充",目的是在不影响能量分辨率的情况下降低计算成本。利用简单的合成数据进行的初步测试显示了良好的结果。本研究探讨了 0-padding 滤波器略胜一筹的性能,并对其在真实数据中的最终应用进行了评估。目的是检验之前在模拟分析过程中观察到的对仪器条件的较大敏感性。使用更真实的模拟和从 NASA 和 NIST 实验室获得的真实数据,对这种 0 填充技术进行了全面测试,这些数据都采用了类似 X-IFU 的 TES 探测器。对数据采用了不同的拟合方法,并进行了比较分析,以评估从这些拟合方法中获得的能量分辨率值。在不同的线复合体和仪器条件下,0-填充滤波器所获得的能量分辨率不亚于标准滤波器,即使是长度较大的滤波器也不例外。事实证明,只要对基线漂移和抖动效应进行适当的修正,这种方法就能对 TES 探测器探测到的 X 射线光子进行能量重建。这一发现非常有前途,特别是在星载处理方面,它可以提高计算资源的效率,促进以高分辨率分析计数率更高的源。
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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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