{"title":"First in-flight observation with the novel coincidence readout SiPM-based detectors of DRO/GTM","authors":"Jia-Cong Liu, Peng Zhang, Jin-Peng Zhang, Shao-Lin Xiong, Zheng-Hua An, Ya-Qing Liu, Xiang Ma, Da-Li Zhang, Chao Zheng, Ke Gong, Xin-Qiao Li, Xiang-Yang Wen, Chen-Wei Wang, Hao-Xuan Guo, Wen-Jun Tan, Yue Wang, Yang-Zhao Ren, Wang-Chen Xue, Zheng-Hang Yu, Yan-Qiu Zhang, Pei-Yi Feng, Min Gao, Yue Huang, Xiao-Bo Li, Xiao-Jing Liu, Ping Wang, Jin Wang, Jin-Zhou Wang, Sheng Yang, Xiao-Yun Zhao, Shi-Jie Zheng, Wen-Bin Wang, Hong-Fei Guan, Rui-Xue Wang, Yu Su, Cai-Yun Shao, Le-Le Xu, Fei Zhang","doi":"10.1007/s11433-026-2954-2","DOIUrl":null,"url":null,"abstract":"<div><p>SiPM-based gamma-ray detector has been increasingly utilized in space telescopes. However, its performance in the space environment would be significantly degraded, especially in the low-energy band, owing to the radiation-induced noise increase of SiPM. To address this problem, we have developed and implemented a novel coincidence readout design for SiPM-based detectors of the Gamma-ray Transient Monitor (GTM) onboard the DRO-A satellite (i.e., DRO/GTM). In this paper, we report the first in-flight observation results of DRO/GTM, focusing on the validation and performance studies of the coincidence readout technology, after a brief introduction of the working mode and data type of coincidence readout. We find that GTM detectors can correctly process and label coincidence events, identify the noise signals of SiPM, and safeguard the detection sensitivity of DRO/GTM especially in the low energy band, which is critically important for scientific observations in multi-messenger astronomy era. Our results not only validate the novel design of the coincident readout of DRO/GTM but also showcase its great advantages in mitigating the problems of SiPM noise. Therefore, this technology provides a very promising solution for future SiPM-based detectors for space exploration.</p></div>","PeriodicalId":774,"journal":{"name":"Science China Physics, Mechanics & Astronomy","volume":"69 6","pages":""},"PeriodicalIF":7.5000,"publicationDate":"2026-04-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Science China Physics, Mechanics & Astronomy","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s11433-026-2954-2","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
SiPM-based gamma-ray detector has been increasingly utilized in space telescopes. However, its performance in the space environment would be significantly degraded, especially in the low-energy band, owing to the radiation-induced noise increase of SiPM. To address this problem, we have developed and implemented a novel coincidence readout design for SiPM-based detectors of the Gamma-ray Transient Monitor (GTM) onboard the DRO-A satellite (i.e., DRO/GTM). In this paper, we report the first in-flight observation results of DRO/GTM, focusing on the validation and performance studies of the coincidence readout technology, after a brief introduction of the working mode and data type of coincidence readout. We find that GTM detectors can correctly process and label coincidence events, identify the noise signals of SiPM, and safeguard the detection sensitivity of DRO/GTM especially in the low energy band, which is critically important for scientific observations in multi-messenger astronomy era. Our results not only validate the novel design of the coincident readout of DRO/GTM but also showcase its great advantages in mitigating the problems of SiPM noise. Therefore, this technology provides a very promising solution for future SiPM-based detectors for space exploration.
期刊介绍:
Science China Physics, Mechanics & Astronomy, an academic journal cosponsored by the Chinese Academy of Sciences and the National Natural Science Foundation of China, and published by Science China Press, is committed to publishing high-quality, original results in both basic and applied research.
Science China Physics, Mechanics & Astronomy, is published in both print and electronic forms. It is indexed by Science Citation Index.
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