GRM Scientific Pipeline
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arXiv
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2026
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| _version_ | 1866913064965636096 |
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| author | Wang, Ping Zhang, Li Wang, Jin Yu, Wen-Hui Zhao, Xiao-Yun Zheng, Shi-Jie Xiong, Shao-Lin Huang, Yue He, Jiang Shi, Hao-Li Li, Lu Dong, Yong-Wei Gao, Min Liu, Jiang-Tao Liu, Xin Sun, Jian-Chao Song, Li-Ming Wu, Bo-Bing Wang, Jin-Zhou Wang, Rui-Jie Zhang, Shuang-Nan |
| author_facet | Wang, Ping Zhang, Li Wang, Jin Yu, Wen-Hui Zhao, Xiao-Yun Zheng, Shi-Jie Xiong, Shao-Lin Huang, Yue He, Jiang Shi, Hao-Li Li, Lu Dong, Yong-Wei Gao, Min Liu, Jiang-Tao Liu, Xin Sun, Jian-Chao Song, Li-Ming Wu, Bo-Bing Wang, Jin-Zhou Wang, Rui-Jie Zhang, Shuang-Nan |
| contents | The Gamma-Ray Monitor (GRM) is a key payload of the Space-based multiband astronomical Variable Objects Monitor (SVOM) mission, which is designed to detect gamma ray bursts (GRBs) within the energy range of 15 keV to 5 MeV. The GRM Instrument Center (GRM\_IC) features real-time data processing through the X-band, enabling rapid response of high-energy GRB events. The system employs an event-driven architecture and distributed design, achieving efficient processing and real-time monitoring of massive observational data. Through comprehensive data production processes and scientific data product management, the system achieves efficient production of scientific data products of the L1B / C level through the submission of jobs to the task scheduling system. Through modular architecture design and automated processing workflow, the GRM data processing system realizes precise conversion and scientific analysis of GRB detection data, providing robust technical support for future system upgrades and cross-platform collaboration. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_24267 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | GRM Scientific Pipeline Wang, Ping Zhang, Li Wang, Jin Yu, Wen-Hui Zhao, Xiao-Yun Zheng, Shi-Jie Xiong, Shao-Lin Huang, Yue He, Jiang Shi, Hao-Li Li, Lu Dong, Yong-Wei Gao, Min Liu, Jiang-Tao Liu, Xin Sun, Jian-Chao Song, Li-Ming Wu, Bo-Bing Wang, Jin-Zhou Wang, Rui-Jie Zhang, Shuang-Nan Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena The Gamma-Ray Monitor (GRM) is a key payload of the Space-based multiband astronomical Variable Objects Monitor (SVOM) mission, which is designed to detect gamma ray bursts (GRBs) within the energy range of 15 keV to 5 MeV. The GRM Instrument Center (GRM\_IC) features real-time data processing through the X-band, enabling rapid response of high-energy GRB events. The system employs an event-driven architecture and distributed design, achieving efficient processing and real-time monitoring of massive observational data. Through comprehensive data production processes and scientific data product management, the system achieves efficient production of scientific data products of the L1B / C level through the submission of jobs to the task scheduling system. Through modular architecture design and automated processing workflow, the GRM data processing system realizes precise conversion and scientific analysis of GRB detection data, providing robust technical support for future system upgrades and cross-platform collaboration. |
| title | GRM Scientific Pipeline |
| topic | Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2604.24267 |