The 2.5-meter Wide Field Survey Telescope Real-time Data Processing Pipeline I: From raw data to alert distribution
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arXiv
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| Main Authors: | , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2025
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| _version_ | 1866914273982152704 |
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| author | Cai, Minxuan Xu, Zelin Fan, Lulu Wan, Zhen Liu, Binyang Kong, Xu Hu, Weida Hu, Lei Zhu, Qing-feng Li, Guoliang Lin, Jie Fang, Min Jiang, Ji-an Xue, Yongquan Zhen, Xianzhong Wang, Tinggui |
| author_facet | Cai, Minxuan Xu, Zelin Fan, Lulu Wan, Zhen Liu, Binyang Kong, Xu Hu, Weida Hu, Lei Zhu, Qing-feng Li, Guoliang Lin, Jie Fang, Min Jiang, Ji-an Xue, Yongquan Zhen, Xianzhong Wang, Tinggui |
| contents | The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying facility built jointly by the University of Science and Technology of China (USTC) and the Purple Mountain Observatory (PMO). Since many of its scientific objectives rely on near-real-time data for effective analysis, prompt processing of WFST images is of great significance. To meet this need, we adapted the Rubin Observatory Legacy Survey of Space and Time (LSST) science pipelines to handle the data collected by WFST. This paper presents the complete data processing workflow, from ingestion of raw images to the distribution of alerts, and details the primary data products generated by our pipeline. Researchers using data processed by this pipeline can refer to this document to fully understand the data processing procedures. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_15018 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The 2.5-meter Wide Field Survey Telescope Real-time Data Processing Pipeline I: From raw data to alert distribution Cai, Minxuan Xu, Zelin Fan, Lulu Wan, Zhen Liu, Binyang Kong, Xu Hu, Weida Hu, Lei Zhu, Qing-feng Li, Guoliang Lin, Jie Fang, Min Jiang, Ji-an Xue, Yongquan Zhen, Xianzhong Wang, Tinggui Instrumentation and Methods for Astrophysics The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying facility built jointly by the University of Science and Technology of China (USTC) and the Purple Mountain Observatory (PMO). Since many of its scientific objectives rely on near-real-time data for effective analysis, prompt processing of WFST images is of great significance. To meet this need, we adapted the Rubin Observatory Legacy Survey of Space and Time (LSST) science pipelines to handle the data collected by WFST. This paper presents the complete data processing workflow, from ingestion of raw images to the distribution of alerts, and details the primary data products generated by our pipeline. Researchers using data processed by this pipeline can refer to this document to fully understand the data processing procedures. |
| title | The 2.5-meter Wide Field Survey Telescope Real-time Data Processing Pipeline I: From raw data to alert distribution |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2501.15018 |