A Heliocentric-orbiting Objects Processing System (HOPS) for the Wide Field Survey Telescope: Architecture, Processing Workflow, and Preliminary Results

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Main Authors: Wang, Shao-Han, Fu, Bing-Xue, Lu, Jun-Qiang, Fan, LuLu, Cai, Min-Xuan, Xu, Ze-Lin, Kong, Xu, Zhao, Haibin, Li, Bin, Liu, Ya-Ting, Zhu, Qing-feng, Zhou, Xu, Wan, Zhen, Cheng, Jingquan, Jiang, Ji-an, Li, Feng, Liang, Ming, Liu, Hao, Luo, Wentao, Lou, Zhen, Wang, Hairen, Wang, Jian, Wang, Tinggui, Xue, Yongquan, Zhang, Hongfei, Zhao, Wen
Format: Preprint
Published: 2025
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_version_ 1866916587969183744
author Wang, Shao-Han
Fu, Bing-Xue
Lu, Jun-Qiang
Fan, LuLu
Cai, Min-Xuan
Xu, Ze-Lin
Kong, Xu
Zhao, Haibin
Li, Bin
Liu, Ya-Ting
Zhu, Qing-feng
Zhou, Xu
Wan, Zhen
Cheng, Jingquan
Jiang, Ji-an
Li, Feng
Liang, Ming
Liu, Hao
Luo, Wentao
Lou, Zhen
Wang, Hairen
Wang, Jian
Wang, Tinggui
Xue, Yongquan
Zhang, Hongfei
Zhao, Wen
author_facet Wang, Shao-Han
Fu, Bing-Xue
Lu, Jun-Qiang
Fan, LuLu
Cai, Min-Xuan
Xu, Ze-Lin
Kong, Xu
Zhao, Haibin
Li, Bin
Liu, Ya-Ting
Zhu, Qing-feng
Zhou, Xu
Wan, Zhen
Cheng, Jingquan
Jiang, Ji-an
Li, Feng
Liang, Ming
Liu, Hao
Luo, Wentao
Lou, Zhen
Wang, Hairen
Wang, Jian
Wang, Tinggui
Xue, Yongquan
Zhang, Hongfei
Zhao, Wen
contents Wide-field surveys have markedly enhanced the discovery and study of solar system objects (SSOs). The 2.5-meter Wide Field Survey Telescope (WFST) represents the foremost facility dedicated to optical time-domain surveys in the northern hemisphere. To fully exploit WFST's capabilities for SSO detection, we have developed a heliocentric-orbiting objects processing system (HOPS) tailored for identifying these objects. This system integrates HelioLinC3D, an algorithm well suited for the WFST survey cadence, characterized by revisiting the same sky field twice on the majority of nights. In this paper, we outline the architecture and processing flow of our SSO processing system. The application of the system to the WFST pilot survey data collected between March and May 2024 demonstrates exceptional performance in terms of both temporal efficiency and completeness. A total of 658,489 observations encompassing 38,520 known asteroids have been documented, and 241 newly discovered asteroids have been assigned provisional designations. In particular, 27% of these new discoveries were achieved using merely two observations per night on three nights. The preliminary results not only illuminate the effectiveness of integrating HelioLinC3D within the SSO processing system, but also emphasize the considerable potential contributions of WFST to the field of solar system science.
format Preprint
id arxiv_https___arxiv_org_abs_2501_17472
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle A Heliocentric-orbiting Objects Processing System (HOPS) for the Wide Field Survey Telescope: Architecture, Processing Workflow, and Preliminary Results
Wang, Shao-Han
Fu, Bing-Xue
Lu, Jun-Qiang
Fan, LuLu
Cai, Min-Xuan
Xu, Ze-Lin
Kong, Xu
Zhao, Haibin
Li, Bin
Liu, Ya-Ting
Zhu, Qing-feng
Zhou, Xu
Wan, Zhen
Cheng, Jingquan
Jiang, Ji-an
Li, Feng
Liang, Ming
Liu, Hao
Luo, Wentao
Lou, Zhen
Wang, Hairen
Wang, Jian
Wang, Tinggui
Xue, Yongquan
Zhang, Hongfei
Zhao, Wen
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Wide-field surveys have markedly enhanced the discovery and study of solar system objects (SSOs). The 2.5-meter Wide Field Survey Telescope (WFST) represents the foremost facility dedicated to optical time-domain surveys in the northern hemisphere. To fully exploit WFST's capabilities for SSO detection, we have developed a heliocentric-orbiting objects processing system (HOPS) tailored for identifying these objects. This system integrates HelioLinC3D, an algorithm well suited for the WFST survey cadence, characterized by revisiting the same sky field twice on the majority of nights. In this paper, we outline the architecture and processing flow of our SSO processing system. The application of the system to the WFST pilot survey data collected between March and May 2024 demonstrates exceptional performance in terms of both temporal efficiency and completeness. A total of 658,489 observations encompassing 38,520 known asteroids have been documented, and 241 newly discovered asteroids have been assigned provisional designations. In particular, 27% of these new discoveries were achieved using merely two observations per night on three nights. The preliminary results not only illuminate the effectiveness of integrating HelioLinC3D within the SSO processing system, but also emphasize the considerable potential contributions of WFST to the field of solar system science.
title A Heliocentric-orbiting Objects Processing System (HOPS) for the Wide Field Survey Telescope: Architecture, Processing Workflow, and Preliminary Results
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
url https://arxiv.org/abs/2501.17472