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Design and Application of an S-band Fast Radio Bursts Search Pipeline for the Nanshan 26 m Radio Telescope | |
Liu, Yan-Ling1,2![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() | |
2024-07-01 | |
Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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ISSN | 1674-4527 |
Volume | 24Issue:7Pages:075008 |
Contribution Rank | 1 |
Abstract | Fast radio bursts (FRBs) are among the most studied radio transients in astrophysics, but their origin and radiation mechanism are still unknown. It is a challenge to search for FRB events in a huge amount of observational data with high speed and high accuracy. With the rapid advancement of the FRB research process, FRB searching has changed from archive data mining to either long-term monitoring of the repeating FRBs or all-sky surveys with specialized equipments. Therefore, establishing a highly efficient and high quality FRB search pipeline is the primary task in FRB research. Deep learning techniques provide new ideas for FRB search processing. We have detected radio bursts from FRB 20201124A in the L-band observational data of the Nanshan 26 m radio telescope (NSRT-26m) using the constructed deep learning based search pipeline named dispersed dynamic spectra search (DDSS). Afterwards, we further retrained the deep learning model and applied the DDSS framework to S-band observations. In this paper, we present the FRB observation system and search pipeline using the S-band receiver. We carried out search experiments, and successfully detected the radio bursts from the magnetar SGR J1935+2145 and FRB 20220912A. The experimental results show that the search pipeline can complete the search efficiently and output the search results with high accuracy. |
Keyword | radio continuum: general methods: data analysis methods: observational |
DOI | 10.1088/1674-4527/ad52c5 |
Indexed By | SCI |
Language | 英语 |
Funding Project | Chinese Academy of Sciences (CAS) Light of West China Program[2022-XBQNXZ-015] ; National Natural Science Foundation of China (NSFC)[11903071] ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance (MOF) of China |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:001265237700001 |
Publisher | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
Funding Organization | Chinese Academy of Sciences (CAS) Light of West China Program ; National Natural Science Foundation of China (NSFC) ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance (MOF) of China |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/6840 |
Collection | 射电天文研究室_微波技术实验室 射电天文研究室_脉冲星研究团组 射电天文研究室_数字技术实验室 射电天文研究室_天线技术实验室 科研仪器设备产出_利用南山26米射电望远镜(NSRT)观测数据的文章 |
Corresponding Author | Liu, Yan-Ling |
Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 2.Xinjiang Key Lab Microwave Technol, Urumqi 830011, Peoples R China 3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China |
First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Recommended Citation GB/T 7714 | Liu, Yan-Ling,Chen, Mao-Zheng,Li, Jian,et al. Design and Application of an S-band Fast Radio Bursts Search Pipeline for the Nanshan 26 m Radio Telescope[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2024,24(7):075008. |
APA | Liu, Yan-Ling.,Chen, Mao-Zheng.,Li, Jian.,Yuan, Jian-Ping.,Yuen, Rai.,...&Zhai, Nan-Nan.(2024).Design and Application of an S-band Fast Radio Bursts Search Pipeline for the Nanshan 26 m Radio Telescope.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,24(7),075008. |
MLA | Liu, Yan-Ling,et al."Design and Application of an S-band Fast Radio Bursts Search Pipeline for the Nanshan 26 m Radio Telescope".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 24.7(2024):075008. |
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Liu-2024-Design and (1064KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text |
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