Piggyback search for fast radio bursts using Nanshan 26 m and Kunming 40 m radio telescopes - I. Observing and data analysis systems, discovery of a mysterious peryton
文献类型：期刊论文
| 作者 | Men, Y. P.1,2; Luo, R.1,2; Chen, M. Z.3 ; Hao, L. F.4; Lee, K. J.1,5; Li, J.3; Li, Z. X.4; Liu, Z. Y.3; Pei, X.3; Wen, Z. G.3
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| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 出版日期 | 2019-09-01 |
| 卷号 | 488期号:3页码:3957-3971 |
| ISSN号 | 0035-8711 |
| 关键词 | methods: data analysis telescopes radio continuum: transients |
| DOI | 10.1093/mnras/stz1931 |
| 产权排序 | 3 |
| 英文摘要 | We present our piggyback search for fast radio bursts using the Nanshan 26 in Radio Telescope and the Kunming 40 in Radio Telescope. The observations are performed in the L band from 1380 to 1700 MHz at Nanshan and the S band from 2170 to 2310 MHz at Kunming. We built the ROACH2-based FFT spectrometer and developed the real-time transient search software. We introduce a new radio interference mitigation technique named zero-DM matched filter and give the formula of the signal-to-noise ratio loss in the transient search. Though we have no positive detection of bursts in about 1600 and 2400 h data at Nanshan and Kunming, respectively, an intriguing peryton was detected at Nanshan, from which hundreds of bursts were recorded. Perytons are terrestrial radio signals that mimic celestial fast radio bursts. They were first reported at Parkes and identified as microwave oven interferences later. The bursts detected at Nanshan show similar frequency swept emission and have double-peaked profiles. They appeared in different sky regions in about tens of minutes observations and the dispersion measure index is not exactly 2, which indicates the terrestrial origin. The peryton differs drastically from the known perytons detected at Parkes, because it appeared in a precise period of p = 1.712 87 +/- 0.000 04 s. Its origin remains unknown. |
| WOS关键词 | HOST GALAXY ; REAL-TIME ; PULSAR ; TRANSIENTS |
| 资助项目 | NSFC[U15311243] ; National Basic Research Program of China, 973 Program[2015CB857101] ; National Basic Research Program of China, 973 Program[XDB23010200] ; National Basic Research Program of China, 973 Program[11690024] ; National Basic Research Program of China, 973 Program[11373011] ; Max-Planck Partner Group ; Tian-ShanChuangXinTuanDui |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | OXFORD UNIV PRESS |
| WOS记录号 | WOS:000485158400072 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/3018]  |
| 专题 | 微波接收机技术实验室 新疆天文台_110米口径全可动射电望远镜（SmART）_110米大口径全可动射电望远镜关键技术研究（973项目）_课题1：大样本射电天体的观测和前沿问题研究 |
| 通讯作者 | Men, Y. P.; Lee, K. J. |
| 作者单位 | 1.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China 2.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China 3.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 4.Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Yunnan, Peoples R China 5.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 6.Peking Univ, Sch Elect Engn & Comp Sci, Beijing 100871, Peoples R China |
| 推荐引用方式 GB/T 7714 | Men, Y. P.,Luo, R.,Chen, M. Z.,et al. Piggyback search for fast radio bursts using Nanshan 26 m and Kunming 40 m radio telescopes - I. Observing and data analysis systems, discovery of a mysterious peryton[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,488(3):3957-3971. |
| APA | Men, Y. P..,Luo, R..,Chen, M. Z..,Hao, L. F..,Lee, K. J..,...&Zhang, C. F..(2019).Piggyback search for fast radio bursts using Nanshan 26 m and Kunming 40 m radio telescopes - I. Observing and data analysis systems, discovery of a mysterious peryton.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,488(3),3957-3971. |
| MLA | Men, Y. P.,et al."Piggyback search for fast radio bursts using Nanshan 26 m and Kunming 40 m radio telescopes - I. Observing and data analysis systems, discovery of a mysterious peryton".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 488.3(2019):3957-3971. |
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来源：新疆天文台
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