Studying the radiation characteristics of rotating radio transient J1913+1330 with FAST

doi:10.1093/mnras/stad3402

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	Studying the radiation characteristics of rotating radio transient J1913+1330 with FAST
	Zhong, Wenqian 1,2; Zhi, Qijun 1,2; Lu, Jiguang 3,4; Dang, Shijun1,2 ; Bai, Juntao5,6 ; Tian, Jie 1,2; Xu, Xin 1,2; Shang, Lunhua 1,2; Zhang, Dandan 1,2; Dong, Aijun 1,2; Zhao, Rushuang 1,2; Du, Changrong 1,2; Yuen, Rai5
	2024-01
Source Publication	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN	0035-8711
Volume	527 Issue:2 Pages:4129-4139
Contribution Rank	5
Abstract	We report a high-resolution study of the radio radiation properties of RRAT J1913 + 1330 based on data obtained from three observing epochs over 4 months using the Five-hundred-meter Aperture Spherical Radio telescope (FAST). Segments of bursts and nulls are detected from the RRAT, which are in agreement with earlier results. From our observations, we identify nine burst segments, and the pulse profile is different for burst segments. We obtain polarization profile for the RRAT J1913 + 1330, and study the polarization, energy distribution, and the wait time distribution between pulses for different burst states. The results show that there are significant differences in the polarization profiles and linear polarization position angle (PA) across different burst states. In addition, pulses in the burst states are discontinuous, and there is no short-term correlation of the arrival time of single pulses in our observations. More interestingly, we find that the PA from some single pulses with high linear polarization demonstrates very different characteristics. The unique radiation characteristics of RRAT J1913 + 1330 will provide important clues for studying its radiation mechanism.
Keyword	pulsars RRAT J1913+1330
DOI	10.1093/mnras/stad3402
Indexed By	SCI
Language	英语
WOS Keyword	PULSAR POLARIZATION FLUCTUATIONS ; SINGLE-PULSE ; EMISSION PROPERTIES ; LONG-TERM ; POLARIMETRY ; UNIVERSE ; SEARCH ; MHZ
Funding Project	National SKA Program of China ; National Natural Science Foundation of China ; Natural Science and Technology Foundation of Guizhou Province ; Foundation of Guizhou Provincial Education Department ; Guizhou Provincial Science and Technology Foundation ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Scientific Research Project of the Guizhou Provincial Education[2022SKA0130100] ; Scientific Research Project of the Guizhou Provincial Education[2022SKA0130104] ; Academic New Seedling Fund Project of Guizhou Normal University[12273008] ; Academic New Seedling Fund Project of Guizhou Normal University[KY (2020) 003] ; National college student innovation training programme[12003047] ; National Natural Science Foundation of China[[2023]024] ; Foundation of Science and Technology of Guizhou Province[ZK[2022]304] ; Foundation of Guizhou Provincial Education Department[2022A03013-4] ; National SKA Program of China[KY(2022)132] ; National SKA Program of China[KY(2022)137] ; National SKA Program of China[KY[2022]132] ; National SKA Program of China[[2022]B18] ; National Key Program for Science and Technology Research and Development[KY[2022]137] ; National Natural Science Foundation of China (NSFC) project[202210663032] ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region[12103013] ; Open programme of the Key Laboratory of Xinjiang Uygur Autonomous Region[(2021)023] ; [KY(2021)303] ; [KY(2020)003] ; [KY(2023)059] ; [2020SKA0120200] ; [2022YFC2205201] ; [12041303] ; [12041304] ; [12288102] ; [2022A03013] ; [2020D04049]
WOS Research Area	Astronomy & Astrophysics
WOS Subject	Astronomy & Astrophysics
WOS ID	WOS:001127751100006
Publisher	OXFORD UNIV PRESS
Funding Organization	National SKA Program of China ; National Natural Science Foundation of China ; Natural Science and Technology Foundation of Guizhou Province ; Foundation of Guizhou Provincial Education Department ; Guizhou Provincial Science and Technology Foundation ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Scientific Research Project of the Guizhou Provincial Education ; Academic New Seedling Fund Project of Guizhou Normal University ; National college student innovation training programme ; National Natural Science Foundation of China ; Foundation of Science and Technology of Guizhou Province ; Foundation of Guizhou Provincial Education Department ; National SKA Program of China ; National Key Program for Science and Technology Research and Development ; National Natural Science Foundation of China (NSFC) project ; Major Science and Technology Program of Xinjiang Uygur Autonomous Region ; Open programme of the Key Laboratory of Xinjiang Uygur Autonomous Region
Citation statistics	Cited Times:3[WOS] [WOS Record] [Related Records in WOS]
Document Type	期刊论文
Identifier	http://ir.xao.ac.cn/handle/45760611-7/5747
Collection	射电天文研究室_脉冲星研究团组科研仪器设备产出_我台利用FAST观测数据文章
Corresponding Author	Zhi, Qijun; Lu, Jiguang; Dang, Shijun
Affiliation	1.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China 2.Guizhou Normal Univ, Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Peoples R China 3.Chinese Acad Sci, CAS Key Lab FAST, Natl Astron Observ, Beijing 100101, Peoples R China 4.Chinese Acad Sci, Guizhou Radio Astron Observ, Guiyang 550001, Peoples R China 5.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 6.Univ Chinese Acad Sci, Sch Astron & Space.Sci, Beijing 100049, Peoples R China
Recommended Citation GB/T 7714	Zhong, Wenqian,Zhi, Qijun,Lu, Jiguang,et al. Studying the radiation characteristics of rotating radio transient J1913+1330 with FAST[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,527(2):4129-4139.
APA	Zhong, Wenqian.,Zhi, Qijun.,Lu, Jiguang.,Dang, Shijun.,Bai, Juntao.,...&Yuen, Rai.(2024).Studying the radiation characteristics of rotating radio transient J1913+1330 with FAST.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,527(2),4129-4139.
MLA	Zhong, Wenqian,et al."Studying the radiation characteristics of rotating radio transient J1913+1330 with FAST".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 527.2(2024):4129-4139.

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