Composite periodogram analysis for low-event-count fast radio burst repeaters

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2025-03-14 DOI:10.1051/0004-6361/202452508
Murthadza Aznam, Zamri Zainal Abidin, Norsiah Hashim, Tomotsugu Goto, Tetsuya Hashimoto, Muhammad Hassan Zakie, Matdhesh Kummar Jayaganthan
{"title":"Composite periodogram analysis for low-event-count fast radio burst repeaters","authors":"Murthadza Aznam, Zamri Zainal Abidin, Norsiah Hashim, Tomotsugu Goto, Tetsuya Hashimoto, Muhammad Hassan Zakie, Matdhesh Kummar Jayaganthan","doi":"10.1051/0004-6361/202452508","DOIUrl":null,"url":null,"abstract":"<i>Context.<i/> Fast radio bursts (FRBs) are a class of transients characterised by their millisecond-scale duration and relatively high dispersion measures. Some FRBs have been observed to repeat. For such repeating FRBs, measuring the period is key to identifying their physical mechanisms. However, periods have only been measured for two FRBs – FRB 20112002A and FRB 20180916B – because most repeating FRBs have a low event count, making it challenging to measure their periods.<i>Aims.<i/> We aim to introduce a composite periodogram strategy designed to measure periods of repeating FRBs out of low event counts.<i>Methods.<i/> We combined the χ<sup>2<sup/> periodogram with the inactivity fraction periodogram (<i>F<i/><sub>0<sub/>) to maximise the detection likelihood and minimise noise. Our approach was validated using FRB 20180916B, whereby we successfully recovered the known period with as few as five events. We then applied this method to 17 FRBs whose event counts range from three to 12.<i>Results.<i/> A candidate period is identified in FRB 20190804E, FRB 20190915D, FRB 20200223B, FRB 20201130A, and FRB 20201221B, with a probability of chance coincidence ≤0.050. Additionally, we did further checks to eliminate false positives and concluded that the candidate periods for FRB 20190804E (168.39<sub>−0.07<sub/><sup>+3.86<sup/> days) and FRB 20201130A (11.38<sub>−0.10<sub/><sup>+0.10<sup/> days) are likely close to its true period. These values provide a basis for informed follow-up observations.","PeriodicalId":8571,"journal":{"name":"Astronomy & Astrophysics","volume":"104 1","pages":""},"PeriodicalIF":5.8000,"publicationDate":"2025-03-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1051/0004-6361/202452508","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

Context. Fast radio bursts (FRBs) are a class of transients characterised by their millisecond-scale duration and relatively high dispersion measures. Some FRBs have been observed to repeat. For such repeating FRBs, measuring the period is key to identifying their physical mechanisms. However, periods have only been measured for two FRBs – FRB 20112002A and FRB 20180916B – because most repeating FRBs have a low event count, making it challenging to measure their periods.Aims. We aim to introduce a composite periodogram strategy designed to measure periods of repeating FRBs out of low event counts.Methods. We combined the χ2 periodogram with the inactivity fraction periodogram (F0) to maximise the detection likelihood and minimise noise. Our approach was validated using FRB 20180916B, whereby we successfully recovered the known period with as few as five events. We then applied this method to 17 FRBs whose event counts range from three to 12.Results. A candidate period is identified in FRB 20190804E, FRB 20190915D, FRB 20200223B, FRB 20201130A, and FRB 20201221B, with a probability of chance coincidence ≤0.050. Additionally, we did further checks to eliminate false positives and concluded that the candidate periods for FRB 20190804E (168.39−0.07+3.86 days) and FRB 20201130A (11.38−0.10+0.10 days) are likely close to its true period. These values provide a basis for informed follow-up observations.
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
低事件数快速射电突发中继器的复合周期图分析
上下文。快速射电暴(frb)是一类瞬变现象,其特征是毫秒级持续时间和相对较高的色散测量。一些快速射电暴已经被观察到重复。对于这种重复的快速射电暴,测量周期是确定其物理机制的关键。然而,只有两个快速射电暴(FRB 20112002A和FRB 20180916B)的周期被测量到,因为大多数重复的快速射电暴的事件计数很低,这使得测量它们的周期具有挑战性。我们的目标是引入一种复合周期图策略,旨在测量低事件计数中重复快速射电暴的周期。我们将χ2周期图与不活动分数周期图(F0)结合起来,以最大化检测可能性并最小化噪声。使用FRB 20180916B验证了我们的方法,由此我们成功地恢复了只有五个事件的已知周期。然后,我们将该方法应用于17个frb,其事件计数范围为3到12。在FRB 20190804E、FRB 20190915D、FRB 20200223B、FRB 20201130A和FRB 20201221B中确定了候选周期,其机会重合概率≤0.050。此外,我们做了进一步的检查以消除假阳性,并得出结论,FRB 20190804E(168.39−0.07+3.86天)和FRB 20201130A(11.38−0.10+0.10天)的候选周期可能接近其真实周期。这些值为后续观察提供了依据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
期刊最新文献
More power on large scales Exploring the origins of high-velocity features in SNe Ia with the spectral synthesis code TARDIS Lyman continuum escaping from in situ formed stars in a tidal bridge at z = 3 Data-driven magnetohydrodynamic simulation of the initiation of a coronal mass ejection with multiple stages eROSITA selection of new period-bounce cataclysmic variables
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1