Commensal Transient Searches in Eight Short Gamma Ray Burst Fields

IF 4.7 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
S. Chastain, A. J. van der Horst, A. Rowlinson, L. Rhodes, A. Andersson, R. Diretse, R. Fender, P. Woudt
{"title":"Commensal Transient Searches in Eight Short Gamma Ray Burst Fields","authors":"S. Chastain, A. J. van der Horst, A. Rowlinson, L. Rhodes, A. Andersson, R. Diretse, R. Fender, P. Woudt","doi":"10.1093/mnras/stad2714","DOIUrl":null,"url":null,"abstract":"\n A new generation of radio telescopes with excellent sensitivity, instantaneous uv coverage, and large fields of view, are providing unprecedented opportunities for performing commensal transient searches. Here we present such a commensal search in deep observations of short gamma-ray burst fields carried out with the MeerKAT radio telescope in South Africa at 1.3 GHz. These four hour observations of eight different fields span survey lengths of weeks to months. We also carry out transient searches in time slices of the full observations, at timescales of 15 minutes, and 8 seconds. We find 122 variable sources on the long timescales, of which 52 are likely active galactic nuclei, but there are likely also some radio flaring stars. While the variability is intrinsic in at least two cases, most of it is consistent with interstellar scintillation. In this study, we also place constraints on transient rates based on state-of-the-art transient simulations codes. We place an upper limit of 2 × 10−4 transients per day per square degree for transients with peak flux of 5 mJy, and an upper limit of 2.5 × 10−2 transients per day per square degree for transients with a fluence of 10 Jy ms, the minimum detectable fluence of our survey.","PeriodicalId":18930,"journal":{"name":"Monthly Notices of the Royal Astronomical Society","volume":" ","pages":""},"PeriodicalIF":4.7000,"publicationDate":"2023-09-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Monthly Notices of the Royal Astronomical Society","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1093/mnras/stad2714","RegionNum":3,"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

A new generation of radio telescopes with excellent sensitivity, instantaneous uv coverage, and large fields of view, are providing unprecedented opportunities for performing commensal transient searches. Here we present such a commensal search in deep observations of short gamma-ray burst fields carried out with the MeerKAT radio telescope in South Africa at 1.3 GHz. These four hour observations of eight different fields span survey lengths of weeks to months. We also carry out transient searches in time slices of the full observations, at timescales of 15 minutes, and 8 seconds. We find 122 variable sources on the long timescales, of which 52 are likely active galactic nuclei, but there are likely also some radio flaring stars. While the variability is intrinsic in at least two cases, most of it is consistent with interstellar scintillation. In this study, we also place constraints on transient rates based on state-of-the-art transient simulations codes. We place an upper limit of 2 × 10−4 transients per day per square degree for transients with peak flux of 5 mJy, and an upper limit of 2.5 × 10−2 transients per day per square degree for transients with a fluence of 10 Jy ms, the minimum detectable fluence of our survey.
八个短伽马暴场的共瞬态搜索
新一代射电望远镜具有卓越的灵敏度、瞬时紫外线覆盖和大视场,为进行共频瞬态搜索提供了前所未有的机会。在这里,我们提出了在南非的MeerKAT射电望远镜进行的1.3 GHz短伽马射线爆发场的深度观测中进行的这种共搜索。这些对八个不同领域的四个小时的观察跨越了几周到几个月的调查时间。我们还在完整观测的时间片段中进行瞬态搜索,时间尺度为15分8秒。我们在长时间尺度上发现了122个可变源,其中52个可能是活跃的星系核,但也可能有一些射电耀斑恒星。虽然这种变化至少在两种情况下是固有的,但大多数情况下与星际闪烁是一致的。在本研究中,我们还基于最先进的暂态模拟代码对暂态速率进行了约束。对于峰值通量为5jy毫秒的瞬态,我们设定了每天每平方度2 × 10−4个瞬态的上限,对于影响为10jy毫秒的瞬态,我们设定了每天每平方度2.5 × 10−2个瞬态的上限,这是我们调查中可检测到的最小影响。
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 求助全文
来源期刊
CiteScore
9.10
自引率
37.50%
发文量
3198
审稿时长
3 months
期刊介绍: Monthly Notices of the Royal Astronomical Society is one of the world''s leading primary research journals in astronomy and astrophysics, as well as one of the longest established. It publishes the results of original research in positional and dynamical astronomy, astrophysics, radio astronomy, cosmology, space research and the design of astronomical instruments.
×
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
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
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 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信