Survey and Monitoring of ASKAP’s RFI Environment and Trends I: Flagging Statistics

IF 4.5 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Publications of the Astronomical Society of Australia Pub Date : 2024-01-29 DOI:10.1017/pasa.2024.4
L. Lourenço, A. P. Chippendale, B. Indermuehle, V. A. Moss, Tara Murphy, T. J. Galvin, G. Hellbourg, A. W. Hotan, E. Lenc, M. T. Whiting
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Abstract

We present an initial analysis of Radio Frequency Interference (RFI) flagging statistics from archived Australian SKA Pathfinder (ASKAP) observations for the “Survey and Monitoring of ASKAP’s RFI environment and Trends” (SMART) project. SMART is a two-part observatoryled project combining analysis of archived observations with a dedicated, comprehensive RFI survey. The survey component covers ASKAP’s full 700MHz to 1800MHz frequency range, including bands not typically used due to severe RFI. Observations are underway to capture a detailed snapshot of the ASKAP RFI environment over representative 24 h periods. In addition to this dedicated survey, we routinely archive and analyse flagging statistics for all scientific observations to monitor the observatory’s RFI environment in near real-time. We use the telescope itself as a very sensitive RFI monitor and directly assess the fraction of scientific observations impacted by RFI. To this end, flag tables are now automatically ingested and aggregated as part of routine ASKAP operations for all science observations, as a function of frequency and time. The data presented in this paper come from processing all archived data for several ASKAP Survey Science Projects (SSPs). We found that the average amount of flagging due to RFI across the routinely-used ‘clean’ continuum science bands is 3%. The ‘clean’ mid band from 1293MHz to 1437MHz (excluding the 144MHz below 1293MHz impacted by radionavigation-satellites which is discarded before processing) is the least affected by RFI, followed by the ‘clean’ low band from 742MHz to 1085MHz. ASKAP SSPs lose most of their data to the mobile service in the low band, aeronautical service in the mid band and satellite navigation service in the 1510MHz to 1797MHz high band. We also show that for some of these services, the percentage of discarded data has been increasing year-on-year. SMART provides a unique opportunity to study ASKAP’s changing RFI environment, including understanding and updating the default flagging behaviour, inferring the suitability of and calibrating RFI monitoring equipment, monitoring spectrum management compliance in the Australian Radio Quiet Zone –Western Australia (ARQZWA), and informing the implementation of a suite of RFI mitigation techniques.
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对 ASKAP 的 RFI 环境和趋势的调查和监测 I.标记统计
我们为 "澳大利亚SKA探路者(ASKAP)射频干扰环境和趋势调查与监测"(SMART)项目提供了对存档的澳大利亚SKA探路者(ASKAP)观测数据中射频干扰(RFI)标记统计的初步分析。SMART是一个由两个部分组成的观测项目,结合了对存档观测数据的分析和专门、全面的射频干扰调查。调查部分涵盖 ASKAP 的整个 700MHz 至 1800MHz 频率范围,包括由于严重射频干扰而通常不使用的频段。目前正在进行观测,以捕捉具有代表性的 24 小时 ASKAP RFI 环境的详细快照。除了这项专门调查外,我们还对所有科学观测的标记统计数据进行例行存档和分析,以近乎实时地监测天文台的射频干扰环境。我们利用望远镜本身作为非常灵敏的射频干扰监测器,直接评估受射频干扰影响的科学观测的比例。为此,作为 ASKAP 日常操作的一部分,标志表现在会根据频率和时间自动摄取和汇总所有科学观测数据。本文介绍的数据来自对几个 ASKAP 勘测科学项目(SSP)所有存档数据的处理。我们发现,在常规使用的 "干净 "连续谱科学波段中,由于射频识别(RFI)引起的标记平均为3%。从1293MHz到1437MHz的 "干净 "中频段(不包括受无线电导航卫星影响的1293MHz以下的144MHz,该频段在处理前已被丢弃)受射频干扰的影响最小,其次是742MHz到1085MHz的 "干净 "低频段。ASKAP SSP 在低频段的移动服务、中频段的航空服务和 1510MHz 至 1797MHz 高频段的卫星导航服务中丢失了大部分数据。我们还显示,就其中一些服务而言,丢弃数据的比例逐年增加。SMART为研究ASKAP不断变化的射频干扰环境提供了一个独特的机会,包括了解和更新默认标记行为、推断射频干扰监测设备的适用性并进行校准、监测澳大利亚无线电静区-西澳大利亚(ARQZWA)的频谱管理合规性,以及为一套射频干扰缓解技术的实施提供信息。
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来源期刊
Publications of the Astronomical Society of Australia
Publications of the Astronomical Society of Australia 地学天文-天文与天体物理
CiteScore
5.90
自引率
9.50%
发文量
41
审稿时长
>12 weeks
期刊介绍: Publications of the Astronomical Society of Australia (PASA) publishes new and significant research in astronomy and astrophysics. PASA covers a wide range of topics within astronomy, including multi-wavelength observations, theoretical modelling, computational astronomy and visualisation. PASA also maintains its heritage of publishing results on southern hemisphere astronomy and on astronomy with Australian facilities. PASA publishes research papers, review papers and special series on topical issues, making use of expert international reviewers and an experienced Editorial Board. As an electronic-only journal, PASA publishes paper by paper, ensuring a rapid publication rate. There are no page charges. PASA''s Editorial Board approve a certain number of papers per year to be published Open Access without a publication fee.
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