The detection of radio emission from known X-ray flaring star EXO 040830−7134.7

This is the radio light curve of known X-ray flaring star EXO 040830−7134.7 observed by MeerKAT as part of ThunderKAT. These data are part of a publication in the Monthly Notice of the Royal Astronomical Society (Driessen et al., Accepted 2021 November 25. Received 2021 November 25; in original form 2021 August 25). The light curve is from the full-time-integration, full-frequency-integration images of VW Hyi, as processed by the LOFAR Transients Pipeline (TraP). The columns in the file are: mjd: the modified Julian Date (MJD) of the observation. The MJD is given by MJD=JD-2400000.5 where JD is the Julian Date f_int_Jy: the integrated flux density of the source in Jansky (Jy) determined by the LOFAR TraP f_int_err_Jy: the uncertainty on f_int_Jy in Jansky determined by the LOFAR TraP freq_eff_Hz: the effect frequency in Hertz (Hz) as determined by the LOFAR TraP taustart_ts: the ISO 8601 time of the observation in Coordinated Universal Time (UTC) The files were made using the Pandas package, so we recommend Python users load them using <pre><code>import pandas as pd pd.read_csv(filename, comment='#')</code></pre> If you use the data shared here please ensure that you cite the MNRAS paper (Driessen at al. 2021) and the Zenodo DOI: 10.5281/zenodo.5084298. The MeerKAT telescope is operated by the South African Radio Astronomy Observatory, which is a facility of the National Research Foundation, an agency of the Department of Science and Innovation.<br> LND acknowledges support from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No 694745).本数据集为MeerKAT望远镜作为ThunderKAT项目的组成部分，对已知X射线耀发星EXO 040830−7134.7开展观测所获得的射电光变曲线。该数据隶属于Driessen等人发表于《皇家天文学会月报》（Monthly Notice of the Royal Astronomical Society，简称MNRAS）的一篇研究论文，该论文于2021年11月25日正式接收，期刊于同日收到投稿稿件，原始投稿版本完成于2021年8月25日。本次公开的光变曲线源自VW Hyi的全时间积分、全频率积分成像结果，经LOFAR瞬变源管道（LOFAR Transients Pipeline，TraP）处理得到。 数据文件各列的含义如下： 1. `mjd`：观测的修正儒略日期（modified Julian Date，MJD），其与儒略日期（Julian Date，JD）的换算关系为`MJD=JD−2400000.5`； 2. `f_int_Jy`：由LOFAR TraP测定的源积分流量密度，单位为央斯基（Jansky，Jy）； 3. `f_int_err_Jy`：LOFAR TraP测定的`f_int_Jy`的测量不确定度，单位为央斯基； 4. `freq_eff_Hz`：LOFAR TraP测定的有效观测频率，单位为赫兹（Hertz，Hz）； 5. `taustart_ts`：协调世界时（Coordinated Universal Time，UTC）下的ISO 8601格式观测时刻。 本数据集文件采用Pandas包生成，因此推荐Python用户通过以下代码加载数据： python import pandas as pd pd.read_csv(filename, comment='#') 若使用本数据集，请务必引用该MNRAS论文（Driessen等，2021）以及Zenodo平台的DOI：10.5281/zenodo.5084298。 MeerKAT望远镜由南非射电天文台（South African Radio Astronomy Observatory）运营，该机构隶属于南非科学与创新部下属的国家研究基金会（National Research Foundation）。 LND感谢欧洲研究理事会（European Research Council，ERC）在欧盟“地平线2020”研究与创新框架计划下提供的资助（资助协议编号：694745）。