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).