Using ASKAP survey light curves and ATCA follow-up, the authors confirm three new magnetospheric radio pulse emitters, demonstrating a variability-based, polarization-free selection method.
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Discovery of Main-sequence Radio Pulse emitters from widefield sky surveys
Using ASKAP survey light curves and ATCA follow-up, the authors confirm three new magnetospheric radio pulse emitters, demonstrating a variability-based, polarization-free selection method.