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We present Murchison Widefield Array (MWA) monitoring of the Kepler K2mission Fields 3, 4, and 5 at frequencies of 155 and 186 MHz, from observationscontemporaneous with the K2 observations. This work follows from previous MWAand GMRT surveys of Field 1, with the current work benefiting from a range ofimprovements in the data processing and analysis. We continue to build a bodyof systematic low frequency blind surveys overlapping with transient/variablesurvey fields at other wavelengths, providing multi-wavelength data for objectclasses such as flare stars. From the current work, we detect no variableobjects at a surface density above 2e-4 per square degree, at flux densities of~500 mJy, and observation cadence of days to weeks, representing almost anorder of magnitude decrease in measured upper limits compared to previousresults in this part of observational parameter space. This continues to showthat radio transients at metre and centimetre wavelengths are rare.

Multi-epoch Low Radio Frequency Surveys of the Kepler K2 Mission Campaign Fields 3, 4, and 5 with the Murchison Widefield Array