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We present the first dedicated radio continuum survey of a Kepler K2 missionfield, Field 1 covering the North Galactic Cap. The survey is wide field,contemporaneous, multi-epoch, and multi-resolution in nature and was conductedat low radio frequencies between 140 and 200 MHz. The multi-epoch and ultrawide field (but relatively low resolution) part of the survey was provided by15 nights of observation with the Murchison Widefield Array (MWA) over a periodof approximately a month, contemporaneous with K2 observations of the field.The multi-resolution aspect of the survey was provided by the low resolution(4') MWA imaging, complemented by non-contemporaneous but much higherresolution (20") observations using the Giant Metrewave Radio Telescope (GMRT).The survey is therefore sensitive to the details of radio structures across awide range of angular scales. Consistent with other recent low radio frequencysurveys, no significant radio transients or variables were detected in thesurvey. The resulting source catalogs consist of 1,085 and 1,468 detections inthe two MWA observation bands (centered at 154 and 185 MHz, respectively) and7,445 detections in the GMRT observation band (centered at 148 MHz), over 314square degrees. The survey is presented as a significant resource formulti-wavelength investigations of the more than 21,000 target objects in theK2 field. We briefly examine our survey data against K2 target lists for dwarfstar types (stellar types M and L) that have been known to produce radioflares.

A multi-resolution, multi-epoch low radio frequency survey of the Kepler K2 mission Campaign 1 field