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Solar radio emission at low frequencies (<1 GHz) can provide valuableinformation on processes driving flares and coronal mass ejections (CMEs).Radio emission has been detected from active M dwarf stars, suggestive of muchhigher levels of activity than previously thought. Observations of active Mdwarfs at low frequencies can provide information on the emission mechanism forhigh energy flares and possible stellar CMEs. Here, we conducted twoobservations with the Australian Square Kilometre Pathfinder Telescope (ASKAP)totalling 26 hours and scheduled to overlap with the Transiting ExoplanetSurvey Satellite (TESS) Sector 36 field, utilising the wide fields of view ofboth telescopes to search for multiple M dwarfs. We detected variable radioemission in Stokes I centered at 888 MHz from four known active M dwarfs. Twoof these sources were also detected with Stokes V circular polarisation. Whenexamining the detected radio emission characteristics, we were not abledistinguish between the models for either electron cyclotron maser orgyrosynchrotron emission. These detections add to the growing number of Mdwarfs observed with variable low frequency emission.

Searching for stellar flares from low mass stars using ASKAP and TESS