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   73001
   We propose observation of three well known, dMe single flare stars,
   spanning a factor of 100 in their quiescent X-ray flux. These
   observations will allow study of 1) the frequency of large and small
   flares, 2) the frequency-intensity relation, specially at the ``bright
   end'', and 3) the (possible) dependence of the flare frequency on
   quiescent X-ray luminosity. Recent observations of very large flares on
   dMe stars show large coronal mass ejections; a determination of the
   frequency of such events is critical for assessing their (possibly
   large) contribution to the chemical equilibrium of the interstellar
   medium. The detailed study of flaring events detected during the
   campaign will allow the sampling of extreme coronal conditions in a way
   not possible in other single stars.
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