  We present the results of a campaign to observe flares on the M dwarf flare
star EV Lacertae over the course of two days in 2001 September, utilizing a
combination of radio continuum, optical photometric and spectroscopic,
ultraviolet spectroscopic, and X-ray spectroscopic observations, to
characterize the multi-wavelength nature of flares from this active, single
late-type star. We find flares in every wavelength region in which we observed.
In the multi-wavelength context, the start of the intense radio flare is
coincident with an impulsive optical U-band flare, to within one minute, and
yet there is no signature of an X-ray response. There are other intervals of
time where optical flaring and UV flaring is occurring, but these cannot be
related to the contemporaneous X-ray flaring: the time-integrated luminosities
do not match the instantaneous X-ray flare luminosity, as one would expect for
the Neupert effect. We investigate the probability of chance occurrences of
flares from disparate wavelength regions producing temporal coincidences, but
find that not all the flare associations can be explained by a superposition of
flares due to a high flaring rate. We caution against making causal
associations of multi-wavelength flares based solely on temporal correlations
for high flaring rate stars like EV Lac.
