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We present results of the search for coincident burst excitations over a 24hours long data set collected by AURIGA, EXPLORER, NAUTILUS and Virgo detectorsduring September 2005. The search of candidate triggers was performedindependently on each of the data sets from single detectors. We looked fortwo-fold time coincidences between these candidates using an algorithmoptimized for a given population of sources and we calculated the efficiency ofdetection through injections of templated signal waveforms into the streams ofdata. To this purpose we have considered the case of signals shaped as dampedsinusoids coming from the galactic center direction. In this framework ourmethod targets an optimal balance between high efficiency and low false alarmrate, aiming at setting confidence intervals as stringent as possible in termsof the rate of the selected source models.

First joint Gravitational Waves search by the Auriga-Explorer-Nautilus-Virgo collaboration