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The TAMA group and the ROG group share the joint goal of observing gravitational radiation as an astrophysical probe.
This agreement is intended to establish and define the exchange of data collected by the TAMA interferometric detector and the bar detectors Explorer and Nautilus in the year 2001, when these detectors had simultaneous periods of observation.
The goal is to search for coincidences due to transient g.w. signals with components at kHz frequency, such as those predicted from different kind of sources involving compact object, like stellar gravit. collapses and the last stable orbits of inspiraling neutron stars or black holes binary system, its merging and its final ringdown