FS Aur VSNET campaign status The Kyoto team has been following FS Aur since the discovery of its potential short-period SU UMa-type nature. The object has been always on the monitoring programs of amateur variable star associations. We have been following the target for past five years in winter seasons (Hajime Baba et al.), including some "outburst" photometry. Very interesting periodicities and "flares" and their relation to the outburst state have been clarified. What is solely lacking: superoutburst. While the present reported magntitude doesn't seem to far exceed the previously recorded maxima, we would be extremely happy to conclude our long-term study of this star, when a genuine superoutburst finally leads to a sparkling campaign by the VSNET collaboration team. Regards, Taichi Kato On behalf of the VSNET FS Aur collaboration team