Dear colleagues, We updated VSNET light curve of SW UMa including the data till Feb. 26 observed by the SW UMa collaboration team. We can see in the light curve that SW UMa on Feb. 26 was a little brighter than the brightness expected from monotonous decline rate. This may tell us that the end of superoutburst will come soon. We are now having a run on SW UMa, which is still in bright state. The follow-up observations are strongly encouraged. The light curve can be seen at: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/swuma00.html Regards, Makoto Uemura on behalf of SW UMa collaboration team