SW UMa: brightening and international campaign Our CCD observation has confirmed the further ongoing brightening of SW UMa. The object has become 0.4 mag brighter in these 4 hours. This may reflect the final rise to the peak brightness! We presently use 10 sec exposure time in order to resolve possible super-QPOs. We will undertake an international observing campaign on SW UMa, as we have had a very successful one in DV UMa and IY UMa. Please post timely to vsnet-alert confirmatory observations, new findings, the progress of the outburst and observations. Collaborating observations should be sent (as usual) to uemura@kusastro.kyoto-u.ac.jp. Regards, Makoto Uemura and Taichi Kato