SX LMi: relatively rapid fading? The Kyoto team performed time-series photometry of SX LMi and found that the object faded with the rate of 0.25 mag/day. This is somewhat faster compared with the ordinary superoutburst. In the light curve, we can find a hint of weak double-peaked variations in one orbital (~superhump) period, but they are not conclusive because the short base-line. Tonight observation will also essential to reveal the nature of the current outburst. Regards, Makoto Uemura