Re: V405 Vul = S10943 = RX J1953.1+2115 is new UGSU-type dwarf nova with second-longest superhump period Congratulations, Tonny! Since some high-inclination SS Cyg stars also tend to show orbital modulations at the last stage of outburst (as you may have seen in IP Peg), further confirmation at the early epoch of the next (presumable) superoutburst is extremely important, which may be able to show the growth of superhumps. We should therefore select this star as one of the high-priority VSNET campaign targets, during this outburst and future outbursts. Regards, Taichi Kato VSNET Collaboration team