Although V630 Cyg has been a relatively well-known program star among variable star observers, this dwarf nova is still a "suspected" SU UMa-type dwarf nova. Some historical records ... max JD mag duration 2437899 15.0 short 37927 13.8 long (15d), probably a superoutburst 37968 14.5 short 38026 14.7 38260 14.6 short 38291 14.1 short 38340 14.8 38583 14.5 I would like to call observers' attention to monitor this star for superoutbursts, in order to confirm the long-suspected classification. Although outbursts of V630 Cyg are not rare, I think this star still deserves to be included in the alert program, especially for alerting superoutbursts. Regards, Taichi Kato