V730 Sgr again showed another outburst on September 5 (vsnet-campaign-dn 138).
V730 Sgr experienced the other bright outburst as reported by R. Stubbings on September 24 (13.6mag) ( vsnet-campaign 512). T. Kato confirmed the outburst on September 25 (V=13.5) (vsnet-campaign-dn 162). The position calculted by H. Yamaoka using Ouda image is well coincident with a USNO star (r=15.2, b=14.9), and if this USNO star is the quiescent state of V730 Sgr, the amplitude is rather small (vsnet-campaign-dn 165). T. Kato obtained a 40-min time-series on September 25. The light curve showed no detectable variability (vsnet-campaign-dn 166). The fading from this outburst was observed on September 28 (14.1mag by R. Stubbings) (vsnet-campaign-dn 173).