The next outburst was reported by R. Stubbings on February 10 (vsnet-campaign 755). The object was reported to be still bright at 15.0mag on February 11 (vsnet-campaign 756), however, the decline rate became faster with time (vsnet-campaign-dn 492). P. Schmeer reported the object coincides with an USNO-A2.0 star with r=18.4 and b=18.6 (vsnet-campaign-dn 496). T. Vanmunster and the Kyoto team reported no obvious periodic modulation was seen during the outburst (vsnet-campaign-dn 495, vsnet-campaign-dn 507).
Other related articles: vsnet-campaign-dn 491, 494, 495, 498,