V2276 Sgr
R. Stubbings reported on August 4 that the dwarf nova V2276 Sgr was in
outburst (14.8mag). The last reported outburst dates back to 1998, suggesting
a low frequency of outbursts. Judging from the outburst amplitude,
the object may be a short-period system such as an SU UMa-type star (vsnet-campaign-dn
2696). H. Yamaoka performed astrometry using images taken by D. Nogami
at Hida observatory: The object was about 16.0CR on Aug 5.5. V2276 Sgr
is identified with a GSC star (r=15.64 b=19.40) and a USNO star (r=18.2
b=19.0) (vsnet-campaign-dn
2702).