Confirmation of variability of NSV15510 (Takamizawa) Kesao Takamizawa (Nagano, Japan) reports the detection of a variable star, which has been identifed with NSV15510. The variability is confirmed. NSV15510 = GSC3687.1863 022750.48 +534639.3 (2000.0) 12.93 1 = USNO1425.03524116 022750.484 +534639.34 (2000.0) 11.4 14.4 = IRAS02243+5333 022422.3 +533308 (1950.0) F12=2.29 F25=1.00 F60=0.40L F100=1.20L VAR= 5 LRS=-1 possibly II: variable star with 'young' O-rich circumstellar shell or VII: variable star with more evolved C-rich circumstellar shell = 022750.0 +534633 (2000.0) IRAS02243+5333 2.237 0.968 0.400L 1.209L 5% = 022750.0 +534633 (2000.0) SSC02243+5333 2.237 0.968 0.400L 1.209L = 022750.4 +534639 (2000.0) NSV15510 LB: 12.5 12.8 V - - - - The star may be a semiregular variable with a range of 12.4-13.1p. Photographic magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code NSV15510 19950127.424 126p Tmz.VSOLJ NSV15510 19960922.666 127p Tmz.VSOLJ NSV15510 19970613.728 127p Tmz.VSOLJ NSV15510 19980116.413 131p Tmz.VSOLJ NSV15510 19980629.701 129p Tmz.VSOLJ NSV15510 19991128.448 128p Tmz.VSOLJ NSV15510 20000902.678 124p Tmz.VSOLJ NSV15510 20011023.605 127p Tmz.VSOLJ Observer's code: Tmz: K.Takamizawa (Saku-machi,Nagano,Japan) SASS (Saku All Sky Survey) Inst.: 10cmR F4 twin patrol cameras and 25cm F2.8 Baker-Schmidt camera T-Max400 120 Comparison stars mag.:GSC Relayed from Kesao Takamizawa <k-takamizawa@nifty.ne.jp>