Confirmation of variability of MisV0200 (Takamizawa) Kesao Takamizawa (Nagano, Japan) reports the detection of a variable star, which has been identifed with MisV0200. The variability is confirmed. MisV0200 = 2MASS 185910.972 +172703.60 (2000.0) 6.525 5.518 4.868 = IRAS18569+1722 185657.4 +172250 (1950.0) F12=2.75 F25=1.58 F60=0.40L F100=3.63L VAR=98 LRS=-1 possibly IIIa: variable star with more evolved O-rich c.s. shell or VII: variable star with more evolved C-rich circumstellar shell = 185910.9 +172704 (2000.0) MisV0200 11.5 12.5C SR? - - = 185910.8 +172701 (2000.0) IRAS18569+1722 2.769 1.567 0.400L 3.584L 98% = 185910.8 +172701 (2000.0) SSC18569+1722 2.769 1.567 0.400L 3.584L Takamizawa's comment: The star may be a Mira-type variable with a range of 11.4-<14.3p, and a period about 340days. Photographic magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code MisV0200 20000919.481 <143p Tmz.VSOLJ MisV0200 20001019.445 135p Tmz.VSOLJ MisV0200 20001027.424 127p Tmz.VSOLJ MisV0200 20001123.413 123p Tmz.VSOLJ MisV0200 20001213.369 <130p Tmz.VSOLJ MisV0200 20010216.792 <130p Tmz.VSOLJ MisV0200 20010302.779 <130p Tmz.VSOLJ MisV0200 20010318.712 <143p Tmz.VSOLJ MisV0200 20010321.768 <143p Tmz.VSOLJ MisV0200 20010326.763 <143p Tmz.VSOLJ MisV0200 20010331.739 <143p Tmz.VSOLJ MisV0200 20010419.684 <143p Tmz.VSOLJ MisV0200 20010426.677 <143p Tmz.VSOLJ MisV0200 20010512.588 <143p Tmz.VSOLJ MisV0200 20010516.634 <143p Tmz.VSOLJ MisV0200 20010525.638 <143p Tmz.VSOLJ MisV0200 20010611.523 <143p Tmz.VSOLJ MisV0200 20010620.619 <143p Tmz.VSOLJ MisV0200 20010701.613 <130p Tmz.VSOLJ MisV0200 20010720.482 <141p Tmz.VSOLJ MisV0200 20010817.470 <130p Tmz.VSOLJ MisV0200 20010924.477 130p Tmz.VSOLJ MisV0200 20011011.430 118p Tmz.VSOLJ MisV0200 20011019.435 120p Tmz.VSOLJ MisV0200 20011023.399 120p Tmz.VSOLJ MisV0200 20011104.413 114p 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>