Further observations of MisV0200 Katsumi Haseda (Aichi, 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 Haseda's comment: Range 11.3-(13.6p Photographic magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code MisV0200 19970413.785 <136p Had.VSOLJ MisV0200 19980204.834 133p Had.VSOLJ MisV0200 19980302.809 136p Had.VSOLJ MisV0200 19980504.731 <136p Had.VSOLJ MisV0200 19980522.715 <136p Had.VSOLJ MisV0200 19980629.664 <136p Had.VSOLJ MisV0200 19981107.427 <136p Had.VSOLJ MisV0200 19990216.822 136p Had.VSOLJ MisV0200 19990315.805 <136p Had.VSOLJ MisV0200 20010922.501 <136p Had.VSOLJ MisV0200 20011011.460 122p Had.VSOLJ MisV0200 20011106.445 113p Had.VSOLJ Observer's code: Had: K. Haseda (Aichi, Japan) Instruments: 10cm F4.0 twin patrol camera +T-Max400(120)