Dear colleagues, New variable star discovery by the MISAO Project (MisV1062). MisV1062 R.A. 21h02m23s.83 Decl. +28o14'26".3 (2000.0) Mag. 11.5-12.8C Type SR? = USNO-A2.0 1125.17698049 21h02m23s.759 +28o14'26".01 Mag(R):13.5 Mag(B):14.8 = IRAS 21002+2802 21h02m23s.8 +28o14'31" Ellipse:28x10" P.A.:67 Flux(12):0.6569 Flux(25):0.1990 Flux(60):<0.4000 Flux(100):<1.404 Var:0% = 2MASS 210223.745 +281425.28 (2000.0) 7.506 6.545 6.008 http://vsnet.aerith.net/misao/data/MisV/MisV1062.gif MisV1062 19990724.61528 12.80C Mis KAF-1600 - KenIchi_Kadota MisV1062 19990724.61571 12.73C Mis KAF-1600 - KenIchi_Kadota MisV1062 20000619.65558 11.52C Mis KAF-1600 - Nobuo_Ohkura MisV1062 20000619.65745 11.46C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1062. It was picked up by Seiichi Yoshida from the candidates of new variable stars detected by the PIXY system 2 from images taken by Nobuo Ohkura comparing with images taken by KenIchi Kadota, and confirmed by KenIchi Kadota. The identification is researched by Taichi Kato (Kyoto University), John Greaves (the United Kingdom), and Seiichi Yoshida. The magnitude are measured automatically by the PIXY system 2. About the MISAO Project and the PIXY system 2: http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/