Dear colleagues, New variable star discovery by the MISAO Project (MisV1121). MisV1121 R.A. 21h31m01s.14 Decl. +41o24'07".5 (2000.0) Mag. 11.8-12.3C Type SR? = USNO-A2.0 1275.15883634 21h31m01s.131 +41o24'07".73 Mag(R):15.8 Mag(B):19.6 = IRAS 21290+4110 21h31m01s.7 +41o24'11" Ellipse:29x10" P.A.:53 Flux(12):0.9591 Flux(25):0.3959 Flux(60):<0.4000 Flux(100):<9.265 Var:0% = 2MASS 213101.127 +412407.96 (2000.0) 7.622 6.548 5.968 http://vsnet.aerith.net/misao/data/MisV/MisV1121.gif MisV1121 20000926.47926 11.83C Mis KAF-1600 - Nobuo_Ohkura MisV1121 20000926.48112 11.86C Mis KAF-1600 - Nobuo_Ohkura MisV1121 20000926.48298 11.91C Mis KAF-1600 - Nobuo_Ohkura MisV1121 20001106.39841 12.33C Mis KAF-1600 - Nobuo_Ohkura MisV1121 20001106.40026 12.32C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, MISAO Project, discovered a new variable star MisV1121. 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, 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/