Dear colleagues, New variable star discovery by the MISAO Project (MisV1057). MisV1057 R.A. 01h24m53s.94 Decl. +55o10'44".9 (2000.0) Mag. 10.9-11.9C Type ? = USNO-A2.0 1425.01922496 01h24m53s.900 +55o10'44".87 Mag(R):13.3 Mag(B):17.0 = IRAS 01217+5455 01h24m53s.8 +55o10'44" Ellipse:16x3" P.A.:49 Flux(12):1.234 Flux(25):0.6117 Flux(60):<0.4000 Flux(100):<8.264 Var:14% http://vsnet.aerith.net/misao/data/MisV/MisV1057.gif MisV1057 20000130.50455 10.97C Mis KAF-1600 - KenIchi_Kadota MisV1057 20000130.50561 10.91C Mis KAF-1600 - KenIchi_Kadota MisV1057 20000829.63703 11.81C Mis KAF-1600 - Nobuo_Ohkura MisV1057 20000829.63888 11.81C Mis KAF-1600 - Nobuo_Ohkura MisV1057 20000829.64075 11.85C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1057. 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/