Dear colleagues, New variable star discovery by the MISAO Project (MisV1058). MisV1058 R.A. 01h27m43s.47 Decl. +55o30'34".4 (2000.0) Mag. 12.9-14.2C Type SR: = IRAS 01245+5515 01h27m43s.9 +55o30'33" Ellipse:57x12" P.A.:41 Flux(12):0.8416 Flux(25):<0.2567 Flux(60):<0.4438 Flux(100):<9.282 http://vsnet.aerith.net/misao/data/MisV/MisV1058.gif MisV1058 19990928.70740 13.18C Mis KAF-1600 - KenIchi_Kadota MisV1058 19991105.67695 13.42C Mis KAF-1600 - KenIchi_Kadota MisV1058 19991105.67738 13.48C Mis KAF-1600 - KenIchi_Kadota MisV1058 20000130.50455 14.18C Mis KAF-1600 - KenIchi_Kadota MisV1058 20000130.50561 14.14C Mis KAF-1600 - KenIchi_Kadota MisV1058 20000829.63888 12.93C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1058. 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/