Dear colleagues, New variable star discovery by the MISAO Project (MisV1070). MisV1070 R.A. 19h55m34s.14 Decl. +48o32'22".2 (2000.0) Mag. 11.6-12.2C Type ? = USNO-A2.0 1350.11303395 19h55m34s.229 +48o32'22".66 Mag(R):13.6 Mag(B):16.8 = IRAS 19541+4824 19h55m34s.2 +48o32'23" Ellipse:76x15" P.A.:58 Flux(12):0.1868 Flux(25):<0.5465 Flux(60):<0.4510 Flux(100):<3.065 http://vsnet.aerith.net/misao/data/MisV/MisV1070.gif MisV1070 19990724.60209 12.15C Mis KAF-1600 - KenIchi_Kadota MisV1070 19990724.60253 12.15C Mis KAF-1600 - KenIchi_Kadota MisV1070 20001011.40455 11.60C Mis KAF-1600 - Nobuo_Ohkura MisV1070 20001011.40641 11.64C Mis KAF-1600 - Nobuo_Ohkura MisV1070 20001011.40827 11.70C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1070. 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/