Dear colleagues, New variable star discovery by the MISAO Project (MisV1090). MisV1090 R.A. 19h51m51s.23 Decl. +35o55'57".4 (2000.0) Mag. 13.0-13.5C Type ? = USNO-A2.0 1200.13535959 19h51m51s.191 +35o55'57".31 Mag(R):14.7 Mag(B):17.2 = 2MASS 195151.206 +355557.19 (2000.0) 9.599 8.578 8.154 http://vsnet.aerith.net/misao/data/MisV/MisV1090.gif MisV1090 19990803.64247 13.52C Mis KAF-1600 - KenIchi_Kadota MisV1090 19990803.64291 13.48C Mis KAF-1600 - KenIchi_Kadota MisV1090 20000920.43264 12.97C Mis KAF-1600 - Nobuo_Ohkura MisV1090 20000920.43451 13.07C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1090. 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/