Dear colleagues, New variable star discovery by the MISAO Project (MisV1117). MisV1117 R.A. 21h10m15s.80 Decl. +43o41'16".4 (2000.0) Mag. 11.9-14.6C Type ? = 2MASS 211015.747 +434115.93 (2000.0) 8.107 6.955 6.232 http://vsnet.aerith.net/misao/data/MisV/MisV1117.gif MisV1117 19991121.50663 14.59C Mis KAF-1600 - KenIchi_Kadota MisV1117 19991121.50704 13.93C Mis KAF-1600 - KenIchi_Kadota MisV1117 20000803.55947 12.19C Mis KAF-1600 - Nobuo_Ohkura MisV1117 20000803.56132 12.23C Mis KAF-1600 - Nobuo_Ohkura MisV1117 20000803.56318 12.27C Mis KAF-1600 - Nobuo_Ohkura MisV1117 20000905.49636 11.93C Mis KAF-1600 - Nobuo_Ohkura MisV1117 20000905.49822 12.02C Mis KAF-1600 - Nobuo_Ohkura MisV1117 20001001.47776 12.18C Mis KAF-1600 - Nobuo_Ohkura MisV1117 20001001.47961 12.20C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1117. 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/