Dear colleagues, New variable star discovery by the MISAO Project (MisV1118). MisV1118 R.A. 21h10m14s.49 Decl. +44o03'00".5 (2000.0) Mag. 12.3-14.5C Type M? = 2MASS 211014.484 +440300.13 (2000.0) 9.182 8.115 7.450 http://vsnet.aerith.net/misao/data/MisV/MisV1118.gif MisV1118 19991121.50663 12.37C Mis KAF-1600 - KenIchi_Kadota MisV1118 19991121.50704 12.34C Mis KAF-1600 - KenIchi_Kadota MisV1118 20000905.49636 14.53C Mis KAF-1600 - Nobuo_Ohkura MisV1118 20000905.49822 14.51C Mis KAF-1600 - Nobuo_Ohkura MisV1118 20001001.47776 14.27C Mis KAF-1600 - Nobuo_Ohkura MisV1118 20001001.47961 14.02C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1118. 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/