Dear colleagues, New variable star discovery by the MISAO Project (MisV1075). MisV1075 R.A. 20h14m27s.86 Decl. +47o29'45".7 (2000.0) Mag. 11.6-13.9C Type M: = USNO-A2.0 1350.11919677 20h14m27s.820 +47o29'45".46 Mag(R):13.1 Mag(B):15.8 = 2MASS 201427.803 +472945.50 (2000.0) 9.673 8.751 8.135 http://vsnet.aerith.net/misao/data/MisV/MisV1075.gif MisV1075 19990803.69485 11.69C Mis KAF-1600 - KenIchi_Kadota MisV1075 19990803.69528 11.63C Mis KAF-1600 - KenIchi_Kadota MisV1075 20000917.44771 13.91C Mis KAF-1600 - Nobuo_Ohkura MisV1075 20000917.44955 13.92C Mis KAF-1600 - Nobuo_Ohkura MisV1075 20000917.45142 13.82C Mis KAF-1600 - Nobuo_Ohkura MisV1075 20001010.41707 12.62C Mis KAF-1600 - Nobuo_Ohkura MisV1075 20001010.41893 12.69C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1075. 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/