Dear colleagues, New variable star discovery by the MISAO Project (MisV1096). MisV1096 R.A. 00h56m44s.22 Decl. +41o29'23".1 (2000.0) Mag. 13.4-14.3C Type S = GSC 2806-01699 00h56m44s.27 +41o29'23".0 Error:0.2" Mag:13.65 MagError:0.41 Band:6 Class:0 Plate:02RY Flag:F Epoch:04 AUG 1984 = USNO-A2.0 1275.00565192 00h56m44s.252 +41o29'23".08 Mag(R):13.3 Mag(B):14.4 http://vsnet.aerith.net/misao/data/MisV/MisV1096.gif MisV1096 20000906.65366 14.08C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000906.65551 14.08C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000917.63931 13.57C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000917.64116 13.50C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000917.64301 13.56C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000919.64003 13.60C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000919.64188 13.43C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000920.63516 13.50C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000920.63701 13.37C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000924.63747 13.49C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000924.63932 13.41C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000926.61856 14.28C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000926.62042 14.16C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000927.65156 13.65C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20000927.65341 13.54C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001004.61989 14.08C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001004.62174 14.10C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001010.60919 13.67C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001010.61105 13.59C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001010.61290 13.56C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001011.61173 13.79C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001011.61359 14.03C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001106.52450 13.66C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001106.52635 13.53C Mis KAF-1600 - Nobuo_Ohkura MisV1096 20001106.52820 13.71C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, MISAO Project, discovered a new variable star MisV1096. 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, 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/