Dear colleagues, New variable star discovery by the MISAO Project (MisV1140). MisV1140 R.A. 22h39m58s.95 Decl. +47o20'16".4 (2000.0) Mag. 13.0-15.2C Type S? = GSC 3624-01696 22h39m58s.91 +47o20'16".2 Error:0.4" Mag:13.04 MagError:0.38 Band:1 Class:3 Plate:00VR Flag:F Epoch:04 SEP 1983 = USNO-A2.0 1350.17102713 22h39m59s.066 +47o20'17".60 Mag(R):12.5 Mag(B):13.3 http://vsnet.aerith.net/misao/data/MisV/MisV1140.gif MisV1140 19990821.75844 13.40C Mis KAF-1600 - KenIchi_Kadota MisV1140 19990821.75887 13.35C Mis KAF-1600 - KenIchi_Kadota MisV1140 20000804.61115 13.14C Mis KAF-1600 - Nobuo_Ohkura MisV1140 20000804.61300 12.96C Mis KAF-1600 - Nobuo_Ohkura MisV1140 20000804.61485 13.00C Mis KAF-1600 - Nobuo_Ohkura MisV1140 20000917.53855 13.13C Mis KAF-1600 - Nobuo_Ohkura MisV1140 20000917.54040 13.17C Mis KAF-1600 - Nobuo_Ohkura MisV1140 20001010.50608 14.95C Mis KAF-1600 - Nobuo_Ohkura MisV1140 20001010.50793 15.18C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, MISAO Project, discovered a new variable star MisV1140. 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/