Dear colleagues, New variable star discovery by the MISAO Project (MisV1100). MisV1100 R.A. 20h00m13s.14 Decl. +36o03'32".5 (2000.0) Mag. 11.1-11.7C Type SR? = USNO-A2.0 1200.14123144 20h00m13s.080 +36o03'32".59 Mag(R):14.2 Mag(B):17.4 = 2MASS 200013.114 +360332.05 (2000.0) 7.274 6.196 5.733 http://vsnet.aerith.net/misao/data/MisV/MisV1100.gif MisV1100 19990430.69374 11.15C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990430.69417 11.13C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990707.67965 11.39C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990707.68009 11.38C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990801.61065 11.33C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990801.61109 11.32C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990803.65726 11.38C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990803.65770 11.36C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990831.63196 11.35C Mis KAF-1600 - KenIchi_Kadota MisV1100 19990831.63242 11.33C Mis KAF-1600 - KenIchi_Kadota MisV1100 20000920.43636 11.63C Mis KAF-1600 - Nobuo_Ohkura MisV1100 20000920.43821 11.72C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1100. 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/