Dear colleagues, New variable star discovery by the MISAO Project (MisV1048). MisV1048 R.A. 19h59m45s.93 Decl. +42o20'32".7 (2000.0) Mag. 12.3-12.8C Type SR? = USNO-A2.0 1275.13017737 19h59m45s.907 +42o20'32".37 Mag(R):13.9 Mag(B):16.7 = 2MASS 195945.926 +422032.13 (2000.0) 9.434 8.421 8.027 http://vsnet.aerith.net/misao/data/MisV/MisV1048.gif MisV1048 19990430.68636 12.76C Mis KAF-1600 - KenIchi_Kadota MisV1048 19990430.68679 12.70C Mis KAF-1600 - KenIchi_Kadota MisV1048 19990724.58430 12.76C Mis KAF-1600 - KenIchi_Kadota MisV1048 19990724.58475 12.84C Mis KAF-1600 - KenIchi_Kadota MisV1048 20000907.46204 12.31C Mis KAF-1600 - Nobuo_Ohkura MisV1048 20000907.46389 12.34C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1048. It was picked up by Seiichih 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/