Dear colleagues, New variable star discovery by the MISAO Project (MisV0957). MisV0957 R.A. 18h29m09s.32 Decl. +04o51'17".6 (2000.0) Mag. 12.3C-13.5C Type SR? = USNO-A2.0_0900.12959112 18 29 09.321 +04 51 17.63 13.6R 16.9B = IRAS 18266+0449 R.A.=18 29 08.91 Decl.=+04 51 14.8 (22 x 5", p.a.=84) flux(12)=1.93 flux(25)=0.86 flux(60)=<0.45 flux(100)=<16.28 21% variable http://vsnet.aerith.net/misao/data/MisV/MisV0957.gif MisV0957 19990605.65144 130C Mis image="KenIchi Kadota" MisV0957 19990605.65189 129C Mis image="KenIchi Kadota" MisV0957 19990831.61456 135C Mis image="KenIchi Kadota" MisV0957 20000523.59351 123C Mis image="Nobuo Ohkura" MisV0957 20000523.59536 123C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0957. It was picked up by Yoshida from the candidates of new variable stars detected by the PIXY system from images taken by Ohkura comparing with images taken by Kadota. Kadota and Yoshida judged it as a real variable star. The magnitude are measured automatically by the PIXY system. Image observers' names are noted after "Mis". Please see the URL below for the MISAO Project and the PIXY system. http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/