Dear colleagues, New variable star discovery by the MISAO Project (MisV1085). MisV1085 R.A. 21h08m42s.91 Decl. +47o19'59".0 (2000.0) Mag. 10.7-11.4C Type SR: = USNO-A2.0 1350.13528832 21h08m42s.994 +47o19'59".38 Mag(R):12.8 Mag(B):17.2 = IRAS 21069+4707 21h08m44s.3 +47o20'09" Ellipse:23x7" P.A.:48 Flux(12):1.029 Flux(25):0.3768 Flux(60):<1.964 Flux(100):7.251 Var:0% = 2MASS 210842.914 +471959.17 (2000.0) 6.532 5.480 4.984 http://vsnet.aerith.net/misao/data/MisV/MisV1085.gif MisV1085 19991121.51011 11.26C Mis KAF-1600 - KenIchi_Kadota MisV1085 19991121.51125 11.32C Mis KAF-1600 - KenIchi_Kadota MisV1085 20000804.55550 11.38C Mis KAF-1600 - Nobuo_Ohkura MisV1085 20000804.55737 11.30C Mis KAF-1600 - Nobuo_Ohkura MisV1085 20000804.55922 11.33C Mis KAF-1600 - Nobuo_Ohkura MisV1085 20000917.48108 10.95C Mis KAF-1600 - Nobuo_Ohkura MisV1085 20000917.48292 10.97C Mis KAF-1600 - Nobuo_Ohkura MisV1085 20000917.48479 10.97C Mis KAF-1600 - Nobuo_Ohkura MisV1085 20001010.45046 10.75C Mis KAF-1600 - Nobuo_Ohkura MisV1085 20001010.45231 10.72C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1085. 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/