Dear colleagues, New variable star discovery by the MISAO Project (MisV1032). MisV1032 R.A. 20h42m15s.85 Decl. +45o32'50".4 (2000.0) Mag. 10.8C-14.5C Type M? = USNO-A2.0_1350.12776036 20 42 15.853 +45 32 50.41 13.5R 19.6B = IRAS 20405+4521 R.A.=20 42 16.19 Decl.=+45 32 48.0 (7 x 7", p.a.=123) flux(12)=13.73 flux(25)=8.93 flux(60)=<1.85 flux(100)=<17.37 77% variable = 2MASS 204215.816 +453249.67 (2000.0) 5.940 0.000 0.000 http://vsnet.aerith.net/misao/data/MisV/MisV1032.gif MisV1032 19990709.76147 143C Mis image="KenIchi Kadota" MisV1032 19990709.76243 142C Mis image="KenIchi Kadota" MisV1032 19991121.46437 145C Mis image="KenIchi Kadota" MisV1032 19991121.46480 143C Mis image="KenIchi Kadota" MisV1032 20000813.50325 108C Mis image="Nobuo Ohkura" MisV1032 20000813.50510 108C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1032. 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". The identification with the 2MASS data is by Taichi Kato. 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/