Dear colleagues, New variable star discovery by the MISAO Project (MisV1027). MisV1027 R.A. 20h14m25s.10 Decl. +47o55'26".0 (2000.0) Mag. 10.2C-11.6C Type SR? = GSC3563.2178 20 14 25.59 +47 55 23.0 13.04 = IRAS 20128+4746 R.A.=20 14 25.61 Decl.=+47 55 27.9 (21 x 4", p.a.=59) flux(12)=3.54 flux(25)=1.39 flux(60)=<1.36 flux(100)=<10.94 20% variable = 2MASS 201425.004 +475526.21 (2000.0) 6.135 5.077 4.501 http://vsnet.aerith.net/misao/data/MisV/MisV1027.gif MisV1027 19991121.42921 102C Mis image="KenIchi Kadota" MisV1027 19991121.42965 102C Mis image="KenIchi Kadota" MisV1027 20000815.47177 115C Mis image="Nobuo Ohkura" MisV1027 20000815.47362 116C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1027. 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". MisV1027 is a pair of double stars. The identification with GSC3563.2178 is by Taichi Kato and John Greaves. 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/