Dear colleagues, New variable star discovery by the MISAO Project (MisV1014). MisV1014 R.A. 20h09m32s.75 Decl. +30o21'08".6 (2000.0) Mag. 11.9C-13.8C Type SR: = IRAS 20075+3012 R.A.=20 09 32.29 Decl.=+30 21 06.1 (21 x 5", p.a.=70) flux(12)=2.34 flux(25)=1.37 flux(60)=0.90 flux(100)=<44.31 47% variable = 2MASS 200932.819 +302107.79 (2000.0) 6.964 5.477 0.000 http://vsnet.aerith.net/misao/data/MisV/MisV1014.gif MisV1014 19990715.65855 119C Mis image="KenIchi Kadota" MisV1014 19990715.65902 119C Mis image="KenIchi Kadota" MisV1014 19990803.67126 125C Mis image="KenIchi Kadota" MisV1014 19990803.67419 125C Mis image="KenIchi Kadota" MisV1014 20000706.60259 138C Mis image="Nobuo Ohkura" MisV1014 20000706.60443 138C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1014. 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/