Dear colleagues, New variable star discovery by the MISAO Project (MisV0997). MisV0997 R.A. 20h02m03s.40 Decl. +26o55'54".7 (2000.0) Mag. 13.1C-13.8C Type SR? = IRAS 19599+2647 R.A.=20 02 04.39 Decl.=+26 55 56.0 (69 x 3", p.a.=74) flux(12)=0.43 flux(25)=<0.29 flux(60)=<0.56 flux(100)=<46.09 = 2MASS 200203.299 +265555.31 (2000.0) 7.965 6.747 6.152 http://vsnet.aerith.net/misao/data/MisV/MisV0997.gif MisV0997 19990430.71321 134C Mis image="KenIchi Kadota" MisV0997 19990430.71363 135C Mis image="KenIchi Kadota" MisV0997 19990724.57537 138C Mis image="KenIchi Kadota" MisV0997 19990724.57582 138C Mis image="KenIchi Kadota" MisV0997 20000615.57788 131C Mis image="Nobuo Ohkura" MisV0997 20000615.57973 131C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0997. 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/