Dear colleagues, New variable star discovery by the MISAO Project (MisV1031). MisV1031 R.A. 20h38m19s.74 Decl. +34o12'20".3 (2000.0) Mag. 11.4C-13.6C Type M? = IRAS 20363+3401 R.A.=20 38 19.81 Decl.=+34 12 21.3 (24 x 5", p.a.=63) flux(12)=6.21 flux(25)=5.10 flux(60)=0.68 flux(100)=<36.21 99% variable = 2MASS 203819.812 +341220.71 (2000.0) 7.216 5.992 5.095 http://vsnet.aerith.net/misao/data/MisV/MisV1031.gif MisV1031 19990709.77422 136C Mis image="KenIchi Kadota" MisV1031 19990709.77470 136C Mis image="KenIchi Kadota" MisV1031 20000803.54104 114C Mis image="Nobuo Ohkura" MisV1031 20000803.54289 115C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1031. 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/