Dear colleagues, New variable star discovery by the MISAO Project (MisV0999). MisV0999 R.A. 20h11m55s.14 Decl. +31o12'20".7 (2000.0) Mag. 13.2C-16.0C Type M: = IRAS 20099+3103 R.A.=20 11 54.78 Decl.=+31 12 14.9 (73 x 9", p.a.=63) flux(12)=0.55 flux(25)=0.37 flux(60)=<2.24 flux(100)=<18.39 0% variable = 2MASS 201155.120 +311220.63 (2000.0) 8.309 6.743 6.010 http://vsnet.aerith.net/misao/data/MisV/MisV0999.gif MisV0999 19990803.67530 132C Mis image="KenIchi Kadota" MisV0999 19990803.67593 133C Mis image="KenIchi Kadota" MisV0999 19991121.40713 141C Mis image="KenIchi Kadota" MisV0999 19991121.40758 138C Mis image="KenIchi Kadota" MisV0999 20000708.56856 160C Mis image="Nobuo Ohkura" MisV0999 20000708.57042 158C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0999. 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/