Dear colleagues, New variable star discovery by the MISAO Project (MisV0995). MisV0995 R.A. 19h51m29s.51 Decl. +27o08'57".8 (2000.0) Mag. 12.4C-<16.0C Type M? = IRAS 19494+2701 R.A.=19 51 29.75 Decl.=+27 08 53.6 (26 x 5", p.a.=73) flux(12)=22.83 flux(25)=22.73 flux(60)=9.73 flux(100)=<39.19 99% variable = 2MASS 195129.412 +270859.03 (2000.0) 6.718 0.000 0.000 http://vsnet.aerith.net/misao/data/MisV/MisV0995.gif MisV0995 19990803.62922 <160C Mis image="KenIchi Kadota" MisV0995 19990803.62966 <160C Mis image="KenIchi Kadota" MisV0995 20000615.57047 125C Mis image="Nobuo Ohkura" MisV0995 20000615.57233 124C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0995. 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/