Dear colleagues, New variable star discovery by the MISAO Project (MisV1035). MisV1035 R.A. 21h29m39s.51 Decl. +49o49'57".2 (2000.0) Mag. 10.7C-11.5C Type SR? = USNO-A2.0_1350.14202461 21 29 39.514 +49 49 57.21 12.5R 16.1B = IRAS 21279+4936 R.A.=21 29 39.59 Decl.=+49 49 55.9 (15 x 8", p.a.=35) flux(12)=1.12 flux(25)=0.43 flux(60)=<0.45 flux(100)=<14.83 20% variable = 2MASS 212939.460 +494956.70 (2000.0) 6.382 5.234 4.715 http://vsnet.aerith.net/misao/data/MisV/MisV1035.gif MisV1035 19990709.67728 107C Mis image="KenIchi Kadota" MisV1035 19990709.67786 108C Mis image="KenIchi Kadota" MisV1035 20000810.54072 115C Mis image="Nobuo Ohkura" MisV1035 20000810.54258 115C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1035. 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 and John Greaves. 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/