Dear colleagues, New variable star discovery by the MISAO Project (MisV1028). MisV1028 R.A. 20h14m52s.00 Decl. +37o18'36".2 (2000.0) Mag. 11.0C-12.0C Type SR? = USNO-A2.0_1200.14780457 20 14 52.001 +37 18 36.21 14.1R 17.6B = IRAS 20130+3709 R.A.=20 14 52.27 Decl.=+37 18 37.0 (30 x 9", p.a.=64) flux(12)=0.73 flux(25)=0.43 flux(60)=<6.40 flux(100)=<68.99 1% variable = 2MASS 201451.982 +371836.09 (2000.0) 6.983 5.861 5.440 http://vsnet.aerith.net/misao/data/MisV/MisV1028.gif MisV1028 19991121.41485 112C Mis image="KenIchi Kadota" MisV1028 19991121.41586 110C Mis image="KenIchi Kadota" MisV1028 20000804.52413 119C Mis image="Nobuo Ohkura" MisV1028 20000804.52598 120C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1028. 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/