Dear colleagues, New variable star discovery by the MISAO Project (MisV1214). MisV1214 R.A. 03h16m56s.11 Decl. +55o52'33".6 (2000.0) Mag. 13.0-15.1C Type M? = IRAS 03131+5541 03h16m56s.8 +55o52'36" Ellipse:25x4" P.A.:72 Flux(12):2.353 Flux(25):1.628 Flux(60):<0.6296 Flux(100):<5.137 Var:99% = MSX5C G142.3708-01.4047 03h16m56s.23 +55o52'33".2 InScanError:2.0" CrossScanError:1.4" Flux(A):3.8658 Flux(C):4.7097(var) Flux(D):2.8994 = 031656.1 +555237 (2000.0) NSS11 13.1 * http://vsnet.aerith.net/misao/data/MisV/MisV1214.gif MisV1214 20001109.61515 13.86C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20001109.61701 13.79C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20001109.61887 13.83C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20001109.62072 14.03C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20001224.48734 13.07C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20001224.48919 13.03C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20001224.49105 12.99C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20001224.49291 13.14C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20011010.70075 14.75C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20011010.70272 14.96C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20011010.70469 14.97C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20011012.69059 14.85C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1214 20011012.69256 15.06C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, MISAO Project, discovered a new variable star MisV1214. It was picked up by Seiichi Yoshida from the candidates of new variable stars detected by the PIXY system 2 from images taken by Nobuo Ohkura, and confirmed by Ken-ichi Kadota. The identification is researched by Taichi Kato (Kyoto University), John Greaves, and Seiichi Yoshida. The magnitude are measured automatically by the PIXY system 2. About the MISAO Project and the PIXY system 2: http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/
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