Dear colleagues, New variable star discovery by the MISAO Project (MisV1211). MisV1211 R.A. 03h24m46s.08 Decl. +55o52'12".8 (2000.0) Mag. 12.1-13.1C Type SR? = USNO-A2.0 1425.04323306 03h24m46s.068 +55o52'11".95 Mag(R):14.9 Mag(B):19.3 = IRAS 03209+5541 03h24m46s.4 +55o52'12" Ellipse:18x4" P.A.:75 Flux(12):1.370 Flux(25):0.5980 Flux(60):<0.5289 Flux(100):<6.923 Var:24% = MSX5C G143.2991-00.8174 03h24m46s.06 +55o52'08".0 InScanError:1.9" CrossScanError:1.4" Flux(A):1.1038 http://vsnet.aerith.net/misao/data/MisV/MisV1211.gif MisV1211 20001109.62072 13.05C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20001109.62257 13.00C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20001109.62442 13.08C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20001224.49291 12.36C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20001224.49477 12.35C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20001224.49661 12.47C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20001224.49847 12.68C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20011010.70469 12.08C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20011010.70667 12.10C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20011010.70863 12.18C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20011010.71060 12.22C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20011012.69650 12.21C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1211 20011012.69847 12.27C 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 MisV1211. 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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