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Dear colleagues, New variable star discovery by the MISAO Project (MisV1213). MisV1213 R.A. 02h38m47s.55 Decl. +56o43'11".3 (2000.0) Mag. 12.9-14.2C Type SR? = IRAS 02351+5630 02h38m47s.8 +56o43'09" Ellipse:18x6" P.A.:63 Flux(12):23.06 Flux(25):8.921 Flux(60):1.943 Flux(100):<1.574 Var:6% = MSX5C G137.2977-03.1281 02h38m47s.42 +56o43'09".1 InScanError:2.2" CrossScanError:1.8" Flux(A):27.325 Flux(C):19.870 Flux(D):14.426 Flux(E):7.2236 = 2MASS 023847.580 +564310.34 (2000.0) 7.283 5.393 0.000 http://vsnet.aerith.net/misao/data/MisV/MisV1213.gif MisV1213 20001224.46506 12.85C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1213 20001224.46692 13.01C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1213 20001224.46877 12.87C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1213 20011010.67709 14.09C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1213 20011122.55814 14.17C 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 MisV1213. 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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