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Dear colleagues, New variable star discovery by the MISAO Project (MisV1190). MisV1190 R.A. 02h09m46s.83 Decl. +46o43'17".4 (2000.0) Mag. 11.6-12.3C Type ? = GSC 3281-02158 02h09m46s.87 +46o43'17".3 Error:0.2" Mag:12.39 MagError:0.44 Band:1 Class:3 Plate:036J Flag:F Epoch:08 SEP 1983 = USNO-A2.0 1350.02032023 02h09m46s.897 +46o43'18".00 Mag(R):12.3 Mag(B):12.9 http://vsnet.aerith.net/misao/data/MisV/MisV1190.gif MisV1190 20001202.47885 11.89C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1190 20001202.48072 11.80C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1190 20001202.48257 11.86C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1190 20001224.45031 11.64C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1190 20001224.45216 11.72C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1190 20011012.64747 12.28C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1190 20011012.64943 12.25C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1190 20011012.65140 12.31C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1190 20011128.52750 12.00C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1190 20011128.52947 12.08C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1190 20011210.50249 11.82C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1190 20011210.50446 11.81C 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 MisV1190. 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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