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Dear colleagues, New variable star discovery by the MISAO Project (MisV1216). MisV1216 R.A. 22h07m38s.51 Decl. +49o02'59".4 (2000.0) Mag. 11.4-12.3C Type ? = IRAS 22056+4848 22h07m38s.1 +49o02'54" Ellipse:28x6" P.A.:46 Flux(12):4.183 Flux(25):2.143 Flux(60):<0.4298 Flux(100):<7.589 Var:0% http://vsnet.aerith.net/misao/data/MisV/MisV1216.gif MisV1216 20000919.51120 12.27C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20000919.51306 12.17C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20000919.51492 12.17C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20001011.48617 12.28C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20001011.48801 12.23C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20001011.48986 12.33C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20011005.51911 11.46C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20011005.52109 11.45C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20011005.52304 11.35C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1216 20011023.45495 11.60C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1216 20011024.44833 11.48C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1216 20011024.45031 11.56C Mis KAF-1600 Tycho_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 MisV1216. 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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