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Dear colleagues, New variable star discovery by the MISAO Project (MisV1188). MisV1188 R.A. 22h22m20s.53 Decl. +47o47'45".2 (2000.0) Mag. 13.1-14.0C Type ? = USNO-A2.0 1350.16471756 22h22m20s.533 +47o47'45".40 Mag(R):12.7 Mag(B):14.0 http://vsnet.aerith.net/misao/data/MisV/MisV1188.gif MisV1188 20001010.49495 14.01C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1188 20001010.49681 14.01C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1188 20001010.49866 13.78C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1188 20011010.50619 13.11C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1188 20011010.50816 13.09C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, MISAO Project, discovered a new variable star MisV1188. 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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