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Dear colleagues, New variable star discovery by the MISAO Project (MisV1183). MisV1183 R.A. 20h27m23s.50 Decl. +47o48'51".9 (2000.0) Mag. 12.7-13.9C Type SR? = USNO-A2.0 1350.12352582 20h27m23s.516 +47o48'51".98 Mag(R):16.4 Mag(B):19.6 = 2MASS 202723.490 +474852.03 (2000.0) 8.793 7.615 7.038 http://vsnet.aerith.net/misao/data/MisV/MisV1183.gif MisV1183 20001010.42449 12.83C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1183 20001010.42634 12.73C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1183 20001010.42819 12.85C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1183 20011010.43137 13.85C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1183 20011010.43333 13.83C 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 MisV1183. 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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