Dear colleagues, New variable star discovery by the MISAO Project (MisV1176). MisV1176 R.A. 20h39m40s.53 Decl. +43o51'47".4 (2000.0) Mag. 14.4-[17.2C Type M: = MSX5C G082.9716+01.3782 20h39m40s.70 +43o51'46".8 InScanError:2.0" CrossScanError:1.3" Flux(A):2.2502 Flux(C):1.7597 Flux(D):1.4603 = 2MASS 203940.458 +435147.07 (2000.0) 8.968 7.125 6.037 http://vsnet.aerith.net/misao/data/MisV/MisV1176.gif MisV1176 20000803.54093 <17.17C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1176 20000803.54278 <17.06C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1176 20000905.47781 16.08C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1176 20000905.47966 15.80C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1176 20001001.45735 14.76C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1176 20001001.45920 14.93C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1176 20001001.46105 14.93C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1176 20011015.40907 14.82C Mis KAF-0261E USNO-A2.0_(R) Nobuo_Ohkura 0.36-m_Schmidt-Cassegrain_+_f/5.5_reducer_lens_+_SBIG_ST-9E MisV1176 20011015.41007 14.47C Mis KAF-0261E Tycho-2_Catalogue Nobuo_Ohkura 0.36-m_Schmidt-Cassegrain_+_f/5.5_reducer_lens_+_SBIG_ST-9E MisV1176 20011015.41134 14.80C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1176 20011015.41331 14.43C Mis KAF-1600L Tycho-2_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 KenIchi Kadota, MISAO Project, discovered a new variable star MisV1176. 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 KenIchi Kadota. The identification is researched by Taichi Kato (Kyoto University), John Greaves (the United Kingdom), 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/