Dear colleagues, New variable star discovery by the MISAO Project (MisV1160). MisV1160 R.A. 21h34m26s.12 Decl. +51o04'32".4 (2000.0) Mag. 13.5-15.5C Type ? = IRAS 21326+5051 21h34m26s.0 +51o04'31" Ellipse:8x4" P.A.:178 Flux(12):0.8083 Flux(25):0.3692 Flux(60):<2.372 Flux(100):<26.34 Var:68% = MSX5C G094.5071-00.5870 21h34m25s.94 +51o04'33".6 InScanError:2.0" CrossScanError:1.4" Flux(A):0.56119(var) http://vsnet.aerith.net/misao/data/MisV/MisV1160.gif MisV1160 20001014.46391 13.54C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1160 20011002.47885 15.13C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1160 20011002.48082 15.10C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1160 20011002.48279 15.49C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1160 20011018.44218 15.21C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, MISAO Project, discovered a new variable star MisV1160. 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/