Dear colleagues, New variable star discovery by the MISAO Project (MisV1169). MisV1169 R.A. 21h52m03s.90 Decl. +57o49'15".5 (2000.0) Mag. 12.8-15.5C Type M: = IRAS 21504+5735 21h52m04s.2 +57o49'17" Ellipse:9x9" P.A.:32 Flux(12):0.7782 Flux(25):0.3767 Flux(60):<2.075 Flux(100):<23.40 Var:45% = MSX5C G100.8448+02.8570 21h52m04s.44 +57o49'11".3 InScanError:2.8" CrossScanError:1.7" Flux(A):0.82442 http://vsnet.aerith.net/misao/data/MisV/MisV1169.gif MisV1169 20001010.47260 13.51C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1169 20001010.47447 13.48C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1169 20001010.47632 13.56C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1169 20001010.47817 13.63C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1169 20001105.41551 12.84C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1169 20001105.41736 12.76C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1169 20001105.41922 12.87C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1169 20001105.42109 12.78C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1169 20011003.49164 14.66C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1169 20011005.50912 15.53C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1169 20011110.41074 14.06C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1169 20011110.41272 14.18C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1169 20011110.41468 14.07C 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 MisV1169. 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/