Dear colleagues, New variable star discovery by the MISAO Project (MisV1173). MisV1173 R.A. 03h00m33s.36 Decl. +56o21'53".0 (2000.0) Mag. 14.9-16.6C Type ? = IRAS 02568+5610 03h00m34s.6 +56o22'00" Ellipse:44x7" P.A.:62 Flux(12):1.402 Flux(25):0.4552 Flux(60):<0.4000 Flux(100):<3.089 Var:20% = MSX5C G140.1511-02.1279 03h00m33s.70 +56o21'52".6 InScanError:2.1" CrossScanError:1.6" Flux(A):1.3422(var) Flux(C):1.8303 Flux(D):1.3649 http://vsnet.aerith.net/misao/data/MisV/MisV1173.gif MisV1173 20001224.47806 15.11C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20001224.47991 14.87C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20001224.48177 15.36C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20001224.48362 15.13C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20011010.68892 16.63C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20011010.69089 16.52C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20011010.69287 16.43C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20011010.69484 16.36C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20011124.56523 16.32C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20011124.56721 16.08C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20011124.56918 16.29C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1173 20011124.57115 16.41C Mis KAF-1600 Tycho-2_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 MisV1173. 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/