Dear colleagues, New variable star discovery by the MISAO Project (MisV1154). MisV1154 R.A. 20h44m18s.47 Decl. +50o04'36".5 (2000.0) Mag. 12.3-13.3C Type ? = USNO-A2.0 1350.12833278 20h44m18s.448 +50o04'36".16 Mag(R):14.9 Mag(B):19.2 = IRAS 20427+4953 20h44m18s.5 +50o04'35" Ellipse:12x5" P.A.:144 Flux(12):10.56 Flux(25):6.445 Flux(60):1.083 Flux(100):<30.13 Var:25% = MSX5C G088.3701+04.5681 20h44m18s.46 +50o04'36".8 InScanError:1.2" CrossScanError:0.8" Flux(A):6.7332(var) Flux(B2):9.4701 Flux(C):6.3442(var) Flux(D):4.4675(var) Flux(E):4.2881(var) http://vsnet.aerith.net/misao/data/MisV/MisV1154.gif MisV1154 20000902.48662 12.68C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1154 20000902.48846 12.69C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1154 20001013.43215 13.31C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1154 20001013.43400 13.31C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1154 20001013.43587 13.18C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1154 20011003.45045 12.39C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1154 20011003.45242 12.29C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1154 20011003.45440 12.31C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG) MisV1154 20011019.40969 12.85C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1154 20011019.41166 12.93C 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 MisV1154. 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/