Return to Home Page
Dear colleagues, New variable star discovery by the MISAO Project (MisV1199). MisV1199 R.A. 00h42m38s.31 Decl. +67o20'07".6 (2000.0) Mag. 10.4-11.1C Type ? = GSC 4028-00416 00h42m38s.36 +67o20'06".6 Error:0.2" Mag:13.20 MagError:0.42 Band:1 Class:0 Plate:00MB Flag:F Epoch:06 NOV 1983 = USNO-A2.0 1500.00743405 00h42m38s.364 +67o20'06".97 Mag(R):12.5 Mag(B):16.6 = IRAS 00396+6703 00h42m38s.6 +67o20'05" Ellipse:16x5" P.A.:34 Flux(12):2.443 Flux(25):1.394 Flux(60):<0.5784 Flux(100):<13.44 Var:17% = MSX5C G122.0815+04.4774 00h42m38s.14 +67o20'04".2 InScanError:2.1" CrossScanError:2.0" Flux(A):1.9605 Flux(C):2.3858 Flux(D):1.9632 http://vsnet.aerith.net/misao/data/MisV/MisV1199.gif MisV1199 20010101.38221 10.42C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20010101.38409 10.37C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20010101.38593 10.37C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20010101.38778 10.36C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20010101.38964 10.35C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20010101.39149 10.40C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20011031.53531 11.05C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20011031.53728 10.96C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20011031.53925 10.98C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20011031.54122 11.00C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 MisV1199 20011031.54318 10.99C Mis KAF-1600 Tycho-2_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8 Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, MISAO Project, discovered a new variable star MisV1199. 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 Ken-ichi Kadota. The identification is researched by Taichi Kato (Kyoto University), John Greaves, 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/
Return to the Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
