Home Page Updated on April 30, 2016
= IRAS 23559+6540 23h58m30s.5 +65o56'57" Ellipse:15x3" P.A.:33 Flu x(12):2.293 Flux(25):1.438 Flux(60):0.7898 Flux(100):<19.48 Var: 20% = MSX5C G117.5671+03.6287 23h58m30s.02 +65o56'51".0 InScanError:2.5" CrossScanError:1.7" Flux(A):3.3159 Flux(C):2.9835(var) Flux(D): 2.2762(var)
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, MISAO Project, discovered a new variable star MisV1347.
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 NSVS data suggests it is a Mira type variable, although the period is not determined.
Light curve by the Northern Sky Variability Survey (NSVS) created using SkyDOT.
SkyDOT is operated by the University of California for the National Nuclear Security Administration of the US Department of Energy.
Observations by MISAO Project