Home Page Updated on May 15, 2016
= IRAS 01470+6557 01h50m43s.7 +66o12'25" Ellipse:26x9" P.A.:47 Flu x(12):0.4258 Flux(25):0.1318 Flux(60):<0.6171 Flux(100):<13.48 V ar:0%
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, MISAO Project, discovered a new variable star MisV1344.
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 with a period of about 300 days and the epoch of JD = 2451370.
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