Home Page Updated on April 20, 2018
= USNO-A2.0_0600.29987534 18 01 06.941 -27 41 33.73 13.2R 15.5B
It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ken-ichi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida.
Klaus Bernhard and Stefan Huemmerich reported the MACHO data revealed it is a Mira type variable with a period of 255 days, brightness range of 11.6:-16.5 mag(Rc) (light curve).
Observations by MISAO Project