They suggest that MisV0955 is a SR-type variable star. Ic Ic-band CCD magnitude observed by Seiichiro Kiyota. Details are in magnitude data page . The two types of light curves well fit each other. They suggest that MisV0956 is a Mira-type variable star.
Details are in magnitude data page .
It faded at only one night, which suggests that this is an eclipsing variable star. Details are in magnitude data page . It brightened and faded repeatedly in short time. Details are in magnitude data page . It brightened and faded repeatedly in short time.