It seems to be a short periodic variable star. So MisV0911 is probably an irregular type. John Greaves, UK, identified MisV0911 and ASAS 170103-2317.1. Ic Ic-band CCD magnitude observed by Seiichiro Kiyota. Kiyota Rc Rc-band CCD magnitude observed by Seiichiro Kiyota.
Details are in magnitude data page .
The three types of light curves well fit one another. 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.