Rc Rc-band CCD magnitude observed by Seiichiro Kiyota. Kiyota Rc Lm Upper limit of Rc-band CCD magnitude observed by Seiichiro Kiyota. The star is fainter than the plotted magnitude. Details are in magnitude data page .
Details are in magnitude data page .
The star is fainter than the plotted magnitude. Details are in magnitude data page . Details are in magnitude data page . Details are in magnitude data page . The light curve suggests the MisV0001 is a Mira type variable star with a period of about 390 days.