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. Taichi Kato reported that MisV0001 was about 16 mag on V-band image taken by Kyoto University Ouda team in 1996 March.
Details are in magnitude data page .
It must be a short-period eclipsing binary. Details are in magnitude data page . The star is fainter than the plotted magnitude. Details are in magnitude data page . I-band CCD magnitude observed by the TASS project.