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. V V-band CCD magnitude observed by the TASS project. The light curve is very strange. If it is linked to the slow fading observed by TASS I-band, the period is 500 days or more, and it was at minimum around 2451100. Details are in magnitude data page .