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 . 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 .
The light curve is strange. The unfiltered CCD observations suggest that short-period variability with about 20 day period. But the difference between unfiltered CCD magnitude and CCD magnitude with IR-blocking filter suggests that MisV0073 is a red variable star. Details are in magnitude data page . I-band CCD magnitude observed by the TASS project, researched by Michael Richmond.