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. Taichi Kato reported that MisV0001 was about 16 mag on V-band image taken by Kyoto University Ouda team in 1996 March. All rights reserved.