Rod Stubbings v Lm Upper limit of visual observation by Rod Stubbings. The star is fainter than the plotted magnitude. Probably a Mira type variable. They reported that the star was fainter than 14.2 mag visually even when it was bright at 12.4 mag on unfiltered CCD image. I I-band CCD magnitude observed by the ASAS project.
Details are in magnitude data page .
I-band CCD magnitude observed by the TASS project, researched by Michael Richmond. The ASAS observations reveal that it is SR-type with a period of 280 days. However, in case there were no systematic shift between the ASAS and TASS magnitude, the period would be 260 days. John Greaves, UK, identified MisV0430 and ASAS 184339-0004.5. I I-band CCD magnitude observed by the ASAS project.