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.
Details are in magnitude data page .
It was observed many times by the ASAS project, around the peak. John Greaves, UK, identified MisV0476 and ASAS 175659-2406.2. I-band CCD magnitude observed by the ASAS project. Details are in magnitude data page . The ASAS observations reveal that it is Mira type with a period of 550 days.