Schmeer C Unfiltered CCD magnitude observed by Patrick Schmeer. MisV0508 is identified with V949 Sgr which was reported as a nova in 1914. But the light curve shows the slow fading, that suggests MisV0508 is a red variable star. Further details are described in IBVS 4845 . 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 400 days. John Greaves, UK, identified MisV0533 and ASAS 175752-2241.5. Details are in magnitude data page . The star is fainter than the plotted magnitude. Details are in magnitude data page .