The ASAS observations reveal that it is SR-type with a period of 340 days. But the light curve behaves a bit strange around the peak. John Greaves, UK, identified MisV0271 and ASAS 170149-2301.3. Details are in magnitude data page . I-band CCD magnitude observed by the TASS project, researched by Michael Richmond.
Details are in magnitude data page .
The star is fainter than the plotted magnitude. Details are in magnitude data page . I-band CCD magnitude observed by the TASS project, researched by Michael Richmond. MisV0380 C. P. Jones v Lm Upper limit of visual observation by C. P. Jones. The star is fainter than the plotted magnitude.