Photometric data collected for LMC562.05.9009. Upper panel: OGLE (dots) and converted EROS-R (+) I-band data; middle panel: MACHO R-band data; lower panel: OGLE (dots) and MACHO (x) V-band data. The pattern seen in the time series out-of-eclipse data is due to the near-3 day pulsation period of the Cepheid in the system.