Fig. A.1.From: Infrared composition of the Large Magellanic CloudThe distribution of positional differences between the sources and identified counterparts in 2MASS, NED, SIMBAD, AKARI FIS All-Sky Survey, OGLE. The size of the bin is 0.1 arcsec for the AKARI data, extended to 0.5 arcsec for the FIS data.Back to article page