Fig. 9.From: Infrared composition of the Large Magellanic CloudColor-magnitude diagrams N3–S11 vs S11 (upper) for sources identified as foreground (diamonds) and background objects (filled circles). Objects fulfilling conditions for foreground objects proposed by Ita et al. (2008) are placed in the gray area with a dashed outline, objects corresponding to background galaxies have a dash-dotted outline. Modifications of the conditions adapted for our sample is shown with a solid thick outline.Back to article page