Fig. 1.From: Infrared composition of the Large Magellanic CloudAKARI observed an area of about 10 deg2 of the Large Magellanic Cloud. The dash-dotted outline indicates the coverage of the Spitzer/SAGE survey (Meixner et al., 2006), and the dashed outline shows the coverage of the Large Magellanic Cloud optical photometric survey (Zaritsky et al., 2004). AKARI sources not identified in any of selected databases are shown with black triangles, and sources with identified counterparts by white squares.Back to article page