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Fig. 12. | Earth, Planets and Space

Fig. 12.

From: Infrared composition of the Large Magellanic Cloud

Fig. 12.

Color-magnitude diagram N3–S7 vs N3 for sources identified as (1) foreground objects, AGBs, possible AGB, stars and multiple stars (light gray area), or (2) post-AGBs, YSOs and background objects (dark gray area) (upper panel) and not identified (lower panel) with classification based on SVM. Dark gray area is corresponding to objects classified as foreground objects, AGBs, possible AGB stars, or multiple stars. The light gray area corresponds to post-AGBs, YSOs, and background objects.

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