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Fig. 3

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NIR–FIR SED of our debris disk candidates with 18 μm excess. The pluses, filled squares, open circles, crosses, open diamonds, open triangles, and filled circles indicate the photometry with the 2MASS, AKARI/IRC, IRAS, MSX, WISE, ground-based observations (Subaru/COMICS and Gemini/T-ReCS), and Spitzer/MIPS, repectively. We also plot contributions of the photosphere (dashed lines) and those of inner disk component (dotted lines) fitted with AKARI/IRC, IRAS, and Spitzer/MIPS measurements by assuming that the debris dust emits blackbody emission.

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