Fig. 5.
Estimated SEDs of ASAGAO sources. Red symbols with errors are observed flux densities. Blue solid lines are the best-fitting SEDs estimated by MAGPHYS (see section 3). The black dashed lines are the best-fitting SEDs using a modified blackbody + mid-IR power-law model by Casey (2012). (Color online)

Estimated SEDs of ASAGAO sources. Red symbols with errors are observed flux densities. Blue solid lines are the best-fitting SEDs estimated by MAGPHYS (see section 3). The black dashed lines are the best-fitting SEDs using a modified blackbody + mid-IR power-law model by Casey (2012). (Color online)

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