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Earth, Planets and Space
Fig. 5. | Earth, Planets and Space

Fig. 5.

From: Dusty Universe viewed by AKARI far infrared detector

Fig. 5.

Distribution of the Bayesian estimates of the output parameters: D4000, Mstar, and logSFR. SSFR values were calculated as the ratio of SFR and Mstar. LUV, and Ltir were calculated as an integral value of SEDs from 1480(1 + z) to 1520(1 + z) Å, and from 8(1 + z) μm to 1(1 + z) mm, respectively.

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