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Table 3.

G RASIL results from the SED fitting.

log LIR SFRIR SFRSED SFRUV sSFRSED log M* log Mdust log Tdust AV log ageM
(L) (M yr−1) (M yr−1) (M yr−1) (Gyr1) (M) (M) (K) (mag) (yr)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
10.74 5.21 3.69 0.54 0.14 10.43 8.93 21 0.96 9.93

Notes.

(1)

8–1000 μm infrared luminosity.

(2)

Star formation rate from LIR (Kennicutt 1998).

(3)

Star formation rate from SED modelling.

(4)

Star formation rate from UV emission (Kennicutt 1998).

(5)

Specific star formation rate (≡SFRSED/M*).

(6)

Stellar mass.

(7)

Dust mass.

(8)

Dust temperature.

(9)

Mean dust attenuation at V-band.

(10)

Mass-weighted age.

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