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Table 4

Comparison between the median-likelihood estimates of the star formation rate derived from our fits to the SEDs (a) and the star formation rate computed from the dust luminosity using the formula of Kennicutt 1998 (b).

Galaxy ψ/M yr-1 ψK98/M yr-1
(a) (b)

IRAS 00199-7426 210
IRAS 01494-1845 189
IRAS Z02376-0054 304
IRAS 04114-5117 180
IRAS 06009-7716 108
IRAS F08208+3211 301
IRAS F10156+3705 414
IRAS 10565+2448 100
IRAS 12112+0305 231
IRAS 13120-5453 176
IRAS 16334+4630 288
IRAS 17208-0014 191
IRAS 19297-0406 251
IRAS 19458+0944 168
IRAS 20414-1651 170
IRAS 22491-1808 143

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