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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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