Table 3
Median-likelihood estimates and confidence ranges (computed as the 16th–84th percentile range of the likelihood distribution) of some relevant parameters derived from the multi-wavelength fits to the observed SEDs of our ULIRGs.
| Galaxy | f μ | log (ψS/M⊙ yr-1) | log (M∗/M⊙) |
|
log (Md/M⊙) |
|
|
|
|
| (a) | (b) | (c) | (d) | (e) | (f) | (g) | (h) | (i) | |
|
|
|||||||||
| IRAS 00199-7426 |
|
|
|
|
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|
|
|
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| IRAS 01494-1845 |
|
|
|
|
|
|
|
|
|
| IRAS Z02376-0054 |
|
|
|
|
|
|
|
|
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| IRAS 04114-5117 |
|
|
|
|
|
|
|
|
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| IRAS 06009-7716 |
|
|
|
|
|
|
|
|
|
| IRAS F08208+3211 |
|
|
|
|
|
|
|
|
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| IRAS F10156+3705 |
|
|
|
|
|
|
|
|
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| IRAS 10565+2448 |
|
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|
|
|
|
|
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| IRAS 12112+0305 |
|
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|
|
|
|
|
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| IRAS 13120-5453 |
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|
|
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| IRAS 16334+4630 |
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|
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|
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| IRAS 17208-0014 |
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| IRAS 19297-0406 |
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| IRAS 19458+0944 |
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| IRAS 20414-1651 |
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|
|
|
|
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| IRAS 22491-1808 |
|
|
|
|
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|
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|
Notes. (a) fraction of total dust luminosity contributed by the diffuse ISM; (b) specific star formation rate; (c) stellar mass; (d) dust luminosity; (e) dust mass; (f) equilibrium temperature of warm dust in birth clouds; (g) contribution of warm dust in thermal equilibrium to the total dust luminosity; (h) equilibrium temperature of cold dust in the diffuse ISM; (i) contribution of cold dust in thermal equilibrium to the total dust luminosity.
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