Table 12.
Far infrared continuum and line luminosities.
| ID | LTIR | LFIRw | LFIRn, SED | LFIRn, H88 | LCII | LOI63 | LOIII88 | LCO10 |
|---|---|---|---|---|---|---|---|---|
| 3−1100 μm | 40−500 μm | 40−120 μm | 40−120 μm | |||||
| [1042 erg s−1] | [1042 erg s−1] | [1042 erg s−1] | [1042 erg s−1] | [1039 erg s−1] | [1039 erg s−1] | [1039 erg s−1] | [1036 erg s−1] | |
| 1 |
 |
 |
 |
 |
– | – | – | < 48 |
| 2 |
 |
 |
 |
 |
17 ± 8 | 62 ± 43 | – | < 80 |
| 3 |
 |
 |
 |
 |
1564 ± 36 | 2994 ± 145 | 1918 ± 124 | 619 ± 31 |
| 4 |
 |
 |
 |
 |
– | – | – | – |
| 5 |
 |
 |
 |
 |
1260 ± 223 | – | 671 ± 114 | < 53 |
| 6 |
 |
 |
 |
 |
– | – | – | – |
| 7 |
 |
 |
 |
 |
– | – | – | < 62 |
| 8 |
 |
 |
 |
 |
3580 ± 549 | – | – | 629 ± 14 |
| 9 |
 |
 |
 |
 |
1471 ± 29 | 1284 ± 119 | – | 69 ± 7 |
| 10 |
 |
 |
 |
 |
– | – | – | < 434 |
| 11 |
 |
 |
 |
 |
8930 ± 542 | – | – | 671 ± 43 |
| 12 |
 |
 |
 |
 |
383 ± 55 | 532 ± 158 | – | < 653 |
| 13 |
 |
 |
 |
 |
1785 ± 182 | 2124 ± 446 | – | 502 ± 45 |
| 14 |
 |
 |
 |
 |
– | – | – | – |
Notes. For continuum (TIR and FIR) luminosities we integrate the best-fit Draine et al. (2007) SED model for each model, using a variety of ranges along the wavelength axis. For total infrared (TIR), we use 3−1100 μm, as defined in Kennicutt & Evans (2012). In order to compare our measurements to previous studies (as done in Fig. 12), we further calculate several versions of the FIR luminosity: LFIRw, which is integrated over 40−500 μm and used on the x-axis of Fig. 12, and LFIRn, H88, which is the FIR luminosity valid for the range of 40−120 μm, but estimated from single flux densities at 60 and 100 μm as defined by Helou et al. (1988). The luminosity LFIRn, H88 is used for the [C II]-to-FIR ratio that is given on the y-axis in Fig. 12. For comparison, we also provide LFIRn, SED, which is the SED-integrated luminosity along the same range of 40−120 μm. The line luminosities are derived via Gaussian fitting.
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