Table 2
Best-fit model parameters (cf. Sect. 4).
| Sourcesa | Modelb | χ2 /d.o.f. | 
(mJy)c |
α 6 d | Spectral indexe | τ 6 f | Additional features |
|
|
|||||||
| IRAS F00235+1024 | A | 238/75 | 86 ± 5 | 0.982 ± 0.002 | 0.8 | 2.57 ± 0.06 | ... |
| B | 218/74 |
|
|
>1.0 |
|
... | |
| IRAS 07380-2342 | A | 22/76 | 213 ± 12 | 0.988 ± 0.006 | 0.8 | 0.49 ± 0.05 | ... |
| B | 16/75 |
|
0.990 ± 0.009 |
|
< 0.3 | ... | |
| IRAS 09104+4109* | A | 44/69 | 176 ± 3 | 0.995 ± 0.002 | 0.8 | 0.69 ± 0.02 | [NeVI] emission line g |
| B | 26/68 | 104 ± 11 | 0.996 ± 0.004 | 1.65 ± 0.17 | 0.16 ± 0.10 | [NeVI] emission lineg | |
| IRAS F10026+4949 | A | 19/88 |
|
>0.988 | 0.8 |
|
... |
| B | 19/87 | 150 ± 60 | >0.992 |
|
|
... | |
| IRAS F12509+3122 | A | 51/85 |
|
|
0.8 | < 0.04 | ... |
| B | 51/84 | 25 ± 6 |
|
|
< 0.2 | ... | |
| IRAS 12514+1027 | A | 116/73 | 57.4 ± 1.0 | 0.958 ± 0.003 | 0.8 | < 0.02 | [NeVI] emission line g |
| B | 114/72 | 57 ± 7 | 0.956 ± 0.004 |
|
< 0.12 | [NeVI] emission lineg | |
| IRAS 14026+4341 | A | 33/75 | 75 ± 2 | 0.977 ± 0.004 | 0.8 | 0.06 ± 0.02 | ... |
| B | 31/74 |
|
0.978 ± 0.004 |
|
< 0.18 | ... | |
| IRAS F15307+3252 | A | 238/84 | 38 ± 2 | 0.981 ± 0.004 | 0.8 | 0.64 ± 0.04 | ... |
| B | 173/83 |
|
0.975 ± 0.006 | >1.4 |
|
... | |
| IRAS F16124+3241 | A | 38/78 | 6.6 ± 1.3 |
|
0.8 | 1.3 ± 0.2 | ... |
| B | 38/77 | 7 ± 4 |
|
|
|
... | |
| ELAIS J1640+41 | A | 33/88 | 17.3 ± 1.1 | 0.993 ± 0.006 | 0.8 | 0.13 ± 0.06 | ... |
| B | 32/87 |
|
>0.988 |
|
< 0.4 | ... | |
| IRAS 18216+6418 | A | 117/77 |
|
>0.999 | 0.8 | < 0.001 | ... |
| A | 18/76 |
|
|
< 0.4 | < 0.17 | ... | |
HLIRG emission model (A: AGN power law slope fixed at 0.8; B: AGN power law slope allowed to vary between 0.2 and 1.8). See Sect. 4.1 for a complete discussion of the adopted model. The best-fit model is shown in boldface.
Emission line at 7.65 μm. See Sect 4.2 for a discussion about these spectral features.
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