Table 4
Physical parameters estimated from the SED fitting.
| Object | L AGN | L SF | SFR | M d | T d |
| (1012L⊙) | (1012L⊙) | (102M⊙ yr-1) | (108M⊙) | (K) | |
| (1) | (2) | (3) | (4) | (5) | (6) |
|
|
|||||
| 3C 002 |
|
|
|
|
|
| 3C 014 |
|
|
|
|
|
| 3C 068.2 |
|
|
|
|
|
| 3C 119a |
|
|
|
|
|
| 3C 124 |
|
|
|
|
|
| 3C 190 |
|
|
|
|
|
| 3C 205 |
|
|
|
|
|
| 3C 222 |
|
|
|
|
|
| 3C 245 |
|
|
|
|
|
| 3C 256 |
|
|
|
|
|
| 3C 257a,d |
|
|
|
|
|
| 3C 266 |
|
|
|
|
|
| 3C 270.1 |
|
|
|
|
|
| 3C 297 |
|
|
|
|
|
| 3C 298d |
|
|
|
|
|
| 3C 305.1a |
|
|
|
|
|
| 3C 318 |
|
|
|
|
|
| 3C 324 |
|
|
|
|
|
| 3C 368d |
|
|
|
|
|
| 3C 432d |
|
|
|
|
|
| 3C 454.0 |
|
|
|
|
|
| 3C 454.1 |
|
|
|
|
|
| 3C 470d |
|
|
|
|
|
|
|
|||||
| Objects detected in fewer than three Herschel bands | |||||
|
|
|||||
| 3C 009 | 17.1 | <1.8 | <3.1 | ||
| 3C 013 | 4.0 | <1.2 | <2.0 | ||
| 3C 036a,b | <1.2 | <0.5 | <0.9 | ||
| 3C 043 | 2.8 | <1.2 | <2.0 | ||
| 3C 065a,b | <1.4 | <0.6 | <1.0 | ||
| 3C 068.1c | 8.6 | <0.7 | <1.1 | ||
| 3C 173b | 0.4 | <0.3 | <0.5 | ||
| 3C 181c | 5.2 | <0.8 | <1.5 | ||
| 3C 186c | 4.7 | <0.5 | <0.8 | ||
| 3C 191 | 17.0 | <1.7 | <3.0 | ||
| 3C 194b | <0.7 | <0.6 | <0.9 | ||
| 3C 204c | <4.8 | <0.5 | <0.9 | ||
| 3C 208.0 | <3.6 | <0.6 | <1.0 | ||
| 3C 208.1a | <1.6 | <0.4 | <0.7 | ||
| 3C 210a | 5.2 | <1.9 | <3.3 | ||
| 3C 212 | 6.2 | <0.8 | <1.3 | ||
| 3C 220.2 | 6.3 | <0.7 | <1.2 | ||
| 3C 225Ab | <1.5 | <1.8 | <3.1 | ||
| 3C 230 | 3.1 | <1.9 | <3.3 | ||
| 3C 238b | <0.7 | <0.5 | <0.9 | ||
| 3C 239b | <3.0 | <1.7 | <2.9 | ||
| 3C 241b | 2.1 | <0.8 | <1.4 | ||
| 3C 249b | <0.9 | <0.8 | <1.5 | ||
| 3C 250 | <0.6 | <0.5 | <0.9 | ||
| 3C 252a | 4.5 | <0.6 | <1.0 | ||
| 3C 255b | <0.5 | <0.5 | <0.9 | ||
| 3C 267a | 3.1 | <0.4 | <0.7 | ||
| 3C 268.4 | 16.2 | <0.8 | <1.4 | ||
| 3C 280.1c | <5.4 | <1.1 | <1.9 | ||
| 3C 294b | <2.3 | <1.7 | <2.9 | ||
| 3C 322 | <1.5 | <1.3 | <2.2 | ||
| 3C 325 | <2.5 | <0.7 | <1.2 | ||
| 3C 326.1 | <3.7 | <3.0 | <5.2 | ||
| 3C 356 | 1.9 | <0.8 | <1.3 | ||
| 3C 437b | <1.6 | <1.2 | <2.1 | ||
| 3C 469.1a | 3.3 | <1.3 | <2.2 | ||
| 4C 13.66 | <1.0 | <0.8 | <1.4 | ||
| 4C 16.49c | <2.4 | <0.9 | <1.5 | ||
Notes. (1) Name of object; (2) IR luminosity (integrated between 1 μm and 1000 μm) of the AGN powered dust emission, i.e. torus component and sum of torus and hot dust components for RGs and QSRs, respectively; (3) IR luminosity (integrated between 8 μm and 1000 μm) of the modified blackbody component (β = 1.6) presumably powered by star formation activity in the AGN host galaxy; (4) star formation rate determined from the IR luminosity in (3), using the calibration derived in Kennicutt (1998); (5) mass of the modified blackbody component; (6) temperature of the modified blackbody component.
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