Table 2.
Best-fit parameters for popular AGN SED templates.
| AFeII | Alines | Wline | β | λbend | Wbend | βUV | EB − V | EB − VAGN | Si | fcov | λcool | Wcool | λhot | Whot | fhot | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| log | log | log | log | log | log | log | log | log | ||||||||
| Template | (km/s) | (nm) | (dex) | (mag) | (mag) | (μm) | (dex) | (μm) | (dex) | |||||||
| Elvis-1994 | 1.8 | −0.5 | 3.6 | −2.7 | 1.7 | 0.2 | 1.9 | −2.0 | −2.0 | 0.1 | 0.6 | 14.0 | 0.4 | 2.5 | 0.5 | 1.1 |
| Lyu-2017-WDD | 0.6 | −0.5 | 3.5 | −2.3 | 2.0 | −1.4 | 0.3 | −2.0 | −1.2 | −0.4 | 0.2 | 18.8 | 0.3 | 2.4 | 0.5 | 3.1 |
| Lyu-2017-HDD | 1.9 | −0.5 | 3.6 | −2.6 | 2.1 | −1.2 | −0.5 | −1.2 | −1.7 | −0.5 | 0.2 | 16.0 | 0.5 | 1.8 | 0.6 | 6.3 |
| Mullaney-2011 | – | – | – | – | – | – | – | – | –1.8 | –0.7 | 0.6 | 14.7 | 0.4 | 2.5 | 0.5 | 0.3 |
Notes. Only AGN shape parameters are shown. The first row represents an average AGN, while the next two rows represent warm- and hot-dust-deficient sub-populations. These differ in the torus properties listed in the last six columns, which give the covering factors and log-quadratic shape parameters of the cool and hot components. The last row is an AGN torus template starting at 6 μm, therefore the first columns are blanked out.
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