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Table 3
Fit results for various AGN luminosity relations.
| Relation | Intercept type 1 | Slope type 1 | Intercept type 2 | Slope type 2 | K-S distance | K-S prob |
|
|
||||||
| Type 1i treated as type 1 | ||||||
| NIR–MIR |
|
|
|
|
0.854 | 2.5e-05 |
| NIR–X-rays |
|
|
|
|
0.875 | 2.5e-05 |
| X-rays–MIR |
|
|
|
|
0.449 | 1.0e-01 |
| OIV–MIR |
|
|
|
|
0.292 | 5.9e-01 |
| OIV–X-ray |
|
|
|
|
0.286 | 6.5e-01 |
|
|
||||||
| Type 1i treated as type 2 | ||||||
| NIR–MIR |
|
|
|
|
0.610 | 7.3e-03 |
| NIR–X-rays |
|
|
|
|
0.722 | 9.2e-04 |
| X-rays–MIR |
|
|
|
|
0.375 | 2.5e-01 |
| OIV–MIR |
|
|
|
|
0.340 | 4.3e-01 |
| OIV–X-ray |
|
|
|
|
0.422 | 2.0e-01 |
Notes. The intercept and slope for e.g. the NIR–MIR relation is defined as: 
= intercept + slope 
. For each relation, the K-S test is computed from the ratio of luminosities for type 1 vs. type 2 AGNs.
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