Table 3
Summary of the results of the spectral fitting.
| Model | N | N IRpl | N IRnon−pl | |||
| (1) | (2) | (3) | (4) | |||
|
|
||||||
| A: powerlaw | 45 | ( ) |
15 | ( ) |
30 | ( ) |
| B: zbbody + powerlaw | 13 | ( ) |
9 | ( ) |
4 | ( ) |
| C: zphabs × powerlaw | 69 | ( ) |
27 | ( ) |
42 | ( ) |
| D: zbbody + (zphabs × powerlaw) | 12 | ( ) |
5 | ( ) |
7 | ( ) |
| E: powerlaw + (zphabs × powerlaw) | 8 | () |
4 | ( ) |
4 | () |
Notes. (1) XSPEC model definition: power-law as a simple photon power-law; zphabs as a rest-frame photoelectric absorption; zbbody as a redshifted blackbody spectrum. All models include Galactic absorption (phabs). (2) Total number and fraction of best fitted AGN with the indicated model. (3) Number and fraction of IR power-law objects best fitted with the indicated model. (4) Number and fraction of IR non-power-law objects best fitted with the indicated model.
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