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Table 4:

Fit parameters, estimated thermal excess, and ratio of ionization to mid-infrared emission strength.

Source
A $\chi^2$ $\log{{\rm MIR}_{\rm excess}}$ $\log{\frac{L_{[\mbox{\scriptsize O {\sc iii}}]}}{L_{{\rm 11.85}~\mu{\rm m}}}}$
      ( ${\rm erg}~{\rm s}^{-1}$)  
(1) (2) (3) (4) (5)
4C 12.03 $\dots$ $\dots$ <1.2 >-2.7
3C 015 -5.26 5.71 <1.2 >-2.5
3C 029 -2.05 0.14 <0.5 >-2.7
3C 040 -2.89 0.03 0.0 $\dots$
3C 078 -3.38 0.25 0.0 $\dots$
Fornax A -2.50 3.96 <1.0 $\dots$
3C 093 $\dots$ $\dots$ <1.7 $\dots$
3C 098 -1.57 1.01 2.0 -2.0
3C 105 -2.93 0.12 <1.0 >-2.1
3C 120 $\dots$ $\dots$ 0.4 -2.4
3C 135 $\dots$ $\dots$ <1.8 >-1.5
Pictor A -1.86 0.19 0.2 -2.4
3C 198 -2.72 10.4 <1.9 >-2.0
3C 227 -6.18 2.51 1.7 -2.2
3C 270 -1.35 12.4 0.0 >-1.8
Centaurus A -1.89 0.50 0.0 -3.4
PKS1417-19 $\dots$ $\dots$ 2.2 $\dots$
3C 317 -2.53 0.69 0.0 >-2.2
3C 327 $\dots$ $\dots$ 2.0 -2.5
3C 353 -1.83 2.73 0.0 >-3.0
PKS1839-48 $\dots$ $\dots$ 0.0 $\dots$
3C 403 -4.32 1.78 2.7 -2.6
3C 403.1 $\dots$ $\dots$ $\dots$ $\dots$
3C 424 $\dots$ $\dots$ <1.0 >-2.8
PKS2158-380 $\dots$ $\dots$ 2.0 $\dots$
3C 445 $\dots$ $\dots$ 2.2 -2.5
PKS2354-35 $\dots$ $\dots$ <1.2 >-2.2

Notes.  Column (2) The fitted curvature of the parabola. Column (3) Goodness of fit parameter, reduced $\chi^2$-value, of the parabolic fit to the core spectral energy distribution data ranging from the radio to UV. Column (4) Logarithm of the thermal excess above the synchrotron fit. Column (5) Logarithm of [O III] ionization over mid-infrared emission strength.


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