Table 2: Radio-excess galaxies found using the radio-FIR correlation.

CIG		 $\log L_{{\rm FIR}}^{1}$ Code2 $\log L_{1.4~{\rm GHz}}^{3}$ T4 Excess factor5
Galaxies belonging to the complete subsample
41 9.67 0 22.07 Sc 5.7
72 9.72 1 21.91 Sbc 3.6
97 10.19 0 22.47 Sc 4.3
156 9.41 0 21.74 SBab 5.0
187 9.83 0 23.17 Sc 50.2
248 10.40 0 22.60 Sc: 3.5
287 9.97 0 22.39 SBbc 6.0
480 9.48 0 21.65 S0a 3.4
488 10.50 1 22.72 Sb 3.7
571 8.93 0 21.39 Sc 6.9
591 9.46 1 21.39 Sbc 4.1
692 10.33 0 22.67 Sb 4.9
734 8.79 1 21.05 S0a 4.4
877 10.40 0 22.66 E: 4.0
893 10.69 1 22.87 E/S0 3.4
1045 8.78 1 21.92 S0 19.7
Galaxies not belonging to the complete subsample
57 10.23 1 22.73 Sb 5.6
510 9.42 1 21.61 Sc 3.6
836 10.17 1 23.29 E/S0 29.7
999 9.90 0 22.09 Sa 3.5
$^{\rm 1}$ $\log L_{{\rm FIR}}$ from Lisenfeld et al. (2007); $^{\rm 2}$ detection code for $\log L_{{\rm FIR}}$: 0 for detections and 1 for upper limits; $^{\rm 3}$ $\log L_{1.4~{\rm GHz}}$ from Leon et al. (2008); $^{\rm 4}$ morphological type from Sulentic et al. (2006), except for CIG 999 (Karachentseva 1973, NED); $^{\rm 5}$ radio luminosity excess above the radio-FIR correlation.

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