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Table 1:

Basic parameters of the observed sample.

Source 		z Class Ref. $\log{\nu L^{{\rm total}}_{{\rm 408~MHz}}}$ $\log{R}$ Freq. Ref. $\frac{[\mbox{O {\sc iii}}]}{[\mbox{O {\sc ii}}]}$ $\frac{[\mbox{O {\sc iii}}]}{[{\rm H}\beta]}$ $\log{\nu L_{[\mbox{\scriptsize O {\sc iii}}]}}$ Ref. VISIR
                        Resolution
        (erg s-1)   (GHz)       (erg s-1)   (parsec)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
4C12.03 0.15600 LEG 5 41.98 -2.66 1.5 5 $\dots$ $\dots$ 40.9 7 1400
3C 015 0.07300 LEG 8 41.64 -2.02 2.3 6 $\dots$ 3.7 40.4 6 610
3C 029 0.04503 FR-I 8 41.26 -1.79 2.3 6 $\dots$ 1.7 39.9 6 370
3C 040 0.01800 FR-I 8 40.63 -1.61 2.3 6 $\dots$ $\dots$ <38.9 6 140
3C 078 0.02865 FR-I 8 40.94 -0.92 2.3 6 $\dots$ $\dots$ <39.1 6 230
Fornax A 0.00587 FR-I 8 40.72 -3.40 2.3 6 $\dots$ $\dots$ <38.6 6 40
3C 093 0.35700 BLRG 6 43.02 -2.38 5.0 2,7 3.9 $\dots$ $\dots$ 3 3500
3C 098 0.03045 HEG 5 41.31 -2.70 8.3 4 2.9 15 40.9 1 240
3C 105 0.08900 HEG 8 41.80 -2.27 2.3 6 $\dots$ 16 40.8 6 750
3C 120 0.03301 BLRG 8 40.73 1.01 2.3 6 5.7 $\dots$ 41.8 6 270
3C 135 0.12738 HEG 5 42.05 -2.71 8.3 3 $\dots$ $\dots$ 42.0 9 1100
Pictor A 0.03506 BLRG 8 42.22 -1.57 2.3 6 1.8 4.2 41.2 6 280
3C 198 0.08147 HEG 3 41.56 -2.20 5.0 1, 7 1.2 2.1 41.1 8 680
3C 227 0.08583 BLRG 8 42.13 -2.55 2.3 6 13 9.0 41.8 6 710
3C 270 0.00746 FR-I 8 40.21 -1.71 2.3 6 $\dots$ 4.7 38.9 2,10 55
Centaurus A 0.00095 FR-I 8 40.30 -1.35 2.3 6 2.5 6.3 38.3 5, 6 7
PKS1417-19 0.12000 BLRG 4 41.79 -2.20 5.0 7, 8 22 2.2 $\dots$ 4 1000
3C 317 0.03446 FR-I 8 41.38 -0.79 2.3 6 0.37 3.1 40.0 6 280
3C 327 0.10480 HEG 8 42.17 -2.19 2.3 6 12 15 42.1 6 890
3C 353 0.03042 LEG 8 42.01 -2.64 2.3 6 $\dots$ 0.92 39.3 6 240
PKS1839-48 0.11120 LEG 8 41.99 -1.16 2.3 6 $\dots$ $\dots$ <39.2 6 960
3C 403 0.05900 HEG 8 41.59 -2.18 2.3 6 8.4 20 41.6 6 490
3C 403.1 0.05540 LEG 7 41.04 $\dots$ $\dots$ $\dots$ $\dots$ $\dots$ $\dots$ $\dots$ 450
3C 424 0.12699 LEG 5 42.03 -1.70 8.3 3 $\dots$ $\dots$ 40.7 9 1100
PKS2158-380 0.03330 HEG 2 40.56 < -1.92 5.0 7, 9 $\dots$ $\dots$ $\dots$ $\dots$ 270
3C 445 0.05620 BLRG 8 41.66 -1.57 2.3 8 14 13 42.0 6 460
PKS2354-35 0.04905 FR-I 1 41.24 -1.16 5.0 7, 10 $\dots$ $\dots$ $\dots$ $\dots$ 400

Notes. Column (2) Redshifts are from the NED catalogue, except for Centaurus A, which is calculated from the distance from Rejkuba (2004). Column (3) Classifications: FR-I stands for Fanaroff-Riley class I radio galaxy, LEG and HEG for low- and high-excitation Fanaroff-Riley class II radio galaxy and BLRG for broad-line radio galaxy. Column (4) References to classifications: 1 = Burgess & Hunstead (2006), 2 = Baum et al. (1992), 3 = Black et al. (1992), 4 = Grandi & Osterbrock (1978), 5 = Hardcastle et al. (1998), 6 = Hes et al. (1996), 7 = Jackson & Rawlings (1997), and 8 = Morganti et al. (1997). Column (5) Integrated radio source luminosities, at rest 408 MHz from Wright & Otrupcek (1996). Columns (6-8) Radio core fraction, i.e. the ratio of the core to the extended radio flux at 1.5, 2.3, 5.0, or 8.0 GHz frequencies and references: 1 = Becker et al. (2003), 2 = Bogers et al. (1994), 3 = Hardcastle et al. (1998), 4 = Hardcastle et al. (1999), 5 = Leahy & Perley (1991), 6 = Morganti et al. (1997), 7 = Wright & Otrupcek (1996), 8 = Zirbel & Baum (1995), 9 = Fosbury et al. (1982), and 10 = Schwartz et al. (1991). Columns (9-12) Optical emission-line ratios of [O III] to [O II], [O III] to H$\beta$, and optical [O III] emission-line luminosities calculated from flux values found in the literature. References to emission-line ratios and fluxes: 1 = Costero & Osterbrock (1977), 2 = Ferrarese et al. (1996), 3 = Eracleous & Halpern (2003), 4 = Grandi & Osterbrock (1978), 5 = Hardcastle et al. (2007), 6 = Tadhunter et al. (1993), 7 = Wold et al. (2007), 8 = Simpson et al. (1996), 9 = Buttiglione et al. (2009), and 10 = Ho et al. (1997). Column (13) Scale of the VISIR mid-infrared diffraction-limit of $0.40\hbox{$^{\prime\prime}$ }$ in parsecs.


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