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Table B.1:

X-ray properties and radio luminosity of the whole GPS sample discussed in this paper (Sects. 5 and 6).
Source name $\log (L_{\rm 5 \ GHz}, {\rm erg \ s^{-1}})$ $L_{{\rm 2-10 \ keV}}$ $N_{\rm H}$ Size HI $\log(N_{\rm H}, {\rm cm}^{-2}$) $\Gamma $
    (1043 erg s-1) (1020 cm-2) (kpc)    
4C+00.02 43.1 0.55$^{\dag }$ <10000 0.220 ... ...
COINSJ0111+3906 44.0 $7 \pm 3$ >500 0.033 21.9 ...
PKS0428+20 43.1 $1.4 \pm 0.6$ <70 0.653 20.5 ...
PKS0500+019 43.6 $50 \pm 6$ $50 \pm^{18}_{16}$ 0.055 20.8 $1.61\pm^{0.16}_{0.15}$
B30710+439 43.8 $34.0 \pm 0.2$ $51 \pm^{17}_{14}$ 0.118 ... $1.59\pm0.06$
PKS0941-080 42.8 $0.091 \pm 0.075$ <10000 0.148 <20.1 ...
B1031+567 43.4 $2.2 \pm 0.2$ $50 \pm 18$ 0.206 <20.1 ...
4C+14.41 43.2 $1.40 \pm 0.19$ <16 0.306 <19.8 ...
4C+32.44 43.6 $3.7 \pm 0.4$ $12 \pm^6_5$ 0.247 19.9 $1.7 \pm 0.2$
PKS1345+125 42.7 $7.8 \pm 1.5$ $480 \pm 40$ 0.166 20.6 $1.1\pm^{0.7}_{0.8}$
4C+62.22 43.6 $30 \pm 20$ $290 \pm^{200}_{100}$ 0.218 20.3 $1.24\pm0.17$
OQ+208 42.2 >9.0 >9000 0.010 20.3 $2.21\pm^{0.19}_{0.14}$
PKS1607+26 43.8 $29.0 \pm 0.1$ >6000 0.262 ... ...
PKS2008-068 44.5 $ 6 \pm 2$ <50 0.218 ... ...
PKS2127+04 44.6 $29 \pm 4$ <19 0.218 ... $2.0\pm^{0.5}_{0.4}$
COINSJ2355+4950 43.0 $1.3 \pm 0.3$ $400 \pm^{700}_{300}$ 0.199 20.5 $1.8\pm^{1.6}_{0.9}$

$^{\dag }$ Extrapolated from the detection in the 0.5-2 keV band with $\Gamma = 1.61$ and $N_{\rm H} = N_{\rm H,~Gal}$.


Source LaTeX | All tables | In the text

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