Table 2: The Chandra/ 2dFGRS correlation sample. Column details are as in the previous figure.
ID Name $\alpha_{\rm X}$ $\delta_{\rm X}$ $\delta_{\rm XO}$ $b_{\rm J}$ $f_{\rm X}/10^{-14}$ z log $L_{\rm X}$ $\log (f_{\rm X}/f_{\rm O})$ HR $\pm$ Type
    (J2000) (J2000) ( $^{\prime\prime}$)   (cgs)   (cgs)        
1 TGS432Z052 23 58 27.21 -32 41 03.3 0.23 19.20 6.36 0.2394 42.99 -0.50 +0.39 0.04 AGN1
2 TGS522Z150 02 57 14.04 -33 18 27.5 0.82 17.93 1.84 0.1093 41.72 -1.54 +0.23 0.11 AGN1
3 TGS212Z026 00 58 24.51 -27 29 23.2 0.78 16.83 0.36 0.0977 40.91 -2.70 -0.63 0.24 H II?
4 TGS211Z082 00 56 51.78 -27 28 56.3 1.44 18.90 4.22 0.2144 42.71 -0.80 +0.61 0.11 AGN1
5 TGS243Z005 03 32 46.89 -27 42 13.3 2.52 17.53 0.39 0.1028 41.00 -2.38 -0.54 0.12 A
6 TGS407Z114 22 01 36.09 -31 53 23.2 1.63 18.06 1.63 0.0972 41.56 -1.55 +0.24 0.03 AGN1
7 TGS132Z150 23 51 39.38 -26 05 02.5 2.90 18.00 9.17 0.2346 43.13 -0.82 -0.61 0.01 LINER?
8 TGN163Z121 10 56 50.04 -03 33 42.8 1.10 17.69 0.69 0.0488 40.56 -2.07 -0.56 0.07 A (noisy)
9 TGN163Z123 10 56 48.84 -03 37 25.8 0.73 18.54 0.41 0.1816 41.55 -1.96 -0.78 0.10 A
10 TGN071Z177 12 49 02.23 -05 49 33.8 1.43 18.34 0.60 0.0485 40.50 -1.87 -0.32 0.08 H II?
11 TGN206Z127 14 12 49.69 -03 07 19.7 2.59 18.09 0.94 0.0748 41.08 -1.77 -0.43 0.13 AGN?
12 TGN440Z057 11 23 20.17 +01 38 09.9 1.84 18.66 0.07 0.1259 40.47 -2.66 -0.68 0.25 A
13 TGN382Z123 12 04 27.15 +01 53 46.2 2.69 14.25 3.10 0.0197 40.42 -2.79 -0.80 0.01 A
14 TGN243Z240 11 55 45.38 -01 41 30.3 0.70 19.00 1.79 0.2476 42.48 -1.13 -0.57 0.08 LINER?
15 TGN247Z076 12 16 01.62 -00 37 33.6 0.46 17.70 0.25 0.1214 40.98 -2.50 -1.00 0.24 A
16 TGN318Z209 12 15 53.29 -00 36 06.9 1.71 18.00 0.23 0.1193 40.90 -2.42 -0.39 0.21 A
17 TGN336Z169 13 44 52.88 +00 05 20.4 0.81 17.38 77.8 0.0876 43.14 -0.14 -0.63 0.02 AGN?2
18 TGN336Z187 13 44 28.34 +00 01 47.2 0.71 18.12 0.56 0.1351 41.43 -1.98 -1.00 0.48 A
19 TGN275Z203 14 12 34.68 -00 35 00.1 0.49 18.16 30.4 0.1269 43.09 -0.24 -0.74 0.07 AGN?3
20 TGS906Z501 23 25 19.74 -12 07 26.2 1.77 15.89 4.94 0.0824 41.89 -1.93 -0.64 0.002 LINER?

1: Obscured AGN suggested by high $N_{\rm H}$ value.
2: Suggested by an H$\beta$ FWHM $\sim $ 2000 km s-1.
3: Suggested by an H$\beta$ FWHM $\sim $ 1500 km s-1.


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