Table 1: Summary of best-fit clustering parameters.
Sample Na z range $\bar z^b$ ${\rm log}L_{0.5-10}^c$ r0       $\gamma $ $r_0(\gamma=1.8)$
          [h-1 Mpc]   [h-1 Mpc]

All AGN
538 0.2-3.0 0.98 43.8 $\rm 8.65^{+0.41}_{-0.48} $ $\rm 1.88^{+0.06}_{-0.07}$ $\rm 8.39^{+0.41}_{-0.39}$
No z=0.36 spike 496 0.2-3.0 1.03 43.9 $\rm 6.12^{+0.64}_{-0.89} $ $\rm 1.74^{+0.13}_{-0.14}$ $\rm 6.32^{+0.53}_{-0.49}$
$z\sim 1$ AGN 349 0.4-1.6 0.94 43.7 $\rm 5.17^{+0.80}_{-1.14} $ $\rm 1.72^{+0.17}_{-0.18}$ $\rm 5.44^{+0.62}_{-0.58}$
BLAGN 305 0.2-3.0 1.45 44.3 $\rm 7.66^{+0.81}_{-1.04} $ $\rm 1.98^{+0.17}_{-0.18}$ $\rm 7.03^{+0.96}_{-0.89}$
non-BLAGN 229 0.2-1.3 0.70 43.2 $\rm 7.03^{+0.87}_{-1.18} $ $\rm 1.60^{+0.13}_{-0.14}$ $\rm 7.75^{+0.62}_{-0.59}$
$\rm HR<-0.2$ 428 0.2-3.0 1.15 44.0 $\rm 9.56^{+0.42}_{-0.45} $ $\rm 1.98^{+0.08}_{-0.07}$ $\rm 9.05^{+0.48}_{-0.45}$
${\rm HR}<-0.2,~z<1.3$ 250 0.2-1.3 0.79 43.5 $\rm 9.96^{+0.48}_{-0.50}$ $\rm 1.93^{+0.07}_{-0.07}$ $\rm 9.68^{+0.48}_{-0.50}$
$\rm HR<-0.2$, no spike 218 0.2-1.3 0.79 43.5 $\rm 6.72^{+0.72}_{-0.88}$ $\rm 1.87^{+0.18}_{-0.18}$ $\rm 6.56^{+0.75}_{-0.68}$
$\rm HR\geq -0.2$ 102 0.2-1.3 0.73 43.4 $\rm 5.07^{+1.58}_{-1.73} $ $\rm 2.38^{+0.85}_{-0.51}$ $\rm 4.97^{+1.93}_{-1.49}$
z<1 276 0.2-1.0 0.68 43.3 $\rm 7.97^{+0.48}_{-0.52} $ $\rm 1.80^{+0.08}_{-0.08}$ $\rm 7.97^{+0.43}_{-0.41}$
z<1 no spike 234 0.2-1.0 0.73 43.4 $\rm 5.16^{+0.71}_{-0.99} $ $\rm 1.81^{+0.20}_{-0.21}$ $\rm 5.14^{+0.66}_{-0.61}$
z>1 262 1.0-3.0 1.53 44.3 $\rm 6.68^{+1.19}_{-1.98} $ $\rm 1.86^{+0.27}_{-0.30}$ $\rm 6.40^{+0.94}_{-0.86}$
a Number of objects in each sample. b Median redshift. c Median X-ray luminosity in the 0.5-10 keV band in units of erg s-1. Errors are $1\sigma $ Poisson confidence levels. Bootstrap errors are a factor of $\sim $2 larger.


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