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Table 5:

Combined binned local AGNLF, based on the SDSS broad line galaxy sample (faint end) and the Hamburg/ESO Survey (bright end).
MB $\log \Phi(M_B)$ $\log L_{\rm Bol}$ $\log \Phi(L_{\rm Bol})$
-14.2 $\rm -2.60^{+0.11}_{-0.14}$ 42.63 $\rm -2.12^{+0.10}_{-0.15}$
-14.8 $\rm -2.95^{+0.12}_{-0.18}$ 42.83 $\rm -2.48^{+0.13}_{-0.18}$
-15.4 $\rm -3.00^{+0.08}_{-0.09}$ 43.03 $\rm -2.52^{+0.07}_{-0.1}$
-16.0 $\rm -3.49^{+0.07}_{-0.09}$ 43.24 $\rm -3.02^{+0.07}_{-0.09}$
-16.6 $\rm -3.63^{+0.08}_{-0.10}$ 43.44 $\rm -3.16^{+0.07}_{-0.10}$
-17.2 $\rm -4.10^{+0.08}_{-0.09}$ 43.65 $\rm -3.64^{+0.08}_{-0.08}$
-17.8 $\rm -4.26^{+0.08}_{-0.08}$ 43.86 $\rm -3.80^{+0.07}_{-0.08}$
-18.4 $\rm -4.44^{+0.08}_{-0.09}$ 44.07 $\rm -3.98^{+0.07}_{-0.10}$
-19.0 $\rm -4.69^{+0.07}_{-0.10}$ 44.28 $\rm -4.24^{+0.07}_{-0.10}$
-19.6 $\rm -5.04^{+0.09}_{-0.10}$ 44.49 $\rm -4.59^{+0.08}_{-0.10}$
-20.2 $\rm -5.46^{+0.06}_{-0.08}$ 44.71 $\rm -5.02^{+0.06}_{-0.08}$
-20.8 $\rm -5.78^{+0.07}_{-0.08}$ 44.93 $\rm -5.34^{+0.06}_{-0.08}$
-21.4 $\rm -6.36^{+0.09}_{-0.12}$ 45.15 $\rm -5.93^{+0.10}_{-0.11}$
-22.0 $\rm -6.85^{+0.09}_{-0.11}$ 45.38 $\rm -6.42^{+0.09}_{-0.11}$
-22.6 $\rm -7.19^{+0.08}_{-0.10}$ 45.60 $\rm -6.77^{+0.09}_{-0.10}$
-23.2 $\rm -7.40^{+0.08}_{-0.09}$ 45.82 $\rm -6.98^{+0.08}_{-0.09}$
-23.8 $\rm -7.87^{+0.10}_{-0.11}$ 46.05 $\rm -7.45^{+0.10}_{-0.11}$
-24.4 $\rm -8.20^{+0.12}_{-0.16}$ 46.28 $\rm -7.78^{+0.12}_{-0.17}$
-25.0 $\rm -8.76^{+0.20}_{-0.37}$ 46.51 $\rm -8.34^{+0.19}_{-0.38}$

The bolometric AGNLF has been computed using the bolometric corrections by Marconi et al. (2004).


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