Low redshift AGN in the Hamburg/ESO survey - I. The local AGN luminosity function

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Table 2:

Binned differential luminosity function in the B_J band, corrected for evolution.
M_{B_J}	N	$\log \Phi(M_{B_J})$	$\sigma(\log \Phi)$
-18.0	1	-5.81	+0.3	$-\infty$
-18.5	6	-5.30	+0.15	-0.24
-19.0	5	-5.72	+0.17	-0.26
-19.5	28	-5.22	+0.08	-0.09
-20.0	30	-5.54	+0.08	-0.09
-20.5	37	-5.74	+0.07	-0.08
-21.0	40	-6.03	+0.07	-0.07
-21.5	23	-6.62	+0.09	-0.10
-22.0	24	-6.95	+0.08	-0.10
-22.5	40	-7.04	+0.06	-0.08
-23.0	38	-7.40	+0.07	-0.08
-23.5	31	-7.65	+0.08	-0.08
-24.0	14	-8.04	+0.10	-0.13
-24.5	9	-8.25	+0.13	-0.17
-25.5	2	-8.91	+0.23	-0.53
-26.0	1	-9.21	+0.3	$-\infty$

N is the number of objects contributing per bin. The luminosity function is expressed as number density per Mpc³ per unit magnitude.

Source LaTeX | All tables | In the text

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