JADES - The diverse population of infant black holes at 4 < z < 11: Merging, tiny, poor, but mighty

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Table 4.

Density of broad-line AGNs at 4 < z < 6 with L_bol > 10⁴⁴ as a function of absolute UV magnitude.

M_UV1	log Φ	log Φ_min
[mag]	[Mpc⁻³ mag⁻¹]
−18.0 ± 0.75	$- 3 . 06_{- 0.26}^{+ 0.18}$ $-3.06_{-0.26}^{+0.18}$	> − 5.73
−19.5 ± 0.75	$- 3 . 83_{- 0.44}^{+ 0.23}$ $-3.83_{-0.44}^{+0.23}$	> − 5.98

Notes. The last column gives the minimum density assuming the most conservative and extreme case that the AGNs identified in the spectroscopic survey are the only AGN in the volume sampled.

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