Best-fitting power-law parameters at z = 8–12 of the AGN UV luminosity function. The fitting model is described by equation (9).
z . | αL . | log ϕ⋆ . |
---|---|---|
8 | −2.45 ± 0.02 | −9.33 ± 0.04 |
9 | −2.36 ± 0.07 | −10.44 ± 0.09 |
10 | −2.35 ± 0.04 | −11.91 ± 0.07 |
11 | −2.02 ± 0.24 | −13.79 ± 0.33 |
12 | −2.43 ± 0.22 | −15.30 ± 0.28 |
z . | αL . | log ϕ⋆ . |
---|---|---|
8 | −2.45 ± 0.02 | −9.33 ± 0.04 |
9 | −2.36 ± 0.07 | −10.44 ± 0.09 |
10 | −2.35 ± 0.04 | −11.91 ± 0.07 |
11 | −2.02 ± 0.24 | −13.79 ± 0.33 |
12 | −2.43 ± 0.22 | −15.30 ± 0.28 |
Best-fitting power-law parameters at z = 8–12 of the AGN UV luminosity function. The fitting model is described by equation (9).
z . | αL . | log ϕ⋆ . |
---|---|---|
8 | −2.45 ± 0.02 | −9.33 ± 0.04 |
9 | −2.36 ± 0.07 | −10.44 ± 0.09 |
10 | −2.35 ± 0.04 | −11.91 ± 0.07 |
11 | −2.02 ± 0.24 | −13.79 ± 0.33 |
12 | −2.43 ± 0.22 | −15.30 ± 0.28 |
z . | αL . | log ϕ⋆ . |
---|---|---|
8 | −2.45 ± 0.02 | −9.33 ± 0.04 |
9 | −2.36 ± 0.07 | −10.44 ± 0.09 |
10 | −2.35 ± 0.04 | −11.91 ± 0.07 |
11 | −2.02 ± 0.24 | −13.79 ± 0.33 |
12 | −2.43 ± 0.22 | −15.30 ± 0.28 |
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