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Table 1.

Emission line constraints for an Lopt = 1043 erg s−1 source.

RPC model
mRPC model
Emission line EW RBLR Baldwin EW RBLR EW RBLR
(Å) (light-days) (index) (Å) (light-days) (Å) (light-days)
Paβ 40 ± 20 0.0 160 11 120 9
Hα 390 ± 120 15 ± 6 0.0 250 13 180 9
Hβ 80 ± 20 10 ± 2 0.0 100 11 65 8
He II λ4686 18 ± 4 2 ± 1 −0.2 17 7 5 6
C III]+Si III] ∼ λ1900 45 ± 15 6 ± 2 −0.1 12 12 27 9
N III] λ1750 8 ± 3 −0.1 32 10 24 7
He II λ1640 22 ± 5 2 ± 1 −0.2 22 7 20 6
C IV λ1548 160 ± 30 3 ± 1 −0.2 190 9 100 7
Si IV+O IV] ∼ λ1400 20 ± 5 3 ± 1 −0.1 29 9 19 7
Lyα 170 ± 40 3 ± 1 −0.1 100 12 63 8
O VI λ1035 80 ± 40 −0.2 120 9 100 7
O VIII λ18.97 0.05 ± 0.02 0.1 6 0.06 6
Fe Kαλ1.93 0.07 ± 0.01 −0.2 0.03 6 0.01 6

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