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Fig. A.1.

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Comparison of the Fe II spectrum from our source with the best χ2 solutions employing the first three ratios (Section 3.3) in the computation. Top: Fe II spectrum assuming equal contribution from bright and dark sides, displayed with a 24% covering factor. The Fe II template corresponds to the CLOUDY simulation with logΦ(H) = 19.25 cm−2 s−1, log(Ptot) = 14 cm−3 K, Z = 20Z and Vturb = 40 km s−1. Bottom: Fe II spectrum assuming a 20% contribution from bright sides and 80% contribution from dark sides, displayed with a 33% covering factor. The Fe II template corresponds to the CLOUDY simulation associated with logΦ(H) = 19.75 cm−2 s−1, log(Ptot) = 15.50 cm−3 K, Z = 20Z and Vturb = 100 km s−1.

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