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Table B.3

Fits of best Cloudy model to dereddend spectrum.

Ion Wavelength (Å) Fobsa Fmodela log L χ2
TOTL 1240 7.20 13.93 36.65 3.5
C 2 1335 0.27 0.01 33.63 3.6
TOTL 1402 3.50 2.30 35.87 0.5
TOTL 1486 7.50 7.45 36.38 0.0
TOTL 1549 2.50 2.47 35.90 0.0
Ne 5 1575 0.50 0.90 35.46 2.5
Ne 4 1602 2.30 4.81 36.19 4.8
He 2 1640 1.30 5.47 36.24 41.1
TOTL 1665 2.10 0.25 34.91 3.1
TOTL 1750 6.60 0.30 34.98 3.6
TOTL 1909 1.70 0.14 34.66 3.4
O 3 2321 0.07 0.09 34.49 0.5
Ne 4 2423 0.50 0.00 0.00 4.0
Mg 2 2803 11.30 0.01 33.69 4.0
Ne 3 3869 6.20 5.59 36.25 0.0
Ne 3 3968 1.90 1.68 35.73 0.1
H 1 4102 0.68 0.28 34.96 1.4
H 1 4340 0.50 0.49 35.20 0.0
TOTL 4363 1.80 0.42 35.13 2.3
He 1 4471 0.08 0.02 33.78 2.3
H 1 4861 1.00 1.00 35.51 0.0
O 3 4959 0.83 1.21 35.59 0.9
O 3 5007 2.60 3.65 36.07 0.7
Fe 6 5177 0.08 0.09 34.45 0.1
N 2 5755 0.12 0.00 32.12 4.0
He 1 5876 0.17 0.05 34.23 1.9
Fe 7 6087 0.06 0.22 34.85 32.0
O 1 6300 0.05 0.00 27.35 4.0
H 1 6563 2.80 3.00 35.98 0.0
He 1 7065 0.12 0.05 34.16 1.6

Notes.

(a)

Normalized to dereddened Hβ flux, 4.01 × 10-10 erg s-1 cm-2 for E(B − V) = 0.85 (see Sect. 4.2).

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