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Table A.4.

Emission-line parameters for the COS 2011 and COS 2013 spectra of NGC 3783.

COS 2011
 COS 2013
Feature λ0a Fluxb νsysc FWHMd Fluxb νsysc FWHMd
C III 1176.01 1.1 ± 0.2 −100 ± 80 1200 ± 180 1.5 ± 0.3 0 ± 50 1200 ± 260
Lyα 1215.67 110.0 ± 3.7 −110 ± 20 800 ± 20 100.0 ± 3.1 −40 ± 10 800 ± 20
Lyα 1215.67 150.0 ± 5.9 180 ± 20 2430 ± 30 170.0 ± 5.8 90 ± 10 2310 ± 10
Lyα 1215.67 260.0 ± 9.3 890 ± 60 5190 ± 60 77.0 ± 3.9 1760 ± 40 6070 ± 50
Lyα 1215.67 230.0 ± 7.6 −1160 ± 60 14870 ± 50 160.0 ± 5.3 200 ± 20 10590 ± 30
N V blue 1238.82 5.1 ± 0.3 −30 ± 30 770 ± 80 7.4 ± 0.3 −30 ± 10 770 ± 20
N V red 1242.80 5.1 ± 0.3 −30 ± 30 770 ± 80 7.4 ± 0.3 −30 ± 10 770 ± 20
N V blue 1238.82 6.0 ± 0.4 1080 ± 20 4240 ± 60 11.0 ± 0.5 580 ± 20 3690 ± 20
N V red 1242.80 6.0 ± 0.4 1080 ± 20 4240 ± 60 11.0 ± 0.5 580 ± 20 3690 ± 20
N V 1240.89 89.0 ± 3.0 480 ± 20 7270 ± 60 2.8 ± 0.4 450 ± 930 13100 ± 720
S II 1260.42 1.1 ± 0.5 −150 ± 20 1600 ± 40 6.4 ± 0.4 −150 ± 30 2460 ± 30
O I+S II 1304.46 11.0 ± 0.8 220 ± 20 2880 ± 100 11.0 ± 0.4 220 ± 20 2920 ± 30
C II 1334.53 4.3 ± 0.4 960 ± 50 2880 ± 100 4.0 ± 0.2 110 ± 30 2920 ± 30
S IV blue 1393.76 4.3 ± 0.4 −280 ± 30 1310 ± 100 3.6 ± 0.2 −70 ± 50 1260 ± 30
S IV red 1402.77 4.3 ± 0.4 −510 ± 90 1310 ± 20 3.6 ± 0.2 −70 ± 50 1260 ± 30
S IV blue 1393.76 19.0 ± 0.6 1060 ± 20 4740 ± 50 23.0 ± 1.3 −120 ± 10 5920 ± 100
S IV red 1402.77 19.0 ± 0.6 1060 ± 20 4740 ± 50 23.0 ± 1.3 −120 ± 10 5920 ± 100
S IV 1398.19 42.0 ± 1.4 −360 ± 50 10850 ± 50 15.0 ± 1.2 −3060 ± 70 17800 ± 50
O IV] 1401.16 1.8 ± 0.1 700 ± 40 1400 ± 130 2.1 ± 0.3 900 ± 40 1260 ± 10
O IV] 1401.16 11.0 ± 0.6 700 ± 40 4740 ± 20 1.9 ± 0.4 900 ± 40 5920 ± 10
N IV] 1486.50 0.0 ± 0.5 10 ± 30 5000 ± 190 0.7 ± 0.4 10 ± 20 500 ± 20
N IV] 1486.50 12.0 ± 0.5 −260 ± 20 2590 ± 60 9.5 ± 0.4 −260 ± 10 2590 ± 70
C IV blue 1548.19 40.0 ± 1.5 −60 ± 20 940 ± 20 37.0 ± 1.6 −60 ± 20 940 ± 10
C IV red 1550.77 40.0 ± 1.5 −60 ± 20 940 ± 20 37.0 ± 1.6 −60 ± 20 940 ± 10
C IV blue 1548.19 7.9 ± 0.8 300 ± 80 2840 ± 50 22.0 ± 1.6 500 ± 30 1390 ± 70
C IV red 1550.77 7.9 ± 0.8 300 ± 80 2840 ± 50 22.0 ± 1.6 500 ± 30 1390 ± 70
C IV blue 1548.19 140.0 ± 4.7 500 ± 20 4580 ± 20 68.0 ± 2.3 −620 ± 30 5030 ± 40
C IV red 1550.77 140.0 ± 4.7 500 ± 20 4580 ± 20 68.0 ± 2.3 −620 ± 30 5030 ± 40
C IV 1549.48 300.0 ± 10.0 −430 ± 20 9840 ± 30 250.0 ± 7.9 −140 ± 10 9220 ± 20
He II 1640.45 9.1 ± 0.6 −80 ± 40 790 ± 50 6.9 ± 0.3 90 ± 20 790 ± 40
He II 1640.45 15.0 ± 0.6 840 ± 90 3250 ± 30 19.0 ± 1.1 −110 ± 30 3450 ± 120
He II 1640.45 98.0 ± 3.0 −120 ± 20 11080 ± 30 39.0 ± 1.9 −5330 ± 40 23200 ± 660
O III] 1660.81 5.5 ± 0.3 −160 ± 20 1200 ± 20 3.5 ± 0.4 −160 ± 20 2790 ± 60
O III] 1666.15 6.5 ± 0.3 −160 ± 20 1200 ± 20 15.0 ± 0.7 −160 ± 10 2790 ± 60
N III] 1750.00 13.0 ± 0.4 0 ± 30 3270 ± 20 15.0 ± 0.5 0 ± 40 3270 ± 30

Notes.

(a)

Vacuum rest wavelength of the spectral feature (Å).

(b)

Integrated flux in units of 10−14 erg cm−2 s−1.

(c)

Velocity (in km s−1) relative to a systemic redshift of z = 0.00973 (Theureau et al. 1998).

(d)

Full-width at half-maximum (km s−1).

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