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Table A.2.

[O III] best-fit results

ID Anarrow vnarrow σnarrow δA vbroad δsigma S/Nbroad χ single 2 $ \chi^2_{\rm single} $ χ double 2 $ \chi^2_{\rm double} $ Δlog K
[10−19 erg s−1 cm−2 Å−1] [km s−1] [km s−1] [km s−1]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
3968 0.37 ± 0.01 51.2 ± 54.5 64.8 ± 1.7 0.0498 ± 0.0004 −160.8 ± 2.8 5.67 ± 0.01 0.8 0.45 0.40 -1.74
4297 1.49 ± 0.02 −30.9 ± 49.3 57.7 ± 1.0 0.0178 ± 0.0003 −304.1 ± 1.0 5.55 ± 0.02 1.2 0.94 0.85 -1.79
4404 2.33 ± 0.05 −5.8 ± 61.4 64.8 ± 2.2 0.0250 ± 0.0003 −31.6 ± 7.8 4.18 ± 0.01 1.8 0.55 0.45 -1.43
5457 0.56 ± 0.02 −20.5 ± 52.7 60.8 ± 0.8 0.3017 ± 0.0032 −153.1 ± 15.8 3.02 ± 0.03 4.1 1.04 0.66 3.89
5759 1.01 ± 0.02 20.1 ± 39.7 66.7 ± 2.0 0.0266 ± 0.0001 30.6 ± 2.9 5.10 ± 0.01 0.5 0.45 0.45 -2.54
6002 0.79 ± 0.02 −15.1 ± 36.9 55.4 ± 1.2 0.1098 ± 0.0002 23.8 ± 11.9 2.06 ± 0.00 4.9 0.79 0.66 -2.17
6246 0.55 ± 0.01 −44.6 ± 50.0 63.0 ± 1.3 0.1140 ± 0.0002 −2.9 ± 6.2 2.08 ± 0.01 3.2 1.08 1.01 -2.47
7938 2.57 ± 0.06 −17.8 ± 39.5 57.2 ± 1.4 0.2580 ± 0.0006 −35.0 ± 9.0 1.99 ± 0.02 15.1 0.76 0.44 0.15
8013 0.50 ± 0.01 −11.0 ± 49.8 52.0 ± 0.8 0.0518 ± 0.0003 83.2 ± 3.2 4.31 ± 0.01 0.9 0.76 0.73 -2.27
8113 2.21 ± 0.04 34.9 ± 54.7 57.1 ± 1.3 0.0215 ± 0.0001 −17.7 ± 6.6 3.22 ± 0.01 1.3 0.89 0.89 -3.71
9422 3.57 ± 0.12 −30.1 ± 75.5 66.0 ± 2.7 0.3328 ± 0.0004 29.8 ± 12.0 1.32 ± 0.00 34.8 3.32 1.65 26.88
9452 1.66 ± 0.07 −18.3 ± 49.1 93.8 ± 3.2 0.0382 ± 0.0001 36.7 ± 6.2 3.72 ± 0.01 0.4 0.85 0.86 -2.89
9743 1.92 ± 0.02 −32.2 ± 35.7 56.1 ± 0.7 0.0508 ± 0.0001 −72.4 ± 5.1 3.17 ± 0.00 1.3 0.48 0.45 -2.71
16625 1.23 ± 0.02 −0.6 ± 54.5 48.6 ± 0.7 0.0191 ± 0.0001 −77.2 ± 3.5 4.61 ± 0.02 1.5 0.72 0.70 -3.15
16745 1.39 ± 0.03 −27.1 ± 46.7 74.4 ± 2.5 0.0132 ± 0.0002 156.1 ± 9.3 6.04 ± 0.02 1.1 0.83 0.77 -2.42
17566 0.90 ± 0.03 −18.7 ± 58.8 81.1 ± 3.3 0.0974 ± 0.0012 50.9 ± 12.9 2.95 ± 0.01 2.2 1.98 1.80 1.74
18090 5.62 ± 0.12 −10.9 ± 44.7 73.7 ± 3.0 0.0460 ± 0.0013 −122.0 ± 10.7 4.00 ± 0.06 4.3 3.22 2.32 15.86
18846 2.29 ± 0.04 −9.2 ± 47.0 61.6 ± 1.8 0.0619 ± 0.0009 26.8 ± 13.6 2.96 ± 0.04 5.9 1.55 1.02 9.27
18976 0.79 ± 0.02 3.2 ± 47.7 41.8 ± 0.0 0.2841 ± 0.0004 49.4 ± 5.3 1.52 ± 0.00 8.3 1.26 1.06 -1.30
19342 1.03 ± 0.02 −18.4 ± 32.8 58.2 ± 1.3 0.0262 ± 0.0001 225.8 ± 7.7 4.22 ± 0.01 1.3 0.86 0.76 -2.53
19606 1.37 ± 0.02 −5.1 ± 50.3 56.3 ± 1.4 0.0290 ± 0.0002 49.9 ± 10.4 4.06 ± 0.02 1.5 1.16 1.13 -2.26
20961 0.51 ± 0.01 −22.2 ± 45.8 47.2 ± 0.4 0.0296 ± 0.0001 39.2 ± 6.3 3.60 ± 0.01 0.6 1.31 1.32 -3.60
22251 2.65 ± 0.05 −7.2 ± 47.4 51.5 ± 1.0 0.2919 ± 0.0001 22.4 ± 9.2 1.36 ± 0.00 24.5 1.73 1.66 -2.33
10009693 0.25 ± 0.01 14.0 ± 0.0 62.1 ± 0.6 0.1024 ± 0.0006 171.9 ± 0.2 5.89 ± 0.05 1.1 0.68 0.63 -1.68
10013609 1.16 ± 0.02 −20.6 ± 43.3 43.8 ± 0.2 0.3577 ± 0.0017 56.2 ± 16.8 2.08 ± 0.01 13.6 2.32 0.99 32.53
10013620 0.88 ± 0.03 −8.2 ± 49.2 64.7 ± 1.8 0.0765 ± 0.0002 −90.1 ± 7.8 2.06 ± 0.00 2.0 0.95 0.89 -2.36
10013704 2.04 ± 0.03 −45.2 ± 50.7 62.6 ± 2.3 0.1323 ± 0.0008 −42.1 ± 11.0 2.29 ± 0.04 9.5 1.53 1.00 7.32
10013905 0.92 ± 0.02 −0.0 ± 50.1 52.0 ± 1.1 0.0797 ± 0.0012 121.5 ± 9.5 2.26 ± 0.01 2.6 1.20 0.96 2.21
10015338 1.76 ± 0.06 −45.5 ± 45.5 86.0 ± 3.3 0.0724 ± 0.0026 −239.3 ± 3.0 5.06 ± 0.08 1.9 1.04 0.75 3.32
10016374 1.76 ± 0.04 −29.1 ± 49.5 79.8 ± 2.7 0.0347 ± 0.0008 208.1 ± 13.2 2.92 ± 0.00 2.1 2.40 1.99 2.97
10056849 0.95 ± 0.02 10.7 ± 40.1 51.9 ± 0.7 0.0364 ± 0.0002 −287.7 ± 2.1 3.73 ± 0.02 1.3 0.99 0.94 -2.44

Note: (1) NIRSpec ID of the target; (2) amplitude of the narrow component; (3,4) velocity centroid and dispersion of the narrow Gaussian component with respect to the systemic redshift of the galaxy reported in Bunker et al. (2023); (5) broad-to-narrow Gaussian amplitude ratio; (6) velocity centroid of the broad Gaussian component with respect to the systemic redshift of the galaxy; (7) broad-to-narrow Gaussian velocity dispersion ratio; (8) signal-to-noise ratio of the integrated flux of the broad component; (9,10) reduced chi-squared for the single- and double-Gaussian models, respectively; (11) log-difference between the two Bayesian evidences of the single- and double-Gaussian models.

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