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Table A.1.

Hα 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)
3184 2.40 ± 0.04 −54.9 ± 43.1 44.3 ± 0.1 0.1865 ± 0.0014 −29.3 ± 14.2 2.72 ± 0.05 10.8 1.41 0.85 7.29
4270 2.51 ± 0.10 −16.1 ± 71.2 108.7 ± 5.0 0.1419 ± 0.0009 107.4 ± 12.9 1.47 ± 0.00 5.1 1.43 0.75 10.33
4297 0.62 ± 0.01 −30.7 ± 28.6 43.4 ± 0.0 0.1089 ± 0.0005 −126.1 ± 3.2 2.90 ± 0.01 1.2 0.74 0.66 -1.89
4404 1.09 ± 0.03 −12.2 ± 55.7 63.2 ± 1.5 0.0137 ± 0.0000 45.2 ± 3.1 4.31 ± 0.01 0.4 0.90 0.92 -3.67
5329 0.45 ± 0.02 −3.5 ± 49.3 65.8 ± 2.2 0.1101 ± 0.0029 197.6 ± 14.0 8.05 ± 0.07 1.9 0.98 0.81 1.36
5759 0.59 ± 0.01 34.5 ± 36.0 55.0 ± 0.9 0.0640 ± 0.0005 −344.9 ± 1.3 4.72 ± 0.00 0.9 1.09 0.99 -1.26
6002 0.35 ± 0.01 −15.9 ± 49.2 58.7 ± 1.5 0.1221 ± 0.0014 114.8 ± 13.3 1.98 ± 0.00 1.7 1.44 1.31 0.61
6246 0.26 ± 0.01 −41.1 ± 40.5 57.4 ± 1.2 0.1659 ± 0.0026 51.8 ± 15.1 3.52 ± 0.03 2.7 0.95 0.69 3.92
6384 0.38 ± 0.01 61.1 ± 31.6 48.1 ± 0.1 0.0872 ± 0.0004 75.7 ± 1.9 4.12 ± 0.01 0.7 1.30 1.29 -1.89
7507 1.11 ± 0.03 31.3 ± 65.4 69.4 ± 2.6 0.0371 ± 0.0001 33.9 ± 9.7 3.05 ± 0.01 1.1 1.00 0.98 -3.55
7762 1.38 ± 0.03 −16.6 ± 40.7 55.9 ± 1.7 0.2383 ± 0.0005 29.3 ± 9.9 1.64 ± 0.00 14.5 1.24 0.64 7.43
7809 1.10 ± 0.05 −37.2 ± 57.5 117.6 ± 5.4 0.0675 ± 0.0006 −70.6 ± 2.8 4.49 ± 0.00 1.0 0.86 0.70 -1.46
7892 1.14 ± 0.03 −57.5 ± 53.9 58.2 ± 1.7 0.1608 ± 0.0010 −68.5 ± 10.5 2.26 ± 0.04 8.2 0.96 0.58 3.16
7938 1.14 ± 0.02 −26.4 ± 52.1 60.5 ± 1.7 0.0595 ± 0.0012 59.8 ± 7.0 3.09 ± 0.02 2.5 1.55 1.36 1.49
8083 3.66 ± 0.09 −48.5 ± 55.8 62.5 ± 2.4 0.0690 ± 0.0013 −78.0 ± 14.4 3.88 ± 0.09 10.5 4.70 1.44 85.81
8113 0.84 ± 0.02 45.6 ± 53.0 52.9 ± 1.0 0.0348 ± 0.0010 −345.9 ± 0.8 7.89 ± 0.04 1.7 0.97 0.82 0.82
9422 2.05 ± 0.03 −11.1 ± 59.0 65.9 ± 1.9 0.0290 ± 0.0003 130.5 ± 10.7 2.01 ± 0.00 1.6 1.32 1.14 -0.38
9743 1.15 ± 0.03 −29.2 ± 31.7 56.4 ± 1.4 0.2357 ± 0.0026 −419.4 ± 7.0 1.45 ± 0.00 1.9 1.51 1.18 3.56
16745 0.51 ± 0.02 −22.9 ± 53.2 69.4 ± 3.0 0.0639 ± 0.0025 204.2 ± 12.8 6.91 ± 0.08 2.0 1.17 0.86 6.38
17072 0.18 ± 0.00 −41.4 ± 32.4 51.6 ± 0.3 0.1003 ± 0.0004 −120.0 ± 9.0 3.49 ± 0.01 1.2 1.01 0.95 -1.48
17260 0.12 ± 0.01 −12.7 ± 47.9 63.3 ± 0.3 0.2794 ± 0.0049 14.8 ± 12.4 4.90 ± 0.06 3.6 1.30 1.09 2.72
17777 0.38 ± 0.01 −39.4 ± 46.4 59.8 ± 1.6 0.0968 ± 0.0020 302.2 ± 15.8 5.47 ± 0.09 2.5 1.18 0.82 4.37
18028 0.38 ± 0.01 −9.9 ± 38.2 41.6 ± 0.0 0.0800 ± 0.0007 27.9 ± 5.7 4.81 ± 0.02 1.6 0.76 0.74 -1.01
18090 1.45 ± 0.04 −28.3 ± 57.1 61.3 ± 2.6 0.2971 ± 0.0005 2.5 ± 9.9 1.87 ± 0.01 12.8 1.22 0.90 2.90
18970 4.20 ± 0.11 −10.9 ± 46.2 62.7 ± 2.3 0.2429 ± 0.0006 −58.3 ± 14.1 1.79 ± 0.01 13.3 2.11 1.81 1.75
19519 2.11 ± 0.03 −62.1 ± 54.2 60.8 ± 1.5 0.0272 ± 0.0000 −13.6 ± 4.9 2.77 ± 0.00 2.2 1.08 1.07 -4.34
10000626 0.26 ± 0.01 23.0 ± 43.4 54.2 ± 0.8 0.0573 ± 0.0003 −40.5 ± 9.7 3.95 ± 0.01 0.9 0.58 0.56 -1.87
10005113 0.45 ± 0.01 13.4 ± 36.5 44.1 ± 0.2 0.0523 ± 0.0003 55.8 ± 6.5 3.77 ± 0.01 1.1 0.46 0.44 -1.99
10009506 2.66 ± 0.06 22.6 ± 55.1 61.2 ± 1.6 0.0948 ± 0.0004 −10.2 ± 8.3 2.11 ± 0.02 5.8 0.81 0.62 -0.71
10013545 2.15 ± 0.03 −13.0 ± 35.6 64.5 ± 1.6 0.0694 ± 0.0001 23.9 ± 2.5 2.81 ± 0.00 4.1 0.88 0.70 -3.00
10013704 0.91 ± 0.03 −43.5 ± 45.4 65.8 ± 2.4 0.1384 ± 0.0046 221.8 ± 19.3 4.29 ± 0.14 4.2 3.02 1.16 60.09
10015338 0.97 ± 0.02 −24.9 ± 52.1 70.3 ± 2.0 0.1132 ± 0.0012 −175.3 ± 15.7 2.67 ± 0.01 1.6 1.06 0.95 -0.50
10016186 0.86 ± 0.04 −38.4 ± 54.2 80.2 ± 3.3 0.0897 ± 0.0032 −89.5 ± 13.4 5.36 ± 0.06 3.1 1.21 0.71 9.05
10016374 0.66 ± 0.02 −14.6 ± 45.1 63.3 ± 2.0 0.1215 ± 0.0002 −68.3 ± 10.5 1.97 ± 0.00 2.7 0.80 0.71 -2.53
10035295 2.24 ± 0.04 19.0 ± 36.3 58.3 ± 1.4 0.1381 ± 0.0002 37.1 ± 9.8 2.11 ± 0.00 8.2 1.01 0.94 -2.50

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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