Open Access

Table A.2.

Emission line measurements of our high-redshift SOFI targets in the Hα spectral region.

Hα

ID FWHM (km/s) σ (km s−1) zcorr fHα No. of Gaussian Comp. (Hα) MBH log10Lbol
(× 10−15) × 109 (erg s−1)
(M)
(1) (2) (3) (4) (5) (6) (7) (8)
1 6765 4448 2.269 22.90 2 8.23 1.99 + 2.61 $ {8.23}_{-1.99}^{+2.61} $ 46.69
2 3928 3691 2.167 2.434 2 1.90 0.46 + 0.60 $ {1.90}_{-0.46}^{+0.60} $ 45.88
3 2973 1264 2.328 0.932 1 0.15 0.04 + 0.05 $ {0.15}_{-0.04}^{+0.05} $ 45.61
4 5179 2284 2.276 3.924 2 2.28 0.55 + 0.72 $ {2.28}_{-0.55}^{+0.72} $ 46.08
5 5040 3500 2.276 17.27 2 4.48 1.08 + 1.42 $ {4.48}_{-1.08}^{+1.42} $ 46.59
6 2833 2589 2.369 7.538 2 1.70 0.41 + 0.54 $ {1.70}_{-0.41}^{+0.54} $ 46.48
7 5135 3464 2.178 5.251 2 2.39 0.58 + 0.76 $ {2.39}_{-0.58}^{+0.76} $ 45.95
8 3850 3067 2.132 8.015 2 2.20 0.53 + 0.70 $ {2.20}_{-0.53}^{+0.70} $ 46.22
9 3999 4815 2.282 8.860 2 6.30 1.52 + 2.00 $ {6.30}_{-1.52}^{+2.00} $ 46.42
10 4195 6260 2.366 12.03 2 12.94 3.13 + 4.11 $ {12.94}_{-3.13}^{+4.11} $ 46.51
11 4373 1858 2.341 1.682 1 0.42 0.10 + 0.14 $ {0.42}_{-0.10}^{+0.14} $ 45.80
12 3666 1558 2.456 0.720 1 0.21 0.05 + 0.07 $ {0.21}_{-0.05}^{+0.07} $ 45.40
13 3521 2541 2.615 7.932 2 1.86 0.45 + 0.59 $ {1.86}_{-0.45}^{+0.59} $ 46.28
14 4871 2069 2.276 1.235 1 0.45 0.45 + 0.14 $ {0.45}_{-0.45}^{+0.14} $ 46.40
15 5450 3654 2.403 7.592 2 3.52 0.85 + 1.12 $ {3.52}_{-0.85}^{+1.12} $ 46.31
16 3937 3620 2.613 4.473 2 2.97 0.72 + 0.94 $ {2.97}_{-0.72}^{+0.94} $ 46.30
17 5644 4436 2.299 4.462 2 3.91 0.94 + 1.24 $ {3.91}_{-0.94}^{+1.24} $ 46.11
18 3382 4008 2.378 13.48 2 5.47 1.32 + 1.74 $ {5.47}_{-1.32}^{+1.74} $ 46.41
19 3845 5036 2.522 4.280 2 5.53 1.34 + 1.76 $ {5.53}_{-1.34}^{+1.76} $ 46.09
20 4190 2529 2.455 11.93 2 2.07 0.50 + 0.66 $ {2.07}_{-0.50}^{+0.66} $ 46.57
21 2509 3467 2.463 15.30 2 4.48 1.08 + 1.43 $ {4.48}_{-1.08}^{+1.43} $ 46.77
22 2633 2757 2.143 3.496 2 1.21 0.29 + 0.39 $ {1.21}_{-0.29}^{+0.39} $ 45.94
23 4079 1733 2.182 2.082 1 0.38 0.09 + 0.12 $ {0.38}_{-0.09}^{+0.12} $ 45.76
24 4071 4142 2.342 29.14 2 8.22 1.99 + 2.61 $ {8.22}_{-1.99}^{+2.61} $ 46.87
25 2938 4309 2.393 2.918 2 3.17 0.77 + 1.01 $ {3.17}_{-0.77}^{+1.01} $ 46.14
26 5996 2547 2.612 2.310 1 1.06 0.26 + 0.34 $ {1.06}_{-0.26}^{+0.34} $ 45.85
27 3035 2517 2.363 16.90 2 2.34 0.56 + 0.74 $ {2.34}_{-0.56}^{+0.74} $ 46.65
28 3160 1343 2.325 1.060 1 0.17 0.04 + 0.06 $ {0.17}_{-0.04}^{+0.06} $ 46.50
29 4248 1805 2.422 1.504 1 0.35 0.08 + 0.11 $ {0.35}_{-0.08}^{+0.11} $ 45.90

Notes: The columns show the (1) ID number, (2) FWHM in km/s, (3) line dispersion (square root of the second moment of the line profile or σ) in km/s, (4) the corrected redshift based on the velocity offset of Hα with respect to its theoretical central wavelength, zcorr, (5) integrated Hα flux in ergs cm−2 s−1, (6) the number of Gaussian components used to fit the Hα line profile, (7) single-epoch BH mass estimate using Eqn. 6 of Woo et al. (2015), and (8) bolometric luminosity using the bolometric correction from Trakhtenbrot et al. (2017) to convert the λLλ(5100 Å) to Lbol. For ID#1-5 that were observed with the Ks filter, the λLλ(5100 Å) were estimated from their Hα luminosity using Eqn. 4 of Woo et al. (2015), and the typical error of their log10Lbol is ∼ 0.25. For the rest of the targets that were observed with the GRF filter, the λLλ(5100 Å) were measured via Monte Carlo analysis of best-fit continuum after 1000 instances of fitting, and the typical error of their log10Lbol is ∼ 0.014.

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