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 |
![]() |
46.69 |
2 | 3928 | 3691 | 2.167 | 2.434 | 2 |
![]() |
45.88 |
3 | 2973 | 1264 | 2.328 | 0.932 | 1 |
![]() |
45.61 |
4 | 5179 | 2284 | 2.276 | 3.924 | 2 |
![]() |
46.08 |
5 | 5040 | 3500 | 2.276 | 17.27 | 2 |
![]() |
46.59 |
6 | 2833 | 2589 | 2.369 | 7.538 | 2 |
![]() |
46.48 |
7 | 5135 | 3464 | 2.178 | 5.251 | 2 |
![]() |
45.95 |
8 | 3850 | 3067 | 2.132 | 8.015 | 2 |
![]() |
46.22 |
9 | 3999 | 4815 | 2.282 | 8.860 | 2 |
![]() |
46.42 |
10 | 4195 | 6260 | 2.366 | 12.03 | 2 |
![]() |
46.51 |
11 | 4373 | 1858 | 2.341 | 1.682 | 1 |
![]() |
45.80 |
12 | 3666 | 1558 | 2.456 | 0.720 | 1 |
![]() |
45.40 |
13 | 3521 | 2541 | 2.615 | 7.932 | 2 |
![]() |
46.28 |
14 | 4871 | 2069 | 2.276 | 1.235 | 1 |
![]() |
46.40 |
15 | 5450 | 3654 | 2.403 | 7.592 | 2 |
![]() |
46.31 |
16 | 3937 | 3620 | 2.613 | 4.473 | 2 |
![]() |
46.30 |
17 | 5644 | 4436 | 2.299 | 4.462 | 2 |
![]() |
46.11 |
18 | 3382 | 4008 | 2.378 | 13.48 | 2 |
![]() |
46.41 |
19 | 3845 | 5036 | 2.522 | 4.280 | 2 |
![]() |
46.09 |
20 | 4190 | 2529 | 2.455 | 11.93 | 2 |
![]() |
46.57 |
21 | 2509 | 3467 | 2.463 | 15.30 | 2 |
![]() |
46.77 |
22 | 2633 | 2757 | 2.143 | 3.496 | 2 |
![]() |
45.94 |
23 | 4079 | 1733 | 2.182 | 2.082 | 1 |
![]() |
45.76 |
24 | 4071 | 4142 | 2.342 | 29.14 | 2 |
![]() |
46.87 |
25 | 2938 | 4309 | 2.393 | 2.918 | 2 |
![]() |
46.14 |
26 | 5996 | 2547 | 2.612 | 2.310 | 1 |
![]() |
45.85 |
27 | 3035 | 2517 | 2.363 | 16.90 | 2 |
![]() |
46.65 |
28 | 3160 | 1343 | 2.325 | 1.060 | 1 |
![]() |
46.50 |
29 | 4248 | 1805 | 2.422 | 1.504 | 1 |
![]() |
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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