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Table A.1.

Compilation of AGN samples that have been spectroscopically characterized with JWST from the literature.

Source RA Dec zspec log MBH, ref log M*, ref fAGN log MBH log M* Reference
[J2000] [J2000] [M⊙] [M⊙] [M⊙] [M⊙]
J0148+0600 177.06933 52.86397 5.98 ⋯ ⋯ ⋯ Yue et al. (2023)
J159−02 159.22579 −2.54387 6.38 ⋯ ⋯ ⋯ Yue et al. (2023)
J1120+0641 170.00617 6.69008 7.09 ⋯ ⋯ ⋯ Yue et al. (2023)
J0100+2802 15.05425 28.04050 6.33 < 11.58 ⋯ ⋯ ⋯ Yue et al. (2023)
J1030+0524 157.61296 5.41529 6.30 < 10.65 ⋯ ⋯ ⋯ Yue et al. (2023)
J1148+5251 27.15683 6.00556 5.98 < 10.93 ⋯ ⋯ ⋯ Yue et al. (2023)
J2236+0032 339.18575 0.54914 6.40 ⋯ ⋯ ⋯ Ding et al. (2023)
J2255+0251 343.90850 2.85739 6.34 ⋯ ⋯ ⋯ Ding et al. (2023)
CEERS01244 215.24067 53.03606 4.48 ⋯ ⋯ ⋯ Harikane et al. (2023)
GLASS160133 3.58029 −30.42439 4.02 < 8.82 0.05 ± 0.20 > 5.78 8.87 ± 0.16 Harikane et al. (2023)
GLASS150029 3.57717 −30.42258 4.58 0.05 ± 0.20 > 4.97 9.01 ± 0.14 Harikane et al. (2023)
CEERS00746 214.80913 52.86847 5.62 < 9.11 ⋯ ⋯ ⋯ Harikane et al. (2023)
CEERS01665 215.17821 53.05936 4.48 ⋯ ⋯ ⋯ Harikane et al. (2023)
CEERS00672 214.88967 52.83297 5.67 < 9.01 0.80 ± 0.17 > 5.46 8.90 ± 0.77 Harikane et al. (2023)
CEERS02782 214.82346 52.83028 5.24 < 9.35 0.80 ± 0.28 > 6.28 9.84 ± 0.28 Harikane et al. (2023)
CEERS00397 214.83621 52.88269 6.00 0.05 ± 0.17 > 5.53 9.21 ± 0.14 Harikane et al. (2023)
CEERS00717 215.08142 52.97219 6.94 ⋯ ⋯ ⋯ Harikane et al. (2023)
CEERS01236 215.14529 52.96728 4.48 0.05 ± 0.24 > 4.98 8.82 ± 0.14 Harikane et al. (2023)
MSAID2008 3.59242 −30.43283 6.74 ⋯ ⋯ 0.20 ± 0.25 > 5.12 9.21 ± 0.41 Greene et al. (2024)
MSAID4286 3.61920 −30.42327 5.84 ⋯ 0.35 ± 0.08 > 6.21 11.25 ± 0.21 Greene et al. (2024)
MSAID10686 3.55084 −30.40660 5.05 ⋯ ⋯ 0.50 ± 0.08 > 6.07 10.61 ± 0.18 Greene et al. (2024)
MSAID13123a 3.57983 −30.40157 7.04 ⋯ 0.35 ± 0.06 > 5.86 10.50 ± 0.10 Greene et al. (2024)
MSAID13821 3.62061 −30.39995 6.34 ⋯ 0.20 ± 0.11 > 5.54 10.12 ± 0.17 Greene et al. (2024)
MSAID15383a 3.58353 −30.39668 7.04 ⋯ ⋯ 0.65 ± 0.01 > 5.95 10.43 ± 0.11 Greene et al. (2024)
MSAID16594a 3.59720 −30.39433 7.04 ⋯ ⋯ 0.50 ± 0.06 > 5.61 10.24 ± 0.14 Greene et al. (2024)
MSAID23608 3.54282 −30.38065 5.80 ⋯ 0.20 ± 0.16 > 5.87 9.34 ± 0.18 Greene et al. (2024)
MSAID28876 3.56960 −30.37322 7.04 ⋯ ⋯ 0.50 ± 0.11 > 5.54 10.1 ± 0.20 Greene et al. (2024)
MSAID32265 3.53753 −30.37017 ⋯ ⋯ ⋯ ⋯ ⋯ ⋯ Greene et al. (2024)
MSAID33437 3.54642 −30.36625 ⋯ ⋯ ⋯ ⋯ ⋯ ⋯ Greene et al. (2024)
MSAID35488 3.57898 −30.36260 6.26 ⋯ 0.05 ± 0.17 > 6.66 9.51 ± 0.12 Greene et al. (2024)
MSAID38108 3.53001 −30.35801 4.96 ⋯ 0.50 ± 0.07 > 5.98 10.67 ± 0.12 Greene et al. (2024)
MSAID39243 3.51389 −30.35602 ⋯ ⋯ ⋯ ⋯ ⋯ ⋯ Greene et al. (2024)
MSAID41225 3.53399 −30.35331 6.76 ⋯ 0.05 ± 0.18 > 5.08 9.69 ± 0.21 Greene et al. (2024)
MSAID45924 3.58476 −30.34363 4.46 ⋯ 0.20 ± 0.01 > 6.56 11.22 ± 0.02 Greene et al. (2024)
CEERS1019 215.03539 52.89066 8.68 0.80 ± 0.26 > 7.13 10.29 ± 0.53 Larson et al. (2023a)
GS3073 53.07888 −27.88416 5.55 ⋯ ⋯ ⋯ Übler et al. (2023)
1670 214.82345 52.83028 5.24 < 9.78 0.95 ± 0.30 > 5.16 7.61 ± 0.51 Kocevski et al. (2023)
3210AV4 214.80914 52.86848 5.62 < 10.78 0.65 ± 0.11 > 5.50 10.36 ± 0.29 Kocevski et al. (2023)
J2239+0207 339.94779 2.12986 6.25 ⋯ ⋯ ⋯ Stone et al. (2023)
10013704a 53.12654 −27.81809 5.92 ⋯ ⋯ ⋯ Maiolino et al. (2023)
10013704b 53.12654 −27.81809 5.92 ⋯ ⋯ ⋯ Maiolino et al. (2023)
8083 53.13284 −27.80186 4.65 0.20 ± 0.24 > 5.86 8.45 ± 0.17 Maiolino et al. (2023)
1093 189.17974 62.22463 5.60 ⋯ ⋯ ⋯ Maiolino et al. (2023)
3608 189.11794 62.23552 5.27 0.20 ± 0.31 > 5.21 7.92 ± 0.39 Maiolino et al. (2023)
11836 189.22059 62.26368 4.41 0.20 ± 0.22 > 5.91 8.57 ± 0.19 Maiolino et al. (2023)
20621 189.12252 62.29285 4.68 0.35 ± 0.33 > 4.97 8.20 ± 0.34 Maiolino et al. (2023)
73488a 189.19740 62.17723 4.13 ⋯ ⋯ ⋯ Maiolino et al. (2023)
73488b 189.19740 62.17723 4.13 ⋯ ⋯ ⋯ Maiolino et al. (2023)
77652 189.29323 62.19900 5.23 ⋯ ⋯ ⋯ Maiolino et al. (2023)
61888 189.16802 62.21701 5.88 0.20 ± 0.27 > 6.51 9.08 ± 0.48 Maiolino et al. (2023)
62309 189.24898 62.21835 5.17 0.50 ± 0.3 > 5.7 7.94 ± 0.39 Maiolino et al. (2023)
53757a 189.26978 62.19421 4.45 ⋯ ⋯ ⋯ Maiolino et al. (2023)
53757b 189.26978 62.19421 4.45 ⋯ ⋯ ⋯ Maiolino et al. (2023)
954 189.15197 62.25964 6.76 0.65 ± 0.2 > 6.25 10.17 ± 0.43 Maiolino et al. (2023)
MSAID20466 3.64041 −30.38644 8.50 < 8.70 0.20 ± 0.12 > 5.38 9.99 ± 0.24 Kokorev et al. (2023)

Notes. Column (1): name or identifier of each source. Column (2)–(3): right ascension (RA) and declination (Dec) in decimal degrees. Column (4): spectroscopic redshift. Column (5): fraction of AGN component to the total emission within the rest-wavelengths of 0.1–0.7 μm. Column (6): lower limit black hole mass assuming an accretion at Eddington limit. Column (7): total stellar mass calculated following the method presented in this work. Column (8): original literature describing the object. Empty columns indicate that the data is unavailable in the public JWST datasets, and the corresponding source is not used to benchmark our quasar selection method.

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