Table C.1.
List of NLAGN selected in this work among CEERS MR spectra.
| ID | Redshift | selection | Log Lbol | AV | Log M* | SFR | Notes | |
|---|---|---|---|---|---|---|---|---|
| method | ergs s−1 | mag | M⊙ | M⊙ yr−1 | ||||
| CEERS-23* | 8.8802 | N5 | 44.92 ([OIII]) | x | 9.17 | 36 | ||
| CEERS-355 | 6.0995 | R3O1 He2N2 | 45.31 (Hβ) | 0.32 | 8.37 | 5 | ||
| CEERS-428 | 6.1022 | M2 | x | x | 8.06 | 2 | ||
| CEERS-496* | 6.5809 | N4 | 43.93 ([OIII]) | x | 7.93 | 1 | ||
| CEERS-613* | 6.7288 | C3He2 | 44.78 (Hβ) | x | 8.28 | 3 | ||
| CEERS-669 | 5.2714 | R3S2 | 45.22 ([OIII]) | >1.92 | 8.59 | 3 | ||
| CEERS-689 | 7.5457 | M1 M2 | 45.53 (Hβ) | x | x | x | ||
| CEERS-1019* | 8.6785 | N4 | 45.87 (Hβ) | x | 9.49 | 88 | ||
| CEERS-1029 | 8.61 | Ne4 | 45.4 (Hβ) | x | 9.86 | 58 | ||
| CEERS-1064 | 6.7905 | M2 | x | x | x | x | ||
| CEERS-1173 | 4.9955 | R3S2 | 45.55 (Hβ) | 1.06 | 8.97 | 6 | ||
| CEERS-1212 | 4.2772 | R3O1 | 44.44 (Hβ) | 0 | 9.22 | 5 | ||
| CEERS-1244 | 4.4778 | M2 | 45.28 (Hα) | x | 9.86 | 1 | BLAGN | |
| CEERS-1400 | 4.4893 | M2 | x | 0 | 8.19 | 3 | ||
| CEERS-1477 | 4.6307 | M1 M2 | 45.8 (Hβ) | 1.14 | 8.54 | 3 | ||
| CEERS-1536 | 5.0338 | M1 M2 | 45.41 (Hβ) | 0.3 | 8.93 | 5 | ||
| CEERS-1539 | 4.8838 | R3S2 R3O1 | 45.71 (Hβ) | 1.14 | 9.03 | 10 | ||
| CEERS-1561 | 6.1965 | M1 M2 | 45.45 (Hβ) | 0.18 | 8.68 | 4 | ||
| CEERS-1605 | 4.6305 | R3S2 M1 M2 | 45.07 (Hβ) | 0.46 | 8.69 | 11 | ||
| CEERS-1658 | 4.6035 | He2N2 | 44.95 (Hβ) | x | 8.65 | 7 | ||
| CEERS-1732 | 4.6598 | R3O1 | 45.28 (Hβ) | 0.27 | 10.02 | 33 | ||
| CEERS-1746 | 4.5602 | M1 M2 | 45.32 (Hβ) | 0.3 | 9.08 | 6 | ||
| CEERS-1767 | 4.5455 | M2 | x | x | 9.28 | 4 | ||
| CEERS-1836* | 4.4694 | R3S2 | 44.93 (Hβ) | 0.95 | 8.44 | 8 | ||
| CEERS-2168 | 5.6541 | M2 | x | x | 9.4 | 51 | ||
| CEERS-2668* | 2.8984 | R3N2 R3S2 | 45.5 ([OIII]) | >3.32 | 10.42 | 19 | ||
| CEERS-2754 | 2.238 | He2N2 | x | 1.47 | x | x | ||
| CEERS-2808 | 3.3834 | R3S2 | 44.99 (Hβ) | 1.31 | 10.68 | 619 | X-ray | |
| CEERS-2900 | 1.9004 | R3N2 R3S2 | 43.62 ([OIII]) | >2.06 | 11.17 | 0 | X-ray & Radio | |
| CEERS-2904 | 2.0249 | R3N2 R3S2 R3O1 He2N2 M1 M2 | 44.9 (Hα) | >2.17 | 10.78 | 26 | X-ray & BLAGN | |
| CEERS-2919 | 1.7177 | R3N2 R3S2 R3O1 He2N2 | 44.84 (Hα) | 1.75 | 10.62 | 203 | X-ray & BLAGN | |
| CEERS-3129 | 1.0373 | R3N2 R3S2 He2N2 | 44.46 (Hα) | 2.12 | 11.04 | 309 | Radio & BLAGN | |
| CEERS-3187 | 1.4896 | He2N2 | 43.76 (Hβ) | 0 | 8.23 | 3 | ||
| CEERS-3223 | 2.2862 | R3S2 | 43.91 (Hβ) | 0.18 | 8.9 | 1 | ||
| CEERS-3535* | 2.4886 | R3S2 | 44.95 (Hβ) | 0.14 | 8.87 | 6 | ||
| CEERS-3585* | 3.8662 | M2 | 45.76 (Hβ) | 1.77 | 7.97 | 2 | ||
| CEERS-3838 | 1.9221 | R3S2 R3O1 | 44.68 (Hβ) | 1.8 | 9.16 | 11 | ||
| CEERS-4210 | 5.2549 | Ne4 | 45.45 (Hβ) | 0.56 | 8.69 | 12 | ||
| CEERS-4385 | 3.4219 | He2N2 | 45.19 (Hβ) | 0.65 | 9.33 | 15 | ||
| CEERS-4402 | 3.3293 | R3O1 | 45.21 (Hβ) | 0.44 | 9.82 | 23 | ||
| CEERS-5117 | 1.5728 | R3S2 R3O1 | 44.41 (Hβ) | 1.16 | 9.26 | 2 | ||
| CEERS-6689 | 1.4608 | He2N2 | x | >5.53 | 10.82 | 95 | ||
| CEERS-8041 | 2.5319 | R3S2 | 44.96 ([OIII]) | >2.73 | 9.24 | 8 | ||
| CEERS-8110 | 1.5662 | R3O1 | 44.43 (Hβ) | 0.43 | 9.72 | 5 | ||
| CEERS-8299 | 2.1567 | Ne5 | 45.62 (Hβ) | 2.37 | 10.1 | 5 | ||
| CEERS-9156 | 2.0534 | R3S2 | 45.05 (Hβ) | 0.42 | 9.54 | 6 | ||
| CEERS-9238 | 1.7415 | R3S2 | 45.07 (Hβ) | 1.67 | 9.29 | 3 | ||
| CEERS-13661 | 3.3279 | R3S2 Ne4 | 45.0 (Hβ) | 0.76 | 9.03 | 9 | ||
| CEERS-16551 | 2.5714 | R3S2 R3O1 | 44.61 (Hβ) | 0 | 8.57 | 5 | ||
| CEERS-17496 | 2.3732 | R3S2 R3O1 | 44.62 (Hβ) | 0 | 8.79 | 3 | ||
| CEERS-31075 | 1.2831 | He2N2 | 44.4 (Hβ) | 0.11 | 7.8 | 0 | ||
| CEERS-44804 | 5.508 | M1 | 44.79 (Hβ) | x | 8.54 | 5 |
Notes. Columns: ID, redshift, diagnostic diagram(s) in which the source is selected, AGN bolometric luminosity (and the emission line used to derive it), ISM obscuration AV, stellar mass, SFR, and any other additional notes. For bolometric luminosities derived from the Hβ line we used the Netzer (2009) calibration, while for those derived from the [O III] λ5007 we used the Lamastra et al. (2009) calibration. Low-z and high-z BLAGN have instead Lbol computed using the broad Hα lines and the calibrations of Greene & Ho (2005). When a ’x’ is reported it means that it was not possible to compute that quantity for that source. Asterisks (*) mark tentative NLAGN selections.
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