JADES: A large population of obscured, narrow-line active galactic nuclei at high redshift

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Table B.1.

Table of AGN from JADES HST Deep & 3215 selected in this work.

ID	field	z	selection	log₁₀ M_*	SFR	M_UV	log₁₀ L_bol	Notes
			method	M_⊙	M_⊙ yr⁻¹		ergs s⁻¹
JADES-NS-GS00004902	1210	5.123	S2-VO87*	8.6 $_{0.02}^{0.03}$ $^{0.03}_{0.02}$	1.4 $_{- 0.14}^{0.21}$ $^{0.21}_{-0.14}$	-19.0	43.0
JADES-NS-GS00007099	1210	2.860	S2-VO87*	9.1 $_{0.01}^{0.01}$ $^{0.01}_{0.01}$	1.1 $_{- 0.06}^{0.07}$ $^{0.07}_{-0.06}$	-17.4	42.9
JADES-NS-GS00007762	1210	4.146	High ion	8.2 $_{0.02}^{0.02}$ $^{0.02}_{0.02}$	4.1 $_{- 0.28}^{0.29}$ $^{0.29}_{-0.28}$	-18.8	43.6	outflows
JADES-NS-GS00008083	1210	4.665	High ion & HeIIλ4686	7.8 $_{0.01}^{0.01}$ $^{0.01}_{0.01}$	7.3 $_{- 0.12}^{0.12}$ $^{0.12}_{-0.12}$	-18.5	44.5	Type-1 & LAE
JADES-NS-GS00008456	1210	1.884	HeIIλ4686	8.1 $_{0.08}^{0.03}$ $^{0.03}_{0.08}$	0.1 $_{- 0.01}^{0.03}$ $^{0.03}_{-0.01}$	-16.1	41.6
JADES-NS-GS00008880	1210	2.327	N2-BPT	7.1 $_{0.70}^{0.25}$ $^{0.25}_{0.70}$	0.1 $_{- 0.02}^{0.03}$ $^{0.03}_{-0.02}$	-14.9	42.0
JADES-NS-GS00009422	1210	5.942	HeIIλ1640 & HeIIλ4686	7.7 $_{0.00}^{0.00}$ $^{0.00}_{0.00}$	5.4 $_{- 0.03}^{0.04}$ $^{0.04}_{-0.03}$	-19.8	44.5	LAE
JADES-NS-GS00009452	1210	5.135	N2-BPT	8.1 $_{0.16}^{0.17}$ $^{0.17}_{0.16}$	4.2 $_{- 0.97}^{1.17}$ $^{1.17}_{-0.97}$	-17.9	43.6
JADES-NS-GS00010073	1210	2.632	HeIIλ4686	6.9 $_{0.04}^{0.06}$ $^{0.06}_{0.04}$	0.8 $_{- 0.04}^{0.05}$ $^{0.05}_{-0.04}$	-16.5	43.0
JADES-NS-GS00016745	1210	5.574	S2-VO87*	8.3 $_{0.04}^{0.03}$ $^{0.03}_{0.04}$	6.5 $_{- 0.27}^{0.26}$ $^{0.26}_{-0.27}$	-19.5	43.7
JADES-NS-GS00017072	1210	4.707	HeIIλ1640	8.2 $_{0.15}^{0.06}$ $^{0.06}_{0.15}$	0.4 $_{- 0.06}^{0.11}$ $^{0.11}_{-0.06}$	-17.9	42.3
JADES-NS-GS00017670	1210	2.350	HeIIλ4686	8.4 $_{0.01}^{0.01}$ $^{0.01}_{0.01}$	0.9 $_{- 0.04}^{0.04}$ $^{0.04}_{-0.04}$	-17.8	43.0
JADES-NS-GS00021842	1210	7.981	High ion	7.4 $_{0.02}^{0.03}$ $^{0.03}_{0.02}$	2.4 $_{- 0.07}^{0.08}$ $^{0.08}_{-0.07}$	-18.6	43.8	LAE
JADES-NS-GS00022251	1210	5.804	HeIIλ1640	7.9 $_{0.03}^{0.03}$ $^{0.03}_{0.03}$	4.7 $_{- 0.13}^{0.12}$ $^{0.12}_{-0.13}$	-18.9	44.1
JADES-NS-GS10000626	1210	4.468	HeIIλ4686 & High ion	6.8 $_{0.20}^{0.29}$ $^{0.29}_{0.20}$	0.3 $_{- 0.01}^{0.01}$ $^{0.01}_{-0.01}$	-16.8	42.5
JADES-NS-GS10008071	1210	2.227	S2-VO87	8.8 $_{0.01}^{0.01}$ $^{0.01}_{0.01}$	7.2 $_{- 0.17}^{0.15}$ $^{0.15}_{-0.17}$	-17.9	43.1
JADES-NS-GS10011849	1210	2.686	S2-VO87*	8.1 $_{0.04}^{0.03}$ $^{0.03}_{0.04}$	2.5 $_{- 0.06}^{0.06}$ $^{0.06}_{-0.06}$	-18.0	43.6
JADES-NS-GS10012477	1210	0.665	S2-VO87	7.8 $_{0.02}^{0.01}$ $^{0.01}_{0.02}$	0.1 $_{- 0.00}^{0.00}$ $^{0.00}_{-0.00}$	-15.7	41.5
JADES-NS-GS10012511	1210	2.019	N2-BPT	8.2 $_{- 0.4}^{0.3}$ $^{0.3}_{-0.4}$	3.2 $_{- 0.9}^{0.7}$ $^{0.7}_{-0.9}$	-16.5	41.7
JADES-NS-GS10013597	1210	3.320	HeIIλ4686	7.5 $_{0.06}^{0.13}$ $^{0.13}_{0.06}$	0.8 $_{- 0.12}^{0.20}$ $^{0.20}_{-0.12}$	-17.4	42.6
JADES-NS-GS10013609	1210	6.931	High ion	7.7 $_{0.07}^{0.06}$ $^{0.06}_{0.07}$	3.9 $_{- 0.18}^{0.19}$ $^{0.19}_{-0.18}$	-18.7	44.0	outflows
JADES-NS-GS10013905	1210	7.206	HeIIλ4686	7.4 $_{0.03}^{0.05}$ $^{0.05}_{0.03}$	2.2 $_{- 0.12}^{0.14}$ $^{0.14}_{-0.12}$	-18.6	43.7
JADES-NS-GS10015338	1210	5.073	HeIIλ4686	7.9 $_{0.04}^{0.04}$ $^{0.04}_{0.04}$	3.6 $_{- 0.19}^{0.15}$ $^{0.15}_{-0.19}$	-19.4	43.9	LAE
JADES-NS-GS10035295	1210	3.588	HeIIλ1640	7.4 $_{0.03}^{0.07}$ $^{0.07}_{0.03}$	2.3 $_{- 0.05}^{0.06}$ $^{0.06}_{-0.05}$	-18.0	43.7
JADES-NS-GS10036017	1210	2.016	N2-BPT & S2-VO87	9.3 $_{0.02}^{0.01}$ $^{0.01}_{0.02}$	85.5 $_{- 1.95}^{1.69}$ $^{1.69}_{-1.95}$	-20.7	44.1
JADES-NS-GS10040620	1210	1.776	N2-BPT	8.1 $_{0.04}^{0.04}$ $^{0.04}_{0.04}$	0.1 $_{- 0.01}^{0.02}$ $^{0.02}_{-0.01}$	-16.4	41.7
JADES-NS-GS10056849	1210	5.821	High ion	7.1 $_{0.04}^{0.06}$ $^{0.06}_{0.04}$	1.1 $_{- 0.04}^{0.05}$ $^{0.05}_{-0.04}$	-18.1	43.2	LAE
JADES-NS-GS10058975	1210	9.437	High ion & HeIIλ1640	8.1 $_{0.03}^{0.03}$ $^{0.03}_{0.03}$	6.6 $_{- 0.20}^{0.20}$ $^{0.20}_{-0.20}$	-20.3	44.4
JADES-NS-GS00095256	3215	4.159	S2-VO87	7.4 $_{0.33}^{0.12}$ $^{0.12}_{0.33}$	0.3 $_{- 0.14}^{0.21}$ $^{0.21}_{-0.14}$	-16.9	43.0
JADES-NS-GS00099671	3215	5.936	HeIIλ4686	7.5 $_{0.05}^{0.05}$ $^{0.05}_{0.05}$	1.2 $_{- 0.06}^{0.07}$ $^{0.07}_{-0.06}$	-18.0	42.9
JADES-NS-GS00104075	3215	3.717	S2-VO87*	7.2 $_{0.07}^{0.12}$ $^{0.12}_{0.07}$	1.3 $_{- 0.28}^{0.29}$ $^{0.29}_{-0.28}$	-17.1	43.6
JADES-NS-GS00108487	3215	3.975	S2-VO87	8.9 $_{0.03}^{0.02}$ $^{0.02}_{0.03}$	0.5 $_{- 0.12}^{0.12}$ $^{0.12}_{-0.12}$	-18.2	44.5
JADES-NS-GS00111091	3215	4.497	S2-VO87	8.6 $_{0.04}^{0.03}$ $^{0.03}_{0.04}$	0.4 $_{- 0.01}^{0.03}$ $^{0.03}_{-0.01}$	-17.4	41.6
JADES-NS-GS00111511	3215	3.008	S2-VO87*	8.0 $_{0.05}^{0.03}$ $^{0.03}_{0.05}$	0.4 $_{- 0.02}^{0.03}$ $^{0.03}_{-0.02}$	-16.8	42.0
JADES-NS-GS00114573	3215	2.881	S2-VO87*	8.0 $_{0.05}^{0.04}$ $^{0.04}_{0.05}$	0.2 $_{- 0.03}^{0.04}$ $^{0.04}_{-0.03}$	-17.3	44.5
JADES-NS-GS00132213	3215	3.012	S2-VO87	7.7 $_{0.03}^{0.04}$ $^{0.04}_{0.03}$	0.3 $_{- 0.97}^{1.17}$ $^{1.17}_{-0.97}$	-17.6	43.6
JADES-NS-GS00143403	3215	0.735	S2-VO87*	8.2 $_{0.01}^{0.01}$ $^{0.01}_{0.01}$	0.1 $_{- 0.04}^{0.05}$ $^{0.05}_{-0.04}$	-15.4	43.0
JADES-NS-GS00201127	3215	5.837	S2-VO87*	8.2 $_{0.08}^{0.06}$ $^{0.06}_{0.08}$	2.1 $_{- 0.27}^{0.26}$ $^{0.26}_{-0.27}$	-18.5	43.7
JADES-NS-GS00202208	3215	5.450	HeIIλ1640	8.1 $_{0.02}^{0.02}$ $^{0.02}_{0.02}$	11.7 $_{- 0.06}^{0.11}$ $^{0.11}_{-0.06}$	-19.7	42.3
JADES-NS-GS00208643	3215	5.566	HeIIλ4686	7.2 $_{0.01}^{0.01}$ $^{0.01}_{0.01}$	1.5 $_{- 0.04}^{0.04}$ $^{0.04}_{-0.04}$	-18.0	43.0
JADES-NS-GS00209979	3215	1.883	S2-VO87*	8.5 $_{0.01}^{0.01}$ $^{0.01}_{0.01}$	1.8 $_{- 0.07}^{0.08}$ $^{0.08}_{-0.07}$	-17.9	43.8

Notes. Columns: ID, redshift, detection method ⁺, stellar mass, SFR and UV magnitude from BEAGLE, AGN bolometric luminosity and any other additional notes. We note that for bolometric luminosity the uncertainties are dominated by the systematical uncertainties (0.3-0.5 dex). ⁺ high-ion refers to identification based on [Ne IV] λ2424 and [Ne V] λ3420. ^* Tentative selection

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