SUPER - VIII. Fast and furious at z ∼ 2: Obscured type-2 active nuclei host faster ionised winds than type-1 systems

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Volume 690 (October 2024)

A&A, 690 (2024) A141

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Table 1.

Main properties of the 12 observed type-2 AGN from SUPER.

Field & Target ID	RA	Dec	z	log M_*	SFR	log L_bol	log L_{2 − 10 keV}	log N_H	Analysed
	(hh:mm:ss)	(dd:mm:ss)		[M_⊙]	[M_⊙ yr⁻¹]	[erg s⁻¹]	[erg s⁻¹]	[cm⁻²]
CDF-S XID36	03:31:50.77	−27:47:03.41	2.255	10.68 ± 0.07	184 ± 9	45.70 ± 0.06	$43 . 84_{- 0.63}^{+ 0.31}$ $43.84^{+0.31}_{-0.63}$	> 24.1	Yes
CDF-S XID57	03:31:54.40	−27:56:49.70	2.298 ^( † )	10.49 ± 0.11	< 34	44.26 ± 0.18	$44 . 04_{- 0.24}^{+ 0.17}$ $44.04^{+0.17}_{-0.24}$	$23 . 30_{- 0.39}^{+ 0.32}$ $23.30^{+0.32}_{-0.39}$	No
CDF-S XID419	03:32:23.44	−27:42:54.97	2.143	10.89 ± 0.02	42 ± 4	45.54 ± 0.05	$43 . 84_{- 0.44}^{+ 0.29}$ $43.84^{+0.29}_{-0.44}$	$24 . 28_{- 0.31}^{+ 0.19}$ $24.28^{+0.19}_{-0.31}$	Yes
CDF-S XID427	03:32:24.20	−27:42:57.51	2.303 ^( † )	10.87 ± 0.08	< 72	44.60 ± 0.13	$43 . 20_{- 0.06}^{+ 0.06}$ $43.20^{+0.06}_{-0.06}$	$22 . 43_{- 0.34}^{+ 0.24}$ $22.43^{+0.24}_{-0.34}$	No
CDF-S XID522	03:32:28.50	−27:46:57.99	2.309 ^( † )	10.42 ± 0.02	492 ± 25	45.02 ± 0.02	$43 . 51_{- 0.87}^{+ 0.76}$ $43.51^{+0.76}_{-0.87}$	> 22.5	No
CDF-S XID614	03:32:33.02	−27:42:00.33	2.453	10.78 ± 0.08	247 ± 12	44.97 ± 0.13	$43 . 61_{- 0.18}^{+ 0.18}$ $43.61^{+0.18}_{-0.18}$	$24 . 25_{- 0.18}^{+ 0.19}$ $24.25^{+0.19}_{-0.18}$	Yes
COSMOS cid_1057	09:59:15.00	+02:06:39.65	2.210	10.84 ± 0.07	85 ± 4	45.91 ± 0.06	$44 . 53_{- 0.30}^{+ 0.26}$ $44.53^{+0.26}_{-0.30}$	$23 . 98_{- 0.28}^{+ 0.24}$ $23.98^{+0.24}_{-0.28}$	Yes
COSMOS cid_451	10:00:00.61	+02:15:31.06	2.444	11.21 ± 0.05	< 125	46.44 ± 0.07	$45 . 18_{- 0.19}^{+ 0.23}$ $45.18^{+0.23}_{-0.19}$	$23 . 87_{- 0.15}^{+ 0.19}$ $23.87^{+0.19}_{-0.15}$	Yes
COSMOS cid_2682	10:00:08.81	+02:06:37.66	2.437	11.03 ± 0.04	< 93	45.48 ± 0.10	$44 . 30_{- 0.27}^{+ 0.96}$ $44.30^{+0.96}_{-0.27}$	$23 . 92_{- 0.20}^{+ 1.01}$ $23.92^{+1.01}_{-0.20}$	Yes
COSMOS cid_1143	10:00:08.84	+02:15:27.99	2.443	10.40 ± 0.17	108 ± 18	44.85 ± 0.12	$44 . 83_{- 0.36}^{+ 0.43}$ $44.83^{+0.43}_{-0.36}$	$24 . 01_{- 0.29}^{+ 0.77}$ $24.01^{+0.77}_{-0.29}$	Yes
COSMOS cid_971	10:00:59.45	+02:19:57.44	2.473 ^( † )	10.60 ± 0.12	< 96	44.71 ± 0.24	$43 . 87_{- 0.38}^{+ 0.36}$ $43.87^{+0.36}_{-0.38}$	< 23.68	No
COSMOS cid_1253	10:01:30.57	+02:18:42.57	2.147 ^( † )	10.99 ± 0.25	280 ± 194	45.08 ± 0.18	$43 . 92_{- 0.31}^{+ 0.29}$ $43.92^{+0.29}_{-0.31}$	$23 . 22_{- 0.39}^{+ 0.47}$ $23.22^{+0.47}_{-0.39}$	No

Notes. From left to right, the columns report the sky field and target ID, the coordinates of the optical counterpart of the target (J2000), the spectroscopic redshift z, the galaxy stellar mass M_*, SFR, the AGN bolometric luminosity L_bol, all with 1σ uncertainties derived from SED fitting (Circosta et al. 2018), the 2–10 keV X-ray luminosity L_{2 − 10 keV} and the hydrogen column density N_H with 90% confidence level errors, measured from archival X-ray data (Circosta et al. 2018), and whether the object is detected in SINFONI observations and is hence included in the final analysed sample (see Sect. 2.2). The redshift of the detected objects is inferred from rest-frame optical SINFONI spectra (Sect. 3.1), and for the others, it is inferred from archival rest-frame UV spectra (marked with the dagger).

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