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 3.

Main properties of ionised outflows in the seven SUPER type-2 AGN.

Target ID	A_V	R_out	v_out	$L_{out}^{[OIII]}$ $L^{\mathrm{[OIII]}}_{\mathrm{out}}$	Ṁ_out	v_esc	w₈₀	v_max
		[kpc]	[km s⁻¹]	[10⁴² erg s⁻¹]	[M_⊙ yr⁻¹]	[km s⁻¹]	[km s⁻¹]	[km s⁻¹]
	(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)
XID36	1.3 ± 0.8	3.5	990 ± 50	14 ± 5	10 ± 6	860 ± 220	1760 ± 120	1450 ± 80
XID419	> 0	3.6	790 ± 120	> 0.3	> 0.2	980 ± 210	1020 ± 110	800 ± 40
XID614	2.8 ± 1.6	< 1.9	590 ± 60	2.2 ± 1.6	> 1.7	> 980	960 ± 140	910 ± 80
cid_1057	1.8 ± 1.0	3.1	720 ± 70	2.2 ± 1.0	1.3 ± 0.9	960 ± 240	1130 ± 130	1420 ± 130
cid_1143	$1 . 2_{- 1.2}^{+ 1.8}$ $1.2^{+1.8}_{-1.2}$	2.9	1070 ± 120	$3_{- 2}^{+ 14}$ $3^{+14}_{-2}$	$3_{- 2}^{+ 29}$ $3^{+29}_{-2}$	760 ± 290	1320 ± 70	1370 ± 120
cid_2682	> 0.6	2.0	670 ± 80	> 0.9	> 0.8	1190 ± 270	1130 ± 90	1240 ± 130
cid_451	> 2.7	2.6	950 ± 40	> 30	> 27	1400 ± 330	1270 ± 70	1290 ± 40

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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