GA-NIFS: Mapping z ≃ 3.5 AGN-driven ionized outflows in the COSMOS field

Open Access

Table 2.

Outflow properties of the GA-NIFS COS-AGNi sample as traced by the Hα emission line.

Target	L_Hα,out	R_out,fw	v_out	M_out	${\dot{M}}_{out}^{}$ ${\dot {M}}_{\mathrm {out}} ^{\mathrm {}}$	${\dot{E}}_{out}^{}$ ${\dot {E}}_{\mathrm {out}} ^{\mathrm {}}$	R_max	v_max
	(10⁴¹ erg s⁻¹)	(kpc)	(km s⁻¹)	(10⁶ M_⊙)	(M_⊙ yr⁻¹)	(10⁴¹ erg s⁻¹)	(kpc)	( km s⁻¹)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
COS590	12.1 ± 0.2	1.0 ± 0.4	569 ± 9	3.9 ± 1.9	6.6 ± 4.1	6.8 ± 4.2	2.6 ± 0.7	796 ± 5
COS1118	6.3 ± 0.2	0.7 ± 0.4	707 ± 4	2.0 ± 1.0	5.9 ± 4.1	9.3 ± 6.5	2.6 ± 0.7	823 ± 3
COS349	7.9 ± 0.4	1.0 ± 0.4	1278 ± 13	2.5 ± 1.3	10.4 ± 6.6	53.5 ± 34.2	2.6 ± 0.7	1384 ± 8
COS1656-A	18.4 ± 1.6	1.2 ± 0.4	950 ± 9	5.9 ± 3.0	14.8 ± 8.9	42.2 ± 25.4	2.6 ± 0.7	1326 ± 6
COS2949	5.7 ± 0.1	1.0 ± 0.4	732 ± 5	1.8 ± 0.9	4.3 ± 2.9	7.3 ± 4.9	2.1 ± 0.9	901 ± 3
COS1638-A	33.9 ± 0.3	0.9 ± 0.4	3199 ± 201	10.9 ± 5.4	120.8 ± 79.7	3900.8 ± 2676.5	3.0 ± 0.7	3551 ± 131
COS1638-B	307.3 ± 0.9	1.1 ± 0.4	2066 ± 90	98.3 ± 49.2	568.0 ± 345.0	7652.3 ± 4754.5	1.8 ± 0.7	2623 ± 56

Notes. Outflow properties in columns (5) to (7) are computed with flux-weighted outflow radii, outflow velocity v_out=max(v₁₀,v₉₀) and n_e = 1000 cm⁻³. The last two columns list the parameters needed to scale the outflow properties to the framework used for the comparison with the literature. Columns: (1) target name; (2) Hα luminosity in units of 10⁴¹ erg s⁻¹; (3) flux-weighted outflow radius in kpc units; (4) outflow velocity v_out=max(v₁₀,v₉₀) in km s⁻¹; (5) outflow mass computed from Eq. (2) in units of solar masses; (6) mass outflow rate computed in biconical geometry (Eq. (4)) in units of solar masses per year; (7) outflow kinetic power in units of 10⁴¹ erg s⁻¹; (8) maximum outflow radius in kpc units; (9) maximum outflow velocity v_max=|v_nar−v_bro|+2σ_bro in km s⁻¹.

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