JWST’s PEARLS: A z ≃ 6 quasar in a train-wreck galaxy merger system

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Table 2.

Properties of the quasar-driven outflow measured from Hβ and [O III] λ 5007 in the integrated quasar spectrum (Figure 3): luminosity, L_out, line width, FWHM_out, velocity offset, v_offset, outflow velocity, v_out, outflow mass, M_out, outflow rate, Ṁ_out, and power, P_out.

L_out, Hβ	L_{out, [OIII]}	FWHM_out	v_offset	v_out	M_out, Hβ	M_{out, [OIII]}	Ṁ_{out, Hβ}	Ṁ_out,[OIII]	P_out, Hβ	P_{out, [OIII]}
(10⁴³ erg / s)		(km / s)			(10⁷ M_⊙)		(M_⊙ / yr)		(10⁴³ erg / s)
$1 . 6_{- 1.2}^{+ 0.0}$ $1.6^{+0.0}_{-1.2}$	$7 . 9_{- 0.6}^{+ 0.2}$ $7.9^{+0.2}_{-0.6}$	$7080_{- 1186}^{+ 238}$ $7080^{+238}_{-1186}$	$- 2510_{- 220}^{+ 450}$ $-2510^{+450}_{-220 }$	$6050_{- 630}^{+ 470}$ $6050^{+470}_{-630 }$	$27_{- 20}^{+ 1}$ $27^{+1}_{-20 }$	$6 . 4_{- 0.4}^{+ 0.1}$ $6.4^{+0.1}_{-0.4 }$	$1655_{- 1230}^{+ 132}$ $1655^{+132}_{-1230 }$	$393_{- 50}^{+ 31}$ $393^{+31}_{-50 }$	$19_{- 14}^{+ 3}$ $19^{+3}_{-14 }$	$4 . 5_{- 0.9}^{+ 0.6}$ $4.5^{+0.6}_{-0.9 }$

Notes. These calculations assume a gas density in the ionised outflow of $⟨ n_{e} ⟩ = 500 {cm}^{- 3}$ $\langle n_{\mathrm{e}}\rangle = 500\,\rm{cm}^{-3}$ , and an outflow radius of R_out = 1 ± 0.1 kpc, as the outflow is spatially unresolved in the current data.

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