Multi-phase investigation of outflows in the circumgalactic and interstellar media of luminous quasars at z ∼ 5

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Table 2.

Results of BAL analysis.

Quasar	BI_C IV	v_min,C IV	v_max,C IV	BI_Si IV
	[km s⁻¹]	[km s⁻¹]	[km s⁻¹]	[km s⁻¹]
J0017-1000	$4430_{- 580}^{+ 1380}$ $4430^{+1380}_{-580}$	$9570_{- 3500}^{+ 2700}$ $9570 ^{+2700}_{-3500}$	$21 140_{- 2330}^{+ 1850}$ $21\,140^{+1850}_{-2330}$	/
J0338+0021	$890_{- 480}^{+ 540}$ $890^{+540}_{-480}$	$12 410_{- 100}^{+ 290}$ $12\,410^{+290}_{-100}$	$22 490_{- 460}^{+ 180}$ $22\,490^{+180}_{-460}$	/
J1601-1828	$2610_{- 820}^{+ 1100}$ $2610^{+1100}_{-820}$	$15 220_{- 2290}^{+ 3820}$ $15\,220^{+3820}_{-2290}$	$40 980_{- 170}^{+ 50}$ $40\,980^{+50}_{-170}$	$1410_{- 250}^{+ 90}$ $1410^{+90}_{-250}$
J1004+2025	$6080_{- 1290}^{+ 1310}$ $6080^{+1310}_{-1290}$	$24 870_{- 230}^{+ 140}$ $24\,870^{+140}_{-230}$	$48 670_{- 90}^{+ 130}$ $48\,670^{+130}_{-90}$	$2600_{- 460}^{+ 360}$ $2600^{+360}_{-460}$
J0957-1016	$5680_{- 1090}^{+ 1140}$ $5680^{+1140}_{-1090}$	$9120_{- 6020}^{+ 2750}$ $9120^{+2750}_{-6020}$	$23 120_{- 690}^{+ 1100}$ $23\,120^{+1100}_{-690}$	$1280_{- 710}^{+ 1230}$ $1280^{+1230}_{-710}$
J2225+0330	$5390_{- 130}^{+ 30}$ $5390^{+30}_{-130}$	$9460_{- 80}^{+ 100}$ $9460^{+100}_{-80}$	$23 580_{- 50}^{+ 60}$ $23\,580^{+60}_{-50}$	$3240_{- 420}^{+ 100}$ $3240^{+100}_{-420}$

Notes. From left to right: C IV balnicity index, minimum and maximum outflow velocities for the six quasars in our sample displaying BAL features. The last column reports the balnicity index for the four targets showing Si IV BAL troughs.

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