Very extended cold gas, star formation and outflows in the halo of a bright quasar at z > 6

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Table B.1

Results of the Gaussian fits to the spectra extracted from different positions on the source shown in Fig. 3

Pos^†	v	σ _v	S _peak	I _ν
	[km s^-1]	[km s^-1]	[mJy]	[Jy km s^-1]

A	−700 ± 300	800 ± 300	0.8 ± 0.2	1.7 ± 0.8
	1100 ± 140	230 ± 150	0.8 ± 0.4	0.5 ± 0.4
B	−170 ± 40	110 ± 50	2.7 ± 1.0	0.7 ± 0.4
	−300 ± 400	800 ± 400	0.9 ± 0.5	1.7 ± 1.3
C	−1120 ± 110	210 ± 120	1.5 ± 0.7	0.8 ± 0.6
	700 ± 500	700 ± 400	1.0 ± 0.5	1.6 ± 1.2
	130 ± 100	140 ± 120	1.4 ± 1.0	0.5 ± 0.6
D	−900 ± 400	600 ± 400	1.1 ± 0.5	1.5 ± 1.3
	800 ± 200	500 ± 200	1.6 ± 0.5	1.9 ± 1.1
E	−1430 ± 90	130 ± 90	1.1 ± 0.6	0.4 ± 0.3
	100 ± 200	500 ± 200	1.5 ± 0.3	2.0 ± 0.9
	1200 ± 200	300 ± 200	0.7 ± 0.6	0.5 ± 0.5
F	110 ± 80	220 ± 80	1.9 ± 0.5	1.0 ± 0.5
	1100 ± 90	100 ± 90	1.0 ± 0.7	0.3 ± 0.3
	−800 ± 500	400 ± 600	0.4 ± 0.4	0.3 ± 0.7

Notes.

^(†)

Each row corresponds to a Gaussian component. We note that in all cases the spectral fit requires multiple Gaussian components.

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