The properties of the extended warm ionised gas around low-redshift QSOs and the lack of extended high-velocity outflows

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Volume 549 (January 2013)

A&A, 549 (2013) A43

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Table 7

Kinematics and line fluxes for specific regions of the EELR.

Object^a		Δv_r^b	σ_line^c	Hβ	[O iii] λ5007	Hα	[N ii] λ6585	Classification



PG 0026 + 129	A	48 ± 34	158 ± 14	2.4 ± 0.9	25.1 ± 1.0	...	...	AGN
	B	136 ± 32	153 ± 9	2.5 ± 0.4	19.8 ± 0.5	...	...	AGN
PG 0050 + 124	A	−312 ± 27	83 ± 24	...	...	9.3 ± 1.4	7.9 ± 0.3	H ii
	B	−475 ± 28	18 ± 23	...	...	6.9 ± 2.8	7.7 ± 0.4	H ii
	C	−215 ± 36	80 ± 30	...	...	9.8 ± 1.9	5.8 ± 0.7	H ii
PG 0052 + 251	A	−127 ± 36	110 ± 31	3.0 ± 0.5	9.4 ± 0.2	9.5 ± 0.4	< 2.5	H ii
	B	−232 ± 32	82 ± 27	6.3 ± 1.1	38.5 ± 0.2	22.1 ± 0.8	< 3.4	H ii?
	C	−264 ± 41	65 ± 28	5.5 ± 1.2	7.0 ± 0.4	14.1 ± 1.1	< 5.3	AGN
RBS 219	A	−95 ± 40	76 ± 22	...	...	12.1 ± 1.2	< 2.5	H ii
	B	17 ± 39	0 ± 25	...	...	5.8 ± 1.7	< 4.6	H ii
	C	−105 ± 47	0 ± 39	...	...	4.7 ± 2.9	< 8.3	H ii
SDSS J0155 − 0857	A	134 ± 40	73 ± 12	0.4 ± 0.3	3.5 ± 0.3	...	...	AGN
	B	−7 ± 42	129 ± 13	1.7 ± 0.8	7.0 ± 0.6	...	...	AGN
Mrk 1014	A	−100 ± 28	155 ± 22	9.1 ± 1.8	53.9 ± 0.5	26.1 ± 5.1^d	14.6 ± 0.7	AGN
	B	67 ± 32	229 ± 17	14.0 ± 3.5	40.1 ± 0.9	40.2 ± 10.0^d	14.2 ± 0.8	AGN
	C	−222 ± 31	113 ± 28	5.0 ± 1.0	23.0 ± 0.5	14.2 ± 2.7^d	6.8 ± 1.0	AGN
SDSS J0846 + 4426	A	−88 ± 46	132 ± 3	18.2 ± 2.2	198.2 ± 2.3	...	...	AGN
	B	−229 ± 46	143 ± 3	14.2 ± 1.4	146.0 ± 1.5	...	...	AGN
	C	−154 ± 50	130 ± 8	< 5.4	58.6 ± 1.8	...	...	AGN
SDSS J1131 + 2623	A	−44 ± 69	117 ± 3	1.9 ± 0.9	32.6 ± 0.6	...	...	AGN
	B	−32 ± 68	87 ± 4	1.6 ± 0.3	25.7 ± 0.4	...	...	AGN
	C	−424 ± 72	54 ± 8	< 1.3	8.6 ± 0.4	...	...	AGN
	D	131 ± 76	105 ± 10	< 2.4	13.9 ± 0.8	...	...	AGN
PKS 1217+023	A	45 ± 35	75 ± 27	2.5 ± 0.6	9.3 ± 0.3	...	...	AGN
	B	−61 ± 37	80 ± 27	3.4 ± 1.1	19.4 ± 0.7	6.1 ± 0.8	2.8 ± 0.5	AGN
SDSS J1230 + 6621	A	299 ± 24	114 ± 6	4.0 ± 0.9	35.3 ± 0.9	...	...	AGN
	B	67 ± 23	80 ± 5	2.9 ± 0.4	19.5 ± 0.5	...	...	AGN
PKS 1545 + 210	A	309 ± 47	93 ± 29	4.5 ± 2.4	36.9 ± 1.8	...	...	AGN
	B	−134 ± 64	212 ± 51	6.0 ± 4.1	35.5 ± 4.7	...	...	AGN
PG 1612 + 261	A	70 ± 29	77 ± 5	< 18.9	111.0 ± 4.7	...	...	AGN
	B	54 ± 28	91 ± 3	< 8.2	289.1 ± 2.0	...	...	AGN
	C	248 ± 28	82 ± 4	18.2 ± 3.7	199.8 ± 1.2	...	...	AGN
	D	−92 ± 33	105 ± 8	< 4.8	29.3 ± 1.2	...	...	AGN
SDSS J1655 + 2146	A	−85 ± 26	161 ± 2	1.3 ± 0.8	127.9 ± 0.9	...	...	AGN
	B	−85 ± 27	183 ± 3	20.4 ± 2.6	319.3 ± 3.0	...	...	AGN
	C	−78 ± 31	197 ± 7	8.1 ± 1.0	44.3 ± 1.2	...	...	AGN
	D	−128 ± 30	94 ± 5	< 4.1	43.5 ± 1.4	...	...	AGN
PG 1700 + 518	A	−889 ± 67	158 ± 39	2.1 ± 0.6	9.2 ± 0.8	...	...	AGN
PG 2130 + 099	A	−99 ± 68	180 ± 105	5.9 ± 3.0	3.5 ± 0.7	7.7 ± 1.6	3.8 ± 0.4	H ii
	B	−262 ± 36	176 ± 32	10.1 ± 2.8	22.1 ± 1.3	21.6 ± 1.1	9.5 ± 0.3	AGN?
PHL 1811	A	49 ± 27	33 ± 15	3.4 ± 0.4	3.4 ± 0.4	14.6 ± 1.0	5.7 ± 0.5	H ii
HE 2158 − 0107	A	42 ± 44	69 ± 26	8.1 ± 1.4	39.6 ± 1.5	11.5 ± 1.6	< 3.8	AGN
	B	−50 ± 39	39 ± 23	11.2 ± 1.8	108.5 ± 1.9	28.4 ± 3.6	< 8.2	AGN
	C	−50 ± 47	0 ± 30	< 3.6	18.7 ± 1.2	...	...	AGN
PKS 2349−014	A	−33 ± 49	172 ± 24	4.2 ± 0.8	6.9 ± 0.3	10.3 ± 0.7	5.7 ± 0.4	H ii
	B	−269 ± 57	299 ± 21	5.6 ± 2.1	20.8 ± 1.1	11.7 ± 2.2	13.2 ± 1.2	AGN
	C	97 ± 39	146 ± 22	12.2 ± 1.2	96.6 ± 0.9	34.0 ± 2.2	36.8 ± 1.6	AGN
	D	418 ± 47	0 ± 26	1.3 ± 0.1	5.8 ± 0.3	...	...	AGN
HE 2353−0420	A	85 ± 51	225 ± 17	7.6 ± 1.5	77.9 ± 2.0	22.5 ± 1.6	18.0 ± 1.0	AGN
	B	66 ± 46	189 ± 18	6.0 ± 1.3	116.5 ± 1.8	32.5 ± 2.2	26.6 ± 1.6	AGN

Notes.

^(a)

Name of QSOs followed with the alphabetically ordered character of the specific co-added spectra.

^(b)

Radial velocity offset with respect to the rest-frame of the nuclear [O iii] line. Negative values corresponds to a blue shift.

^(c)

Emission line dispersion after the instrumental dispersion was subtracted in quadrature. A zero dispersion means that the line was unresolved.

^(d)

The Hα line was strongly affected by telluric absorption and its flux was estimates from the Hβ line assuming zero dust extinction (Hα/Hβ = 2.87).

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