H in nearby low-luminosity QSO host galaxies | Astronomy & Astrophysics (A&A)

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Table 2:

Summary of the H I properties.
Object	$v_{\rm0}$ (LSR)	$I_{\rm H {\sc i}}$ ^a	$W_{\rm 50}$ ^b	LS^c	$M_{\rm H {\sc i}}$	$M_{\rm dyn}$	$M_{\rm tot, gas}$	$L^{\prime}$ $_{\rm CO}$ / $M_{\rm H {\sc i}}$	$L_{\rm IR}$	f	$\Sigma$ _M	$M_{\rm H {\sc i}}$ / $L_{\rm IR}$	$M_{H {\sc i}}$ / $L_{\rm B}$
	[km s^-1]	[Jy km s^-1]	[km s^-1]		[10 $^{\rm 9}$ $M_{\hbox{$\odot$ }}$ ]	[10 $^{\rm 10}$ $M_{\hbox{$\odot$ }}$ ]	10 $^{\rm 10}$ $M_{\hbox{$\odot$ }}$ ]	[ $\frac{\rm {K~km~s}^{\rm -1}{\rm pc}^{\rm 2}}{{M}_{\hbox{$\odot$ }}}$ ]	[10 $^{\rm 10}$ $L_{\hbox{$\odot$ }}$ ]		[ $M_{\hbox{$\odot$ }}$ pc $^{\rm -2}$ ]	[ $M_{\hbox{$\odot$ }}$ / $L_{\hbox{$\odot$ }}$ ]	[ $M_{\hbox{$\odot$ }}$ / $L_{\hbox{$\odot$ }}$ ]
HE 0045	6 403	3.29 $\pm$ 0.13	180.8	$\upuparrows$ $_{\rm A}$	5.7 $\pm$ 0.2	7.1	11.5	0.13	8.10	0.6	20.0	0.08	1.2
HE 0150	14 329	2.70 $\pm$ 0.28	263.0	$\upuparrows$ $_{\rm A}$	23.8 $\pm$ 2.5	45.0	26.8	0.02	11.10	0.9	27.0	0.21	4.9
HE 0212	7 921	1.97 $\pm$ 0.18	206.4	$\wedge$ $_{\rm A}$	5.3 $\pm$ 0.5	3.3	11.7	0.09	4.07	1.1	121.6	0.13	0.4
HE 0224	18 150	$2.64 \pm 0.26$	271.0	$\sqcap$ $_{\rm A}$	37.5 $\pm$ 3.7	90.8	41.5	0.01	10.50	0.3	20.3	0.34	3.8
HE 0227	4914	$2.58 \pm 0.16$	193.9	$\sqcap$	2.6 $\pm$ 0.2	0.9	3.4	0.07	1.08	1.0	466.9	0.24	0.7
HE 0232	12 886	3.31 $\pm$ 0.40	559.0	$\wedge$ $_{\rm A}$	$23.6 \pm 2.8$	46.9	56.6	0.18	18.50	0.8	114.9	0.13	0.8
HE 0949	5974	5.88 $\pm$ 0.46	181.4	$\wedge$ $_{\rm A}$	8.7 $\pm$ 0.7	3.5	9.5	0.01	-	1.5	58.0	-	1.7
HE 1029	12 112	$1.05 \pm 0.10$	241.0	$\upuparrows$	6.6 $\pm$ 0.6	24.2	17.2	0.20	21.20	0.9	14.4	0.05	0.6
HE 1237	2531	$7.55 \pm 0.36$	355.5	$\upuparrows$	$2.0 \pm 0.1$	67.5	2.82	0.05	1.44	0.9	1.00	0.14	1.2
HE 1248	4338	$0.78\pm0.03$	119.5	$\wedge$ $_{\rm A}$	$1.2 \pm 0.2$ ^d	5.7	2.2	0.08	1.29	1.4	2.6	0.12	3.5
HE 1330	6744	$1.84 \pm 0.35$	180.4	$\upuparrows$	$3.6 \pm 0.7$	16.1	5.0	0.05	-	1.0	6.3	-	1.6
HE 2302	14 120	$1.39 \pm 0.18$	338.0	$\upuparrows$ $_{\rm A}$	$11.9 \pm 1.5$	130.7	19.7	0.08	-	1.3	4.7	-	1.1
Non-detections
HE 0021	15 889	<2.03	222.7		<22.2		<2.4	>0.01	-			-	<4.1
HE 0040	12 390	<1.58	222.7		<10.7		<1.3	>0.03	-			-	<4.2
HE 0114	13 672	<1.75	222.7		<14.0		<1.7	>0.03	-			-	<2.5
HE 0119	16 291	<1.42	222.7		<16.5		<2.7	>0.08	24.6			<0.07	<1.0
HE 0253	9470	<2.58	222.7		<10.1		<1.5	>0.06	4.90			<0.21	<2.2
HE 0433	10 658	<2.21	222.7		<10.7		<2.9	>0.21	22.7			<0.05	<1.1
HE 0853	17 930	<1.03	222.7		<14.3		<2.1	>0.06	-			-	<1.5
HE 1011	17 388	<0.56	222.7		<7.5		<1.5	>0.12	-			-	<0.2
HE 1017	14 985	<1.22	222.7		<11.4		<1.6	>0.05	9.88			<0.12	<1.2
HE 1107	17 088	<1.03	222.7		<13.6		<1.8	>0.04	-			-	<0.8
HE 1108	7199	<0.50	222.7		<1.1		<0.9	>0.85	10.4			<0.01	<0.1
HE 1126	17 988	<1.83	222.7		<25.7		<3.4	>0.04	-			-	<0.5
HE 1353	10 388	<2.44	222.7		<11.4		<1.7	>0.07	-			-	<4.7
HE 2222	17 431	<1.22	222.7		<15.9		<1.7	>0.01	-			-	<3.7
HE 2233	16 933	<2.93	222.7		<36.1		<4.0	>0.01	-			-	<4.4

^a Upper limits and errors represent 3 $\sigma$ values; ^b for the non-detections, values of W $_{\rm 50}$ correspond to the median value of all detected sources; ^c line shape: $\wedge$ represents a triangular shaped line profile; A stands for asymmetries in the line profiles; spectra with $\sqcap$ show a boxy line profile; $\upuparrows$ mark line profiles of a double-horn shape; ^d this detection was already confirmed by follow-up observations with the VLA. The obtained value for the H I mass is $\sim$ $1.0 \times 10^{\rm 9}$ $M_{\hbox{$\odot$ }}$ (König et al. 2009).

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