TANGO I: Interstellar medium in nearby radio galaxies - Molecular gas

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Table 5:

Molecular gas data.
Galaxy	$Z_{\rm CO}$	Distance	$I_{\rm CO(1-0)}$	$\delta I_{\rm CO(1-0)}$	FWZI $_{\rm CO(1-0)}$	$I_{\rm CO(2-1)}$	$\delta I_{\rm CO(2-1)}$	FWZI $_{\rm CO(2-1)}$	$M_{{\rm H}_2}$
		(Mpc)	(K Km s^-1)	(K Km s^-1)	(km s^-1)	(K Km s^-1)	(K Km s^-1)	(km s^-1)	( $\times 10^8~M_{sun}$ )
3C31^**,a	0.0169	71.06	5.68	0.81	550	14.06	1.13	550	$16.81\pm2.38$ ^**
3C40	...	...	<1.11	...	...	...	...	...	<3.25
3C66B^*,b	0.0157	85.20	0.2081	0.053	250	...	...	...	$0.89 \pm 0.23$ ^*
3C83.1^*,c	0.0251	104.6	0.53	0.002	-	1.13	0.12	200	$3.60 \pm 0.0013$
3C88^**,b	0.03	126.20	0.23 8	0.05	300	...	...	...	$2.19 \pm 0.44$ ^**
3C98	...	...	<0.73	...	...	...	...	...	<7.27
3C129^*,c	0.0208	86.4	0.28	0.024	-	0.59	0.11	200	$1.3 \pm 0.11$
3C236	...	...	<0.75	...	...	X	X	X	<80.70
3C264^**,a	0.02	90.90	0.70	0.15	200	1.48	0.16	225	$3.37 \pm 0.74$ ^**
3C270	...	...	<1.16	...	...	...	...	...	<0.69
3C272.1^*,a	0.0028	12.00	0.36	0.12	200	0.90	0.16	150	$0.03 \pm 0.01$ ^*
3C274^**,b	0.0035	14.90	4.02	0.39	200	...	...	...	$0.52 \pm 0.05$ ^**
3C296	...	...	<0.85	...	...	...	...	...	<5.05
3C305^**,b	0.042	171.70	1.19	0.14	600	X	X	X	$20.52 \pm 2.49$ ^**
3C321^**,b	0.10	379.97	0.83	0.09	500	X	X	X	$70.58 \pm 7.93$ ^**
3C327^*,b	0.1035	401.87	0.28	0.10	200	X	X	X	$26.48 \pm 9.59$ ^*
3C353^**,b	0.0327	153.73	0.31	0.05	200	...	...	...	$4.27 \pm 0.68$ ^**
3C386^**,c	0.017	71.7	0.58	0.02	--	1.23	0.17	175	$1.78 \pm 0.058$
3C402	...	...	<0.95	...	...	...	...	...	<6.59
3C403^**,b	0.058	134.97	0.44	0.11	500	X	X	X	$4.75 \pm 1.18$ ^**
3C433	...	...	<0.87	...	...	X	X	X	<93.13
3C442^**,c	0.0263	110.5	0.09	0.02	--	0.20	0.07	300	$0.67 \pm 0.16^{**}$
3C449^**,b	0.0169	71.40	1.20	0.24	500	...	...	...	$3.59 \pm 0.73$
3C465	...	...	<0.78	...	...	...	...	...	<7.69
NGC 315^*,b	0.0175	73.80	0.26	0.06	150	...	...	...	$0.82 \pm 0.19^{*}$
NGC 326^*	0.0474	203.18	0.2320	0.05	100	0.65	0.2	400	$5.61 \pm 1.2^{*}$
NGC 541^*,c	0.018	75.0	0.72	0.08	400	1.53	0.32	350	$2.5 \pm 0.27$
NGC 708^**,b	0.0166	69.86	1.84	0.31	600	...	...	...	$5.25 \pm 0.88$ ^**
NGC 2484	...	...	<1.00	...	...	...	...	...	<19.77
NGC 2892	...	...	<1.22	...	...	...	...	...	<6.85
NGC 3801^**,b	0.0117	49.50	3.82	1.14	600	...	...	...	$5.49 \pm 1.63$ ^**
NGC 4278^*,a	0.0022	9.40	1.00	0.22	600	3.13	0.31	500	$0.05 \pm 0.01$ ^**
NGC 5127^**,c	0.016	67.1	0.28	0.02	-	0.59	0.10	100	$0.79 \pm 0.053$
NGC 5141	...	...	<1.55	...	...	...	...	...	<5.04
NGC 5490	...	...	<1.92	...	...	...	...	...	<5.41
NGC 6251	...	...	<1.03	...	...	X	X	X	<6.78
NGC 7052^**,a	0.016	66.36	0.76	0.16	700	0.58	0.16	180	$1.96 \pm 0.41$ ^**
B2 0034+25	...	...	<0.96	...	...	...	...	...	<10.41
B2 0116+31^**,b	0.06	242.10	1.77	0.49	700	4.29	0.69	1000	$60.63 \pm 16.92$ ^**
B2 0648+27^**,a	0.04	169.83	0.72	0.07	300	1.44	0.34	350	$12.25 \pm 1.18$ ^**
B2 0836+29B^**,b	0.065	261.70	1.20	0.30	500	X	X	X	$48.18 \pm 11.95$ ^**
B2 0915+32B	...	...	<1.83	...	...	...	...	...	<70.52
B2 0924+30^*,b	0.025	104.25	0.32	0.11	200	...	...	...	$2.01 \pm 0.68$ ^*
B2 1101+38	...	...	<1.35	...	...	...	...	...	<13.09
B2 1347+28^*,b	0.072	297.9	0.35	0.08	--	0.75	0.25	500	17.04^*
B2 1357+28	...	...	<1.13	...	...	...	...	...	<48.09
B2 1447+27	...	...	<0.79	...	...	...	...	...	<7.96
B2 1512+30	...	...	<1.19	...	...	...	...	...	<110.54
B2 1525+29	...	...	<1.52	...	...	...	...	...	<69.55
B2 1553+24	...	...	<1.52	...	...	...	...	...	<29.68
UGC7115	...	...	<1.53	...	...	...	...	...	<7.66
OQ208^**,b	0.0766	304.90	2.51	0.33	400	X	X	X	$136.51 \pm 17.94^{**}$

Notes. The ^* means that this galaxy is a tentative detection, the ^** means this galaxy is detected. The letter a is for (1-0) $\&$ (2-1) detected galaxies, b is for the CO(1-0) only detected galaxy and c is for the galaxies detected in CO(2-1) only; note that in this cases the velocity with is represented as - since the CO(1-0) value was calculated using the average of the ratio and therefore the width of the line is unknown. The case of NGC 4278, that has an a^* is because this galaxy has been detected in (2-1) and tentatively detected in (1-0). In $M_{{\rm H}_2}$ the ^* have the same meaning, only that in this case refers strictly to CO(1-0) since the integrated velocity for 3 mm was the one used to calculate the molecular mass.

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