CO in the ALMA Radio-source Catalogue (ARC): The molecular gas content of radio galaxies as a function of redshift

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Table C.1.

CO properties of 54 literature-based sources.

Galaxy	z	log(M_H₂)	log(L’_CO(1−0))	f_1.4GHz	reference
		(M_⊙)	(K km s⁻¹ pc²)	(Jy)
NGC1399	0.005	7.47	6.83	0.639	Prandoni et al. 2010
IC1459	0.006	< 6.00	< 5.36	0.840	Ruffa et al. 2019
NGC4696	0.010	7.95	7.31	3.922	Olivares et al. 2019
NGC3801	0.011	8.74	8.10	1.141	Ocaña-Flaquer et al. 2010
NGC7626	0.011	< 7.90	< 7.26	0.627	Leon et al. 2002
NGC 193	0.014	< 8.08	< 7.44	1.375	Leon et al. 2002
J0048+3157	0.015	< 8.73	< 8.09	0.401	Taniguchi et al 1990
NGC5127	0.015	7.90	7.26	0.500	Ocaña-Flaquer et al. 2010
NGC5490	0.016	< 8.73	< 8.09	0.971	Ocaña-Flaquer et al. 2010
NGC5141	0.018	< 8.70	< 8.06	0.638	Ocaña-Flaquer et al. 2010
NGC541	0.018	8.40	7.76	0.826	Ocaña-Flaquer et al. 2010
NGC741	0.019	< 8.74	< 8.10	0.635	Evans et al. 2005
NGC2329	0.019	< 8.15	< 7.51	0.512	Leon et al. 2002
IC1531	0.026	8.04	7.40	0.505	Ruffa et al. 2019
3C442	0.026	7.83	7.19	2.216	Ocaña-Flaquer et al. 2010
PKS0718-34	0.028	< 6.83	< 6.19	1.909	Ruffa et al. 2019
3C465	0.030	< 8.89	< 8.25	6.134	Ocaña-Flaquer et al. 2010
ESO422-G028	0.038	< 10.05	< 9.41	1.500	Saripalli et al. 2007
Arp187	0.040	10.07	9.43	1.461	Evans et al. 2005
J0758+3747	0.041	< 9.30	< 8.66	1.734	Ocaña-Flaquer et al. 2010
3C305	0.042	9.31	8.67	2.950	Ocaña-Flaquer et al. 2010
NGC326	0.048	8.75	8.11	1.231	Ocaña-Flaquer et al. 2010
J1521+0420	0.052	< 9.69	< 9.05	0.551	Evans et al. 2005
B21101+38	0.053	< 9.12	< 8.48	0.648	Ocaña-Flaquer et al. 2010
3C390.3	0.057	< 9.72	< 9.08	10.225	Evans et al. 2005
J0119+3210	0.059	9.78	9.14	2.483	Ocaña-Flaquer et al. 2010
4C26.42	0.063	9.51	8.87	0.925	Olivares et al. 2019
4C29.30	0.065	9.68	9.04	0.514	Ocaña-Flaquer et al. 2010
OQ208	0.077	10.14	9.50	0.703	Ocaña-Flaquer et al. 2010
B2 1707+34	0.082	< 9.72	< 9.08	0.474	Evans et al. 2005
Abell2597	0.083	9.36	8.72	1.627	Olivares et al. 2019
3C326	0.090	9.15	8.51	2.292	Nesvadba et al. 2010
3C321	0.095	9.85	9.21	3.352	Ocaña-Flaquer et al. 2010
PKS0745-191	0.102	9.69	9.05	2.003	Olivares et al. 2019
PKS1559+02	0.105	9.42	8.78	7.905	Ocaña-Flaquer et al. 2010
4C26.35	0.112	< 9.32	< 8.68	0.400	Saripalli et al. 2007
4C12.50	0.122	10.62	9.98	5.155	Fotopoulou et al. 2019
4C12.03	0.156	< 9.80	< 9.16	1.500	Saripalli et al. 2007
PKS2128-123	0.501	< 10.99	< 10.35	1.895	Lo et al. 1999
3C285	0.790	< 9.69	< 9.05	1.601	Evans et al. 2005
B0235+164	0.940	< 11.11	< 10.47	1.473	Lo et al. 1999
J0830+2410	0.941	< 11.03	< 10.39	0.841	Lo et al. 1999
3C368	1.131	< 10.90	< 10.26	1.087	Evans et al. 1996
J1022+3041	1.320	< 10.69	< 10.05	0.590	Lo et al. 1999
MRC0114-211	1.410	11.29	10.65	3.723	Emonts et al. 2014
3C68.2	1.575	< 11.39	< 10.75	0.909	Evans et al. 1996
MRC1017-220	1.768	< 11.06	< 10.42	0.539	Emonts et al. 2014
MRC0324-228	1.898	< 11.25	< 10.62	0.459	Emonts et al. 2014
MRC0152-209	1.921	11.46	10.82	0.425	Emonts et al. 2014
MRC0156-252	2.016	11.61	10.97	0.423	Emonts et al. 2014
MRC2048-272	2.060	11.58	10.94	0.485	Emonts et al. 2014
Spiderweb	2.156	11.50	10.86	0.815	Emonts et al. 2014
MRC0406-244	2.433	< 11.21	< 10.57	0.629	Emonts et al. 2014
MRC2104-242	2.491	< 11.06	< 10.42	0.447	Emonts et al. 2014

Notes. The values for the molecular mass listed here are corrected by our adopted CO-to-H₂ conversion factor. References: Prandoni et al. (2010), Ruffa et al. (2019a), Olivares et al. (2019), Ocaña Flaquer et al. (2010), Leon et al. (2003), Taniguchi et al. (1990), Evans et al. (2005), Saripalli & Mack (2007), Nesvadba et al. (2010), Fotopoulou et al. (2019), Lo et al. (1999), Evans et al. (1996) and Emonts et al. (2014).

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