The relation between black hole spin, star formation rate, and black hole mass for supermassive black holes

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Table A.1.

The sample of supermassive black holes.

Name	redshift	log L_IR	log SFR	log M_*/M_⊙	log M_BH/M_⊙	a	Mass/spin Reference
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)
Mrk 359	0.0168	43.846	0.499	9.677±0.03	6.041	0.66 $_{- 0.54}^{+ 0.30}$ $_{-0.54}^{+0.30}$	Bambi21
Ark564	0.0247	43.836	0.489	8.842±0.06	6.041	0.96 $_{- 0.06}^{+ 0.01}$ $_{-0.06}^{+0.01}$	Rey21
Mrk 766	0.01288	43.999	0.653	8.031±0.04	6.54 $_{- 0.04}^{+ 0.05}$ $_{-0.04}^{+0.05}$	> 0.92	Bambi21
NGC 4051	0.00234	43.07	-0.274	7.913±0.03	6.281 $_{- 0.18}^{+ 0.18}$ $_{-0.18}^{+0.18}$	> 0.99	Rey21
NGC 1365	0.00546	44.612	1.265	9.655±0.02	7.81 $_{- 0.23}^{+ 0.53}$ $_{-0.23}^{+0.53}$	> 0.97	Bambi21
1H0707-495	0.041	43.297	-0.048	7.522±0.1	5.81 $_{- 0.04}^{+ 0.05}$ $_{-0.04}^{+0.05}$	> 0.988	Bambi21
MCG-6-30-15	0.00775	42.548	-0.798	8.522±0.07	6.462 $_{- 0.24}^{+ 0.27}$ $_{-0.24}^{+0.27}$	0.91 $_{- 0.07}^{+ 0.06}$ $_{-0.07}^{+0.06}$	Rey21
NGC5506	0.00608	43.209	-0.137	7.022±0.04	6.70 $_{- 0.10}^{+ 0.19}$ $_{-0.10}^{+0.19}$	0.93 $_{- 0.04}^{+ 0.04}$ $_{-0.04}^{+0.04}$	Bambi21
IRAS 13224-3809	0.0658	45.127	1.78	9.411±0.02	5.87 $_{- 0.14}^{+ 0.12}$ $_{-0.14}^{+0.12}$	> 0.975	Bambi21
TON S180	0.062	44.056	0.709	9.46±0.08	6.908	> 0.98	Rey21
ESO 362-G18	0.0124	43.559	0.212	9.251±0.03	7.097 $_{- 0.16}^{+ 0.16}$ $_{-0.16}^{+0.16}$	> 0.92	Rey21
Swift J2127.4+5654	0.0147	44.034	0.687	9.601±0.02	7.18 $_{- 0.09}^{+ 0.09}$ $_{-0.09}^{+0.09}$	0.58 $_{- 0.17}^{+ 0.11}$ $_{-0.17}^{+0.11}$	Bambi21
Mrk 335	0.02578	43.716	0.369	9.669±0.05	7.15 $_{- 0.11}^{+ 0.11}$ $_{-0.11}^{+0.11}$	0.99 $_{- 0.03}^{+ 0.01}$ $_{-0.03}^{+0.01}$	Bambi21
Mrk 110	0.0353	43.3	-0.046	9.22±0.11	7.4 $_{- 0.11}^{0.11}$ $_{-0.11}^{0.11}$	> 0.99	Rey21
NGC 3783	0.00973	43.725	0.378	9.2±0.02	7.474 $_{- 0.08}^{+ 0.08}$ $_{-0.08}^{+0.08}$	> 0.88	Rey21
1H0323+342	0.0629	45.156	1.809	10.017±0.06	7.531 $_{- 0.08}^{+ 0.12}$ $_{-0.08}^{+0.12}$	> 0.9	Rey21
NGC 4151	0.0033	42.78	-0.566	9.421±0.06	7.12 $_{- 0.15}^{+ 0.15}$ $_{-0.15}^{+0.15}$	0.98 $_{- 0.01}^{+ 0.01}$ $_{-0.01}^{+0.01}$	Bambi21
Mrk 79	0.022	44.192	0.846	9.957±0.02	7.72 $_{- 0.12}^{+ 0.12}$ $_{-0.12}^{+0.12}$	> 0.5	Bambi21
PG1229+204	0.0636	44.19	0.843	10.045±0.06	7.756 $_{- 0.22}^{+ 0.22}$ $_{-0.22}^{+0.22}$	0.93 $_{- 0.02}^{+ 0.06}$ $_{-0.02}^{+0.06}$	Rey21
IRAS13197-1627	0.01654	44.419	1.072	9.011±0.02	7.806	> 0.7	Rey21
3C120	0.033	44.55	1.207	10.08±0.02	7.839 $_{- 0.15}^{+ 0.20}$ $_{-0.15}^{+0.20}$	> 0.95	Rey21
Mrk 841	0.03642	43.996	0.649	9.355±0.07	7.897 $_{- 0.01}^{+ 0.01}$ $_{-0.01}^{+0.01}$	> 0.52	Bambi21
IRAS09149-6206	0.0573	44.76	1.413	10.824±0.06	8.00 $_{- 0.3}^{+ 1.3}$ $_{-0.3}^{+1.3}$	0.94 $_{- 0.07}^{+ 0.02}$ $_{-0.07}^{+0.02}$	Bambi21
Ark120	0.0327	44.196	0.85	10.464±0.04	8.176 $_{- 0.06}^{+ 0.06}$ $_{-0.06}^{+0.06}$	0.83 $_{- 0.03}^{+ 0.05}$ $_{-0.03}^{+0.05}$	Bambi21
RBS1124	0.208	43.714	0.367	8.5±0.31	8.26 $_{- 0.10}^{+ 0.10}$ $_{-0.10}^{+0.10}$	> 0.97	Bambi21
1RXS J113155.4-123155	0.654	47	3.657	11.73±0.02	8.30 $_{- 0.09}^{+ 0.09}$ $_{-0.09}^{+0.09}$	0.87 $_{- 0.15}^{+ 0.08}$ $_{-0.15}^{+0.08}$	Bambi21
Fairall 9	0.046	44.188	0.841	9.151±0.07	8.407 $_{- 0.10}^{+ 0.10}$ $_{-0.10}^{+0.10}$	> 0.997	Bambi21
1H0419-577	0.104	44.517	1.171	9.821±0.07	8.11 $_{- 0.10}^{+ 0.10}$ $_{-0.10}^{+0.10}$	> 0.96	Bambi21
PG0804+761	0.1005	44.839	1.492	11.095±0.02	8.74 $_{- 0.05}^{+ 0.05}$ $_{-0.05}^{+0.05}$	> 0.97	Rey21
Q 2237+0305	1.695	48.0224	4.675	13.213±0.02	9.0 $_{- 0.09}^{+ 0.09}$ $_{-0.09}^{+0.09}$	0.74 $_{- 0.03}^{+ 0.06}$ $_{-0.03}^{+0.06}$	Bambi21
PG2112+059	0.459	45.643	2.296	10.595±0.1	9.0 $_{- 0.09}^{+ 0.09}$ $_{-0.09}^{+0.09}$	> 0.86	Bambi21
H1821+643	0.297	46.417	3.07	11.178±0.04	9.653 $_{- 0.14}^{+ 0.14}$ $_{-0.14}^{+0.14}$	> 0.4	Rey21
IRAS 00521-7054	0.069	45.084	1.737	10.278±0.02	7.698 $_{- 0.09}^{+ 0.09}$ $_{-0.09}^{+0.09}$	> 0.77	Bambi21
IRAS13349+2438	0.108	45.274	1.927	11.368±0.02	7.00 $_{- 0.17}^{+ 0.09}$ $_{-0.17}^{+0.09}$	0.80 $_{- 0.5}^{+ 0.2}$ $_{-0.5}^{+0.2}$	Bambi21
Fairall 51	0.0142	43.585	0.238	8.845±0.06	8.00 $_{- 0.09}^{+ 0.09}$ $_{-0.09}^{+0.09}$	0.80 $_{- 0.2}^{+ 0.2}$ $_{-0.2}^{+0.2}$	Bambi21
Mrk 1501	0.087	44.33	0.983	10.06±0.07	8.26 $_{- 0.06}^{+ 0.06}$ $_{-0.06}^{+0.06}$	> 0.98	Bambi21
Mrk 1018	0.043	43.021	-0.325	6.873±0.3	7.81	0.58 $_{- 0.74}^{+ 0.36}$ $_{-0.74}^{+0.36}$	Kos22/Vas16
Mrk 509	0.034	43.825	0.478	9.823±0.12	8.15 $_{- 0.04}^{+ 0.04}$ $_{-0.04}^{+0.04}$	> 0.993	Bambi21
3C382	0.055	44.174	0.827	10.864±0.06	8.01 $_{- 0.05}^{+ 0.09}$ $_{-0.05}^{+0.09}$	0.75 $_{- 0.04}^{+ 0.07}$ $_{-0.04}^{+0.07}$	Lu19/Wal13
PKS 0558-504	0.137	45.17	1.823	9.812±0.05	7.62	> 0.8	Kos22/Wal13
NGC 7469	0.016	45.14	1.794	9.59±0.04	6.42 $_{- 0.09}^{+ 0.06}$ $_{-0.09}^{+0.06}$	> 0.96	Lu19/Wal13
PDS 456	0.185	45.154	1.808	9.884±0.02	8.4	> 0.97	Wil18/Wal13
UGC 6728	0.0065	42.758	-0.588	7.951±0.05	5.55 $_{- 0.25}^{+ 0.22}$ $_{-0.25}^{+0.22}$	> 0.95	Lu19/Wal13
1H1934-063	0.01	43.778	0.431	9.223±0.02	6.477	> 0.45	Xu22/Jia19
Mrk 279	0.03	44.293	0.946	10.433±0.02	7.97 $_{- 0.12}^{+ 0.09}$ $_{-0.12}^{+0.09}$	> 0.95	Lu19/Jia19
Mrk 590	0.0263	44.058	0.711	10.492±0.02	7.55 $_{- 0.07}^{+ 0.05}$ $_{-0.07}^{+0.05}$	> 0.1	Lu19/Jia19
NGC 4748	0.0146	43.677	0.331	8.904±0.03	6.61 $_{- 0.23}^{+ 0.11}$ $_{-0.23}^{+0.11}$	> 0.8	Lu19/Jia19
PG 0844+349	0.064	43.308	-0.037	7.045±0.28	8.35 $_{- 0.26}^{+ 0.26}$ $_{-0.26}^{+0.26}$	> 0.95	Afa19/Jia19

Notes. Columns (1) is the name of the sources; Columns (2) is the redshift; Columns (3) is the torus-subtracted IR luminosity in the 8–1000 μm band in units erg s⁻¹; Columns (4) is SFR calculated from the torus-subtracted IR luminosity in the 8–1000 μm band, units M_⊙yr⁻¹; Columns (5) is stellar mass; Columns (6) is the black hole mass; Columns (7) is the black hole spin; Columns (8) is the reference of black hole mass and spin. Rey21=Reynolds (2021); Bambi21=Bambi et al. (2021); Afa19=Afanasiev et al. (2019); Kos22=Koss et al. (2022); Vas16=Vasudevan et al. (2016); Wal13=Walton et al. (2013); Lu19=Lu et al. (2019); Xu22=Xu et al. (2022); Jia19=Jiang et al. (2019). Some of the sources in the samples of Reynolds (2021) were updated from Bambi et al. (2021).

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