The M•–σe relation for local type 1 AGNs and quasars

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Volume 691 (November 2024)

A&A, 691 (2024) A114

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Table A.1.

Basic parameters of the sample.

Object	R.A.	Decl.	z	D_L	Morphology	log M_*	log M_•	$log λ L_{λ} (5100 Å)$ $\log \lambda L_\lambda(5100\,\mathrm{\AA})$	R_e		n	B/T
	(J2000.0)	(J2000.0)		(Mpc)		(M_⊙)	(M_⊙)	(erg s⁻¹)	(″)	(kpc)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)		(11)	(12)

Palomar-Green Quasars
PG 0050+124	00:53:34.94	+12:41:36.2	0.0611	282	Disk	11.12 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	7.57	44.76	1.33	1.62	1.7	0.52
PG 0923+129	09:26:03.29	+12:44:03.6	0.0287	131	Disk	10.71 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	7.52	43.83	1.01	0.60	1.0	0.37
PG 0934+013	09:37:01.05	+01:05:43.2	0.0506	230	Disk	10.38 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	7.15	43.85	0.57	0.58	0.5	0.05
PG 1011−040	10:14:20.69	−04:18:40.5	0.0584	268	Disk	10.87 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	7.43	44.23	0.84	0.98	2.8	0.14
PG 1126−041	11:29:16.66	−04:24:07.6	0.0601	278	Disk	10.85 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	7.87	44.36	0.66	0.79	4.0	0.37
PG 1211+143	12:11:17.67	+14:03:13.2	0.0815	400	Disk	10.38 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	8.10	45.04	0.95	1.51	5.8	0.72
PG 1244+026	12:46:35.25	+02:22:08.8	0.0484	220	Disk	10.19 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	6.62	43.77	0.10	0.10	1.0	0.03
PG 1426+015	14:29:06.57	+01:17:06.2	0.0866	401	Merger	11.05 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	9.15	44.85	0.98	1.64	4.0	1.0
PG 2130+099	21:32:27.81	+10:08:19.5	0.0631	292	Disk	10.85 $_{- 0.3}^{+ 0.3}$ $^{+0.3}_{-0.3}$	8.04	44.54	2.26	2.83	4.0	0.33

CARS AGNs

HE 0021−1810	00:23:39.34	−17:53:54.6	0.0537	247	Spheroidal	10.64 $_{- 0.05}^{+ 0.04}$ $^{+0.04}_{-0.05}$	7.81	42.82	...	...	...	...
HE 0021−1819	00:23:55.29	−18:02:51.0	0.0533	245	Disk	10.50 $_{- 0.05}^{+ 0.04}$ $^{+0.04}_{-0.05}$	7.10	42.80	1.9	2.04	1.4	0.33
HE 0040−1105	00:42:36.76	−10:49:22.4	0.0419	191	Spheroidal	10.16 $_{- 0.10}^{+ 0.13}$ $^{+0.13}_{-0.10}$	7.43	43.13	0.9	0.77	3.5	0.5
HE 0108−4743	01:11:09.68	−47:27:35.6	0.0239	108	Disk	9.77 $_{- 0.10}^{+ 0.18}$ $^{+0.18}_{-0.10}$	6.03	42.63	3.0	1.49	0.8	0.94
HE 0114−0015	01:17:03.51	+00:00:27.9	0.0458	210	Disk	10.47 $_{- 0.19}^{+ 0.13}$ $^{+0.13}_{-0.19}$	6.78	42.64	2.8	2.60	0.3	0.97
HE 0119−0118	01:21:59.76	−01:02:24.4	0.0548	253	Disk	10.91 $_{- 0.06}^{+ 0.02}$ $^{+0.02}_{-0.06}$	7.40	43.68	2.7	2.97	0.9	0.91
HE 0203−0031^*	02:06:15.97	−00:17:28.9	0.0425	194	Peculiar	10.88 $_{- 0.02}^{+ 0.02}$ $^{+0.02}_{-0.02}$	8.17	43.79	3.3	2.83	3.8	0.55
HE 0212−0059	02:14:33.58	−00:45:59.9	0.0264	119	Disk	10.59 $_{- 0.01}^{+ 0.01}$ $^{+0.01}_{-0.01}$	8.18	43.33	1.2	0.66	0.7	1.0
HE 0224−2834	02:26:25.70	−28:20:59.2	0.0602	278	Peculiar	10.13 $_{- 0.17}^{+ 0.19}$ $^{+0.19}_{-0.17}$	8.18	43.54	2.6	3.12	2.6	0.17
HE 0227−0913	02:30:05.51	−08:59:53.5	0.0165	74	Disk	9.92 $_{- 0.12}^{+ 0.17}$ $^{+0.17}_{-0.12}$	6.27	43.15	0.7	0.24	1.0	0.96
HE 0232−0900	02:34:37.79	−08:47:15.5	0.0427	195	Peculiar	10.88 $_{- 0.12}^{+ 0.23}$ $^{+0.23}_{-0.12}$	8.05	44.05	3.7	3.22	1.4	0.33
HE 0253−1641	02:56:02.70	−16:29:14.7	0.0319	145	Disk	10.28 $_{- 0.24}^{+ 0.11}$ $^{+0.11}_{-0.24}$	6.64	43.16	3.3	2.17	0.9	0.80
HE 0345+0056	03:47:40.17	+01:05:14.8	0.0310	140	Spheroidal	8.85 $_{- 0.26}^{+ 0.62}$ $^{+0.62}_{-0.26}$	6.92	43.97	1.3	0.83	2.0	0.06
HE 0351+0240	03:54:09.48	+02:49:31.3	0.0354	161	Peculiar	9.85 $_{- 0.70}^{+ 0.34}$ $^{+0.34}_{-0.70}$	7.48	43.23	1.5	1.09	5.2	0.09
HE 0412−0803	04:14:52.65	−07:55:40.4	0.0380	173	Spheroidal	10.08 $_{- 0.12}^{+ 0.10}$ $^{+0.10}_{-0.12}$	7.73	43.82	1.7	1.32	1.8	0.33
HE 0429−0247	04:31:37.12	−02:41:23.4	0.0423	193	Uncertain	9.18 $_{- 0.10}^{+ 0.51}$ $^{+0.51}_{-0.10}$	6.61	43.35	0.9	0.78	0.7	0.86
HE 0433−1028	04:36:22.30	−10:22:33.1	0.0355	161	Disk	10.80 $_{- 0.09}^{+ 0.08}$ $^{+0.08}_{-0.09}$	7.35	43.77	10.1	7.37	0.2	0.83
HE 0853+0102	08:55:54.25	+00:51:11.9	0.0526	241	Disk	10.54 $_{- 0.10}^{+ 0.04}$ $^{+0.04}_{-0.10}$	7.25	42.99	0.9	1.07	0.8	0.86
HE 0949−0122	09:52:19.05	−01:36:43.7	0.0197	88	Spheroidal	10.02 $_{- 0.31}^{+ 0.09}$ $^{+0.09}_{-0.31}$	6.58	42.72	1.5	0.62	3.5	0.05
HE 1017−0305	10:19:32.84	−03:20:14.6	0.0491	225	Disk	10.93 $_{- 0.15}^{+ 0.10}$ $^{+0.10}_{-0.15}$	8.18	43.71	3.8	3.77	2.2	0.28
HE 1029−1831	10:31:57.33	−18:46:32.7	0.0405	185	Disk	10.49 $_{- 0.18}^{+ 0.06}$ $^{+0.06}_{-0.18}$	7.06	43.30	2.1	1.74	0.7	0.50
HE 1107−0813	11:09:48.50	−08:30:14.7	0.0585	270	Disk	11.17 $_{- 0.38}^{+ 0.20}$ $^{+0.20}_{-0.38}$	8.14	44.11	1.4	1.64	3.0	0.39
HE 1108−2813	11:10:47.99	−28:30:04.1	0.0240	108	Disk	10.29 $_{- 0.05}^{+ 0.11}$ $^{+0.11}_{-0.05}$	7.06	43.04	5.8	2.90	0.2	0.99
HE 1237−0504	12:39:39.42	−05:20:38.5	0.0083	37	Disk	10.92 $_{- 0.01}^{+ 0.01}$ $^{+0.01}_{-0.01}$	7.07	42.64	5.5	0.97	1.5	0.97
HE 1248−1356	12:51:32.39	−14:13:16.1	0.0145	65	Disk	10.31 $_{- 0.01}^{+ 0.01}$ $^{+0.01}_{-0.01}$	6.58	41.93	1.1	0.34	1.5	0.99
HE 1330−1013	13:32:39.15	−10:28:52.4	0.0225	101	Disk	10.69 $_{- 0.13}^{+ 0.03}$ $^{+0.03}_{-0.13}$	6.49	42.75	8.3	3.90	1.8	0.44
HE 1353−1917	13:56:36.77	−19:31:44.9	0.0348	158	Disk	10.99 $_{- 0.06}^{+ 0.03}$ $^{+0.03}_{-0.06}$	8.20	43.10	11.4	8.16	2.7	0.01
HE 1417−0909	14:20:06.34	−09:23:12.8	0.0437	200	Disk	10.23 $_{- 0.17}^{+ 0.10}$ $^{+0.10}_{-0.17}$	7.37	43.44	2.2	1.96	0.6	1.0
HE 2128−0221	21:30:49.96	−02:08:14.0	0.0527	242	Disk	9.93 $_{- 0.67}^{+ 0.21}$ $^{+0.21}_{-0.67}$	6.71	43.02	2.1	2.23	1.7	0.01
HE 2211−3903	22:14:42.06	−38:48:22.7	0.0397	181	Disk	9.83 $_{- 0.21}^{+ 0.22}$ $^{+0.22}_{-0.21}$	7.81	43.32	11.0	8.93	0.2	0.94
HE 2222−0026	22:24:35.22	−00:11:03.4	0.0581	268	Disk	10.20 $_{- 0.15}^{+ 0.09}$ $^{+0.09}_{-0.15}$	7.28	43.41	1.1	1.28	1.1	0.50
HE 2233+0124	22:35:41.94	+01:39:34.5	0.0567	262	Disk	10.71 $_{- 0.03}^{+ 0.10}$ $^{+0.10}_{-0.03}$	8.63	43.48	2.5	2.84	8.3	0.44
HE 2302−0857	23:04:43.70	−08:41:08.3	0.0470	215	Disk	11.20 $_{- 0.13}^{+ 0.09}$ $^{+0.09}_{-0.13}$	8.54	43.93	3.9	3.72	5.5	0.39

Notes. (1) Source name. (2) Right ascension. (3) Declination. (4) Redshift. (5) Luminosity distance. (6) Morphological type of the host galaxy. For the PG quasars, we adopt the results of Kim et al. (2017), Zhang et al. (2016), and Zhao et al. (2021); for the CARS AGNs, we follow Husemann et al. (2022), but we relabel their “irregular" category to “peculiar" to avoid confusion with the “dwarf irregular" systems. We also relabel their “bulge-dominated” category to simply “spheroidal.” (7) Host galaxy stellar mass (Zhao et al. 2021; Smirnova-Pinchukova et al. 2022). (8) Black hole mass, based on the calibration of Ho & Kim (2015); the 1σ uncertainty is ∼0.32 − 0.38 dex (Section 3.6). (9) AGN monochromatic luminosity at 5100 Å; for the CARS data, the values were derived from the broad Hβ luminosity following Greene & Ho (2005b). (10) Bulge effective radius. (11) Bulge Sérsic (1963) index. (12) Bulge-to-total (B/T) light fraction. The bulge properties for the PG quasars are obtained from optical and near-IR HST image modeling (Veilleux et al. 2009; Kim et al. 2017; Zhao et al. 2021), while for the CARS AGNs we adopt the MUSE-based i−band image models of Husemann et al. (2022), assuming the Sérsic model subcomponent with smaller R_e value. (*) For this target, the AGN optical spectrum and bulge properties were derived by Bennert et al. (2011) and Bennert et al. (2021), respectively.

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