Continuum reverberation mapping of accretion disks depending on the vertical structures in active galactic nuclei

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Volume 695 (March 2025)

A&A, 695 (2025) A143

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Table 1.

Comparison with observations.

Objects	Redshift	RA	Dec	log(M_•/M_⊙)	$\dot{M}$ ${\dot{\mathscr{M}}}$	${\dot{M}}_{crit}$ ${\dot{\mathscr{M}}}_{\mathrm{crit}}$	ratio	Disk-RM Ref.	SED Ref.
Mrk 335	0.025	00 06 19.5	+20 12 10.6	6.93	–	0.03	∼6	1	2
Fairall 9	0.047	01 23 45.8	–58 48 20.8	8.09	2.0	0.5	3.5	3	4
Ark 120^*	0.032	05 16 11.4	–00 08 59.2	8.47	0.06	1.09	2.0	5	6
MCG +08-11-011^*	0.020	05 54 53.6	+46 26 21.6	7.72	0.15	0.19	1.9	7	8
NGC 2617^*	0.014	08 35 38.8	–04 05 17.9	7.74	0.03	0.20	1.5 − 2	7	7
Mrk 110	0.035	09 25 12.8	+52 17 10.4	7.10	10.0	0.05	1.5	9	6
Mrk 817	0.032	14 36 22.1	+58 47 39.4	7.99	1.5	0.4	1.5 − 2	10	6
NGC 4151	0.003	12 10 32.6	+39 24 21.1	7.56	0.5	0.1	2	11	6
NGC 4593	0.001	12 39 39.4	–05 20 39.0	7.26	0.09	0.07	1.5 − 2.5	12	2
NGC 5548^*	0.016	14 17 59.5	+25 08 12.6	8.08	0.3	0.44	1.5 − 3	4	4
Mrk 509	0.035	20 44 09.8	–10 43 24.7	8.15	0.5	0.5	1.5 − 2	11	6, 13
NGC 7469	0.017	23 03 15.6	+08 52 26	7.60	1.1	0.2	1.5 − 2.5	14	6

Notes. ${\dot{M}}_{crit}$ ${\dot{\mathscr{M}}}_{\mathrm{crit}}$ is the criteria dimensionless accretion rate ${\dot{M}}_{crit} = 0.37 M_{8}$ ${\dot{\mathscr{M}}}_{\mathrm{crit}} = 0.37 M_8$ and AGNs marked with * indicate those with accretion rates less than this criteria. References: (1) Kara et al. (2023), (2) Grupe et al. (2010), (3) Hernández Santisteban et al. (2020), (4) Fausnaugh et al. (2016), (5) Lobban et al. (2020), (6) Brown et al. (2019), (7) Fausnaugh et al. (2018), (8) Fian et al. (2023), (9) Vincentelli et al. (2021), (10) Kara et al. (2021), (11) Edelson et al. (2019), (12) Cackett et al. (2018), (13) Kaastra et al. (2011), (14) Pahari et al. (2020).

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