Parsec-scale dust distributions in Seyfert galaxies - Results of the MIDI AGN snapshot survey

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Volume 502 / No 1 (July IV 2009)

A&A, 502 1 (2009) 67-84

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Table 3:

Characteristics derived from the interferometric observations of the AGN in the snapshot survey (marked by asterisks) and other AGN studied by MIDI.
	Galaxy		D	${\rm BL}$	$F_{{\rm tot}, 12~{\rm\mu m}}$	$F_{{\rm cor, 12~{\rm\mu m}}}$	$s_{12~{\rm\mu m}}$
	name	type	[Mpc]	[m]	[Jy]	[Jy]	[pc]
	(1)	(2)	(3)	(4)	(5)	(6)	(7)
	NGC 1068	Sy 2	14	33.6	16.50	4.00	3.2
	NGC 1068	Sy 2	14	79.9	16.50	1.20	1.8
*	NGC 1365	Sy 1.8	18	46.6	0.51	0.28	2.0
*	NGC 1365	Sy 1.8	18	54.4	0.34	0.25	2.7
*	NGC 1365	Sy 1.8	18	62.3	0.47	0.32	1.1
*	MCG-05-23-016	Sy 2	35	46.1	0.60	0.35	2.8
*	Mrk 1239	Sy 1.5	80	43.0	0.57	0.48	7.0
	NGC 3783	Sy 1	40	68.6	1.25	0.50	3.6
	NGC 3783	Sy 1	40	64.9	1.02	0.54	3.1
*	NGC 4151	Sy 1.5	14	35.8	1.21	0.27	2.6
*	3C 273	QSO	650	36.7	0.32	0.32	67.
*	3C 273	QSO	650	29.7	0.29	0.20	108.
*	IC 4329A	Sy 1.2	65	46.6	1.00	0.75	10.8
	Circinus	Sy 2	4	20.7	10.20	1.80	1.5
	Circinus	Sy 2	4	62.4	10.20	1.10	0.6
*	NGC 7469	Sy 1.2	65	46.4	0.70	0.17	10.5

Notes: the columns are (1) the name; (2) the type and (3) the distance of the galaxy (all repeated from Table 1); (4) the baseline length for the respective observation; (5) the total and (6) correlated fluxes at $12~\mu{\rm m}$ as well as (7) the approximate size of the emitter at $12~\mu{\rm m}$ .

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