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Table 1.

Properties of the S7 subsample used in this paper.

Target RA (J2000) Dec (J2000) z Typea Seeing FWHM (arcsec)
NGC 613 01:34:18.10 −29:25:03.00 0.0049 Seyfert 2 2.2
NGC 1365 03:33:36.41 −36:08:24.00 0.0056 Seyfert 1 1.1
NGC 1672 04:45:42.19 −59:14:51.00 0.0046 SB+Seyfert 2 1.9
NGC 4303 12:21:55.40 +04:28:31.00 0.0053 SB/LINER 1.3
NGC 4691 12:48:13.01 −03:19:59.16 0.0038 SB 1.4
NGC 5990 15:46:16.49 +02:24:56.16 0.0125 SB+PSB+Seyfert 2 1.9
NGC 6000 15:49:49:60 +29:23:13.00 0.0072 SB 1.8
NGC 6221 16:52:46.00 −59:13:01.00 0.0047 SB+Seyfert 2 1.8
NGC 7469 23:03:16.00 08:52:24.50 0.0164 Seyfert 1 1.3
NGC 7496 23:09:47.3 −43:25:40.50 0.0056 SB+Seyfert 2 1.2
NGC 1068 02:42:40.70 +00:00:47.16 0.0038 Seyfert 2 1.2
NGC 1266 03:16:00.70 −02:25:37.92 0.0072 LINER 1.0
NGC 2110 05:52:11.40 −07:27:23.04 0.0078 Seyfert 2 1.4

Notes.

(a)

SB = Starburst, PSB = Post-starburst, LINER = Low-Ionization Nuclear Emitting Region

(∗)

Sample with ionized outflows inferred from the [O III]λ5007 emission line in the optical spectra of the S7 survey.

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