Table 1: The complete, distance-limited sample of Seyfert galaxies.
Galaxy Other Seyfert Hubble Distance BT RA Dec
name name type type (Mpc) (mag) (J2000) (J2000)
(1) (2) (3) (4) (5) (6) (7) (8)
NGC 676   S2: S0/a: spin 19.5 10.50 01 48 57.4 +05 54 25.7
NGC 1058   S2 Sc 9.1 11.82 02 43 30.2 +37 20 27.2
NGC 1068   S1.9 Sb 14.4 9.61 02 42 40.7 -00 00 47.6
NGC 2685 Arp336 S2/T2: SB0+ pec 16.2 12.12 08 55 34.8 +58 44 01.6
NGC 3031 M81 S1.5/L1.5 Sab 3.5a 7.89 09 55 33.2 +69 03 55.0
NGC 3079   S2 SBc spin 17.3b 11.54 10 01 58.5 +55 40 50.1
NGC 3185   S2: SB0/a 21.3 12.99 10 17 38.7 +21 41 17.2
NGC 3227 Arp94 S1.5 SABa pec 20.6 11.10 10 23 30.6 +19 51 53.9
NGC 3486   S2 SABc 7.4 11.05 11 00 24.1 +28 58 31.6
NGC 3941   S2: SB0 12.2c 11.25 11 52 55.4 +36 59 10.5
NGC 4051   S1.5* SABbc 17.0 10.83 12 03 09.6 +44 31 52.8
NGC 4138   S1.9 S0+ 13.8c 12.16 12 09 29.9 +43 41 06.0
NGC 4151   S1.5 SABab: 20.3 11.50 12 10 32.6 +39 24 20.6
NGC 4258 M106 S1.9 SABbc 7.2c 9.10 12 18 57.5 +47 18 14.3
NGC 4388   S1.9 Sb: spin 16.7 11.76 12 25 46.7 +12 39 40.9
NGC 4395   S1.5* Sm: 4.1d 10.64 12 25 48.9 +33 32 47.8
NGC 4472 M49 S2:: E2 16.7 9.37 12 29 46.8 +07 59 59.9
NGC 4477   S2 SB0? 16.8 11.38 12 30 02.2 +13 38 11.3
NGC 4501 M88 S2 Sb 16.8 10.36 12 31 59.3 +14 25 13.4
NGC 4565   S1.9 Sb? spin 9.7c 10.42 12 36 21.1 +25 59 13.5
NGC 4579 M58 S1.5/L1.5* SABb 16.8 10.48 12 37 43.4 +11 49 04.9
NGC 4639   S1.5* SABbc 16.8 12.24 12 42 52.5 +13 15 24.1
NGC 4698   S2 Sab 16.8 11.46 12 48 22.9 +08 29 14.8
NGC 4725   S2: SABab pec 13.0c 10.11 12 50 26.7 +25 30 02.3
NGC 5033   S1.5 Sc 18.7 10.75 13 13 27.5 +36 35 37.8
NGC 5194 M51 S2 Sbc pec 8.4 8.96 13 29 52.4 +47 11 40.8
NGC 5273   S1.5 S0 16.5c 12.44 13 42 08.3 +35 39 15.2
Notes: Col. (1); galaxy name; Col. (2): other name; Col. (3): optical classification as given by HFS97a: "S'' represents Seyfert, "L'' represents LINER, and "T'' represents objects with LINER plus H II-region spectra. "2'' implies that no broad H$\alpha$ is detected; "1.9'' implies that broad H$\alpha$ is present, but not broad H$\beta$; "1.5'' implies that both broad H$\alpha$ and broad H$\beta$ are detected, with substantial contributions from both the BLR and NLR (Osterbrock 1981). Objects with a changed classification with respect to the original given by HFS97a (see also Ho et al. 1997b and HU01) are denoted by "*'' after their name; Col. (4): Hubble type as listed in HFS97a; Col. (5): distance from Tully (1988), except when marked with (a) Paturel et al. (2002), (b) Cecil et al. (2002), (c) Tonry et al. (2001), and (d) Thim et al. (2004); Col. (6): total apparent BT magnitude of the galaxy; Cols. (7)-(8): nuclear optical position in epoch J2000 as given by HU01. N.B: Two sources (NGC 3031 and NGC 4579) have classifications which fall near the somewhat arbitrary boundary between a Seyfert and a LINER, depending on the adopted criteria. Because they are on the Seyfert side in HFS97a, they are included here and classified as "S/L''. In objects like NGC 676, NGC 2685, NGC 3185, NGC 4472, and NGC 4725, the starlight subtraction process has been particularly difficult, leading to uncertain classifications. Following HFS97b, we marked these sources with a quality rating ":'' (uncertain) or "::'' (highly uncertain).

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