\begin{table}%t1
\caption{The complete, distance-limited sample of Seyfert galaxies.\label{tab1}}
%\centerline
{\begin{tabular}{llllrrcc}
\hline
\hline
\multicolumn{1}{c}{Galaxy} &
\multicolumn{1}{c}{Other} &
\multicolumn{1}{c}{Seyfert} &
\multicolumn{1}{c}{Hubble} &
\multicolumn{1}{c}{Distance} &
\multicolumn{1}{c}{$B_{T}$} &
\multicolumn{1}{c}{RA} &
\multicolumn{1}{c}{Dec} \\
\multicolumn{1}{c}{name} &
\multicolumn{1}{c}{name} &
\multicolumn{1}{c}{type} &
\multicolumn{1}{c}{type} &
\multicolumn{1}{c}{(Mpc)} &
\multicolumn{1}{c}{(mag)} &
\multicolumn{1}{c}{(J2000)} &
\multicolumn{1}{c}{(J2000)} \\
\multicolumn{1}{c}{(1)} &
\multicolumn{1}{c}{(2)} &
\multicolumn{1}{c}{(3)} &
\multicolumn{1}{c}{(4)} &
\multicolumn{1}{c}{(5)} &
\multicolumn{1}{c}{(6)} &
\multicolumn{1}{c}{(7)} &
\multicolumn{1}{c}{(8)} \\
\hline
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   &3.5$^a$& 7.89 &   09 55 33.2  &  +69 03 55.0 \\
NGC 3079 &        & S2      & SBc spin   &17.3$^b$&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        & 12.2$^c$ & 11.25&11 52 55.4  &  +36 59 10.5  \\   
%NGC 3982 &       & S1.9    & SABb:      & 20.5 & 11.78 &   11 56 28.1  &  +55 07 31  \\   
NGC 4051 &        & S1.5$^*$    & SABbc      & 17.0 & 10.83 &   12 03 09.6  &  +44 31 52.8  \\   
NGC 4138 &        & S1.9    & S0+        & 13.8$^c$ & 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 4168 &       & S1.9:   & E2         & 31.7$^*$ & 12.11 &   12 12 17.3  &  +13 12 18 \\  
NGC 4258 & M106   & S1.9    & SABbc      &  7.2$^c$ &  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:    &  4.1$^d$ & 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   &  9.7$^c$ & 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  & 13.0$^c$ & 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         & 16.5$^c$ & 12.44&13 42 08.3  &  +35 39 15.2  \\   
\hline
\end{tabular}}
\par
\smallskip
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. (\cite{Paturel02}), ($^b$) Cecil 
et~al. (\cite{Cecil02}), ($^c$) Tonry et~al. (\cite{Tonry01}), and ($^d$) Thim et~al. (\cite{Thim04}); Col. (6):
total apparent $B_T$ 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).
\end{table}