\begin{table}%t1
\par
%\centering
\par
\caption{\label{t1}Heliocentric redshift, position, and morphological type for
galaxies of A376, A970, A1356, and A2244.}
\begin{tabular}{lllllll}
\hline
\hline
\noalign{\smallskip}
Galaxy &  RA  &  Dec & Type & Hel. Vel. & $R$ & $N$ \\
 id.   & (2000) & (2000) &    & $V \pm {\Delta}V$  & & \\
\hline
{\bf A376} &            &           &        &         &     & \\
  1 & 02 46 29.0 & +36 27 19 &    S   & 40~451  32 &  6.53 & 1  \\
  4 & 02 46 21.0 & +36 30 43 &    E   & 39~967  26 &  5.93 & 2  \\
 10 & 02 46 40.5 & +36 35 44 &    S0  & 36~533  49 &  3.08 &    \\
 12 & 02 46 25.4 & +36 34 48 &    S0  & 13~881  59 &  3.98 &    \\
 13 & 02 46 25.3 & +36 32 24 &    S   & 15~026  61 &  5.69 & l1 \\
 14 & 02 45 47.0 & +36 35 57 &    S   & 13~526 127 &  3.05 &    \\ 
 15 & 02 45 07.6 & +36 36 49 &    S0  & 14~018  74 &  5.03 &    \\
 16 & 02 45 06.7 & +36 34 02 &    S   & 12~977  68 &  4.49 & 3  \\
 17 & 02 44 43.9 & +36 35 46 &  E/S0  & 13~638 101 &  3.22 &    \\
 19 & 02 46 47.6 & +36 40 38 &    S0  & 13~629 108 &  3.01 & weak \\
 21 & 02 45 55.6 & +36 43 14 &    S0  & 14~873  53 &  3.68 & l2 \\
 23 & 02 45 32.6 & +36 40 46 &    S   & 13~398  29 & 10.65 & 4  \\
 29 & 02 44 52.5 & +36 40 21 &    S   & 15~602  68 &  3.35 &    \\ 
 30 & 02 44 16.2 & +36 44 00 &    S   & 41~071  50 &  3.79 & 5  \\
 38 & 02 46 25.0 & +36 48 37 &    E   & 13~975 131 &  3.76 &    \\
 39 & 02 46 20.5 & +36 46 20 &  E/S0  & 15~415 100 &  3.39 &    \\
 46 & 02 44 58.9 & +36 45 54 &    S   & 14~401  49 &  4.25 & l3 \\
 47 & 02 44 53.9 & +36 47 32 &    Ep  & 14~514  60 &  3.29 & l4 \\
 48 & 02 44 44.5 & +36 45 00 &    I   & 14~702  56 &  6.69 & 6  \\
 50 & 02 44 11.1 & +36 45 36 &   S0   & 29~935  61 &  4.25 & l5 \\
 51 & 02 43 49.1 & +36 46 30 &  S0/E  & 41~546  51 &  5.49 &    \\
 53 & 02 47 31.8 & +36 49 45 &    S   & 13~701  21 &  8.87 &    \\
 56 & 02 46 54.5 & +36 53 03 &    E   & 13~897  58 &  4.69 & l6 \\
 58 & 02 46 34.2 & +36 54 19 &    S   & 16~215  66 &  4.00 & l7 \\
 59 & 02 46 28.3 & +36 51 55 &    S   & 13~310  94 &  3.49 &    \\
 62 & 02 46 19.7 & +36 50 52 &   S/I  & 13~772  73 &       & 7  \\ 
 74 & 02 45 48.7 & +36 52 28 &   S0   & 13~466  86 &  3.02 & weak \\
 77 & 02 45 41.1 & +36 52 39 &    S   & 13~553  65 &  3.03 &    \\
 79 & 02 45 33.5 & +36 51 43 &   S0   & 14~184 119 &  3.19 &    \\
 80 & 02 45 28.8 & +36 53 33 &   S0   & 14~948 118 &  3.02 &    \\
 82 & 02 45 22.6 & +36 50 32 &  S0/S  & 26~848  58 &  3.73 &    \\
 83 & 02 45 16.5 & +36 50 45 &   S0   & 15~265  35 & 12.35 & 8  \\
 87 & 02 44 16.6 & +36 54 49 &   S0   & 12~072  78 &  4.03 & 9  \\
 99 & 02 45 47.9 & +36 59 09 &   S0   & 13~421  63 &  6.41 &    \\
105 & 02 45 09.4 & +37 00 57 &   S0   & 13~550  98 &  3.81 &    \\
107 & 02 43 54.1 & +36 57 49 &  E/S0  & 14~365  81 &  4.28 &    \\
110 & 02 45 41.9 & +37 06 05 &    E   &  9255  49 &  5.96 & l8 \\
112 & 02 43 51.6 & +37 03 30 &    S   & 13~535  88 &  2.54 & weak \\
114 & 02 46 08.5 & +37 09 49 &    S   & 13~260  98 &  3.04 & 10 \\
115 & 02 44 56.2 & +37 11 56 &    S   & 44~634  76 &  3.02 &    \\
116 & 02 44 14.2 & +37 09 24 &  E/S0  & 40~204  75 &  5.16 &    \\
117 & 02 44 18.8 & +37 08 20 &    S0  & 40~124  74 &  3.10 &    \\
118 & 02 45 38.4 & +37 18 18 &    S   & 17~561  66 &  4.32 & 11 \\
119 & 02 45 38.7 & +37 18 25 &  S0/a  & 14~587  55 &  4.29 & l9 \\ 
120 & 02 45 07.8 & +37 14 24 &    E   & 14~530  53 &  4.49 &    \\
    &            &           &        &           &       &    \\
{\bf A970}  &            &           &        &           &  & \\
 70 & 10 16 05.3 & --10 57 40 &    E   & 17~014 112 &  3.47 &    \\
 71 & 10 16 08.0 & --10 29 49 &  E/S0  & 11~033  91 &  5.70 & 12 \\
 72 & 10 16 10.8 & --10 28 28 &   S0   & 55~419  77 &  2.96 & weak \\
 73 & 10 16 14.0 & --10 31 13 &   S0   & 17~610 116 &  3.07 & l10 \\
 74 & 10 16 25.7 & --10 57 43 &  E/S0  & 18~009 154 &  3.01 & l11 \\
 75 & 10 16 31.9 & --10 37 45 &   S0   & 12~360  93 &  3.66 & l12 \\
 76 & 10 16 39.8 & --10 59 59 &    E   & 15~662  94 &  6.18 & l13 \\
 77 & 10 16 41.3 & --10 59 03 &  S0/S  & 47~793  60 &  3.04 &    \\ 
 78 & 10 17 17.5 & --11 07 50 &   S0   & 17~709  83 &  4.26 &    \\
 79 & 10 18 53.9 & --10 49 25 &    S   & 19~173  17 &       & 13 \\
 80 & 10 18 59.0 & --10 54 02 &    E   &  2701  23 &       & 14 \\
 81 & 10 19 09.6 & --10 58 39 &    S   & 19~404  32 &       & 15 \\
 82 & 10 19 13.7 & --10 22 31 &    E   & 33~248  50 &  3.32 &    \\
 83 & 10 19 16.2 & --10 22 09 &  S0/S  & 16~887 111 &  3.01 & weak \\
{\bf A1356} &            &           &        &           &  & \\
  1 & 11 42 04.8 & +10 21 49 &    S   &  6395  43 &  5.19 & l14 \\
  2 & 11 42 08.7 & +10 27 19 &    S   & 21~030  82 &  3.63 &    \\     %ok
  3 & 11 42 15.3 & +10 26 50 &    E   & 35~166  27 & 11.75 & l15 \\
  4 & 11 42 22.3 & +10 44 19 &    S   & 23~753  45 &  8.93 & l16 \\
  5 & 11 42 23.7 & +10 26 09 &    E   & 21~474  54 &  6.96 & 16  l29 \\
  6 & 11 42 24.4 & +10 40 04 &    S   & 23~794  79 &  6.70 & l17 \\
  7 & 11 42 29.6 & +10 29 24 &    S   & 20~910  75 &  6.27 &    \\    %ok
  8 & 11 42 29.7 & +10 28 31 &   S0   & 20~702  51 & 10.56 & l18 \\
  9 & 11 42 31.7 & +10 25 24 &    S   & 10~655  75 &  5.61 & 17  l30\\
 10 & 11 42 43.4 & +10 31 00 &    E   & 36~132  74 &  3.62 & weak  l31 \\
    &            &           &        &        &          &    \\
{\bf A2244} &            &           &        &           &  & \\
  1 & 17 02 16.7 & +33 58 49 &    S   & 29~626  39 & 10.37 & l19 \\
  2 & 17 02 25.9 & +33 59 54 &   S0   & 29~062  32 & 11.18 & l20 \\
  3 & 17 02 42.5 & +34 03 38 &   S0   & 29~811  46 &  9.50 & l21 \\
  4 & 17 02 45.6 & +34 03 39 &    ?   & 27~984  66 &  8.67 & l22 \\
  5 & 17 03 23.5 & +34 06 49 &    S   & 11~080  25 & 12.40 & 18 l23 \\
  6 & 17 04 03.3 & +33 55 19 &    S   & 11~144  39 & 10.96 & l24 \\
  7 & 17 04 04.1 & +34 15 29 &   S0   & 30~606  73 &  6.83 & l25 \\
  8 & 17 04 14.4 & +34 15 03 &    S   & 12~180  80 &  6.39 & 19 l26 \\
  9 & 17 04 45.9 & +34 06 34 &   S0   & 30~707  58 &  8.76 & l27 \\
 10 & 17 04 50.1 & +34 05 29 &    S   &  9959  58 &  7.29 & 20 l28 \\ 
\hline
\end{tabular}
\tablefoot{Data from NED: \\
{\bf l1}~$15~130\kms$; {\bf l2}~$14~958\kms$; {\bf l3}~$14~590\kms$;
{\bf l4}~$14~466\kms$; {\bf l5}~$29~892\kms$; {\bf l6}~$13~988\kms$;
{\bf l7}~$16~273\kms$; {\bf l8}~$9324\kms$; {\bf l9}~$14~765\kms$;
{\bf l10}~$17~631\kms$; {\bf l11}~$18~067\kms$; {\bf l12}~$12~098\kms$; 
{\bf l13}~$15~782\kms$; {\bf l14} NGC~3819 $6274\kms$;
{\bf l15}~$35~155\kms$; {\bf l16}~$23~768\kms$; {\bf l17}~$23~789\kms$;
{\bf l18}~$20~773\kms$; {\bf l19}~$29~585\kms$; {\bf l20}~$29~046\kms$; 
{\bf l21}~$29~652\kms$; {\bf l22}~$27~955\kms$; {\bf l23}~$11~121\kms$; 
{\bf l24}~$11~156\kms$; {\bf l25}~$30~655\kms$; {\bf l26}~$12~110\kms$; 
{\bf l27}~$30~809\kms$; {\bf l28}~$9908\kms$; {\bf l29}~$21~288\kms$; 
{\bf l30}~$10~601\kms$; {\bf l31}~$36~047\kms$.\\[2mm]
%
{\bf 1}  emission line:  ${\rm H}\alpha= 40~498\kms$;  {\bf 2} emission
line:  ${\rm H}\alpha=  39~982\kms$;   {\bf 3}  emission  line:  ${\rm H}\alpha=
13~072\kms$;   {\bf 4}~emission  line:   ${\rm H}\beta$,  2O\textsc{iii},
${\rm H}\alpha,  S2$;   {\bf 5}  emission  line:   ${\rm H}\alpha=  41~167\kms$;
{\bf 6}~emission line:  ${\rm H}\alpha= 14~829\kms$;  {\bf 7} emission
line:   O\textsc{ii},   ${\rm H}\beta$,   2O\textsc{iii},   ${\rm H}\alpha,   S1$;
{\bf 8}  emission   line:  ${\rm H}\alpha,  S2=   15~478\kms$;  {\bf 9}
emission  line:  ${\rm H}\alpha=   12~066\kms$;  {\bf 10}  emission  line:
${\rm H}\alpha= 13~267\kms$; {\bf 11} emission line: ${\rm H}\alpha= 17~652\kms$;
{\bf 12} emission line:  ${\rm H}\alpha= 11~058\kms$; {\bf 13} emission
line: ${\rm H}\alpha$; {\bf 14} emission lines: 2O\textsc{iii}, ${\rm H}\alpha,
S1$; {\bf 15} emission line: ${\rm H}\alpha$; {\bf 16} emission lines:
O\textsc{ii},  O\textsc{iii},  ${\rm H}\alpha$,   $N2=  21~398  \pm  68\kms$;
{\bf 17}  emission  lines:   2O\textsc{iii},  ${\rm H}\alpha=  10~684  \pm
35\kms$;  {\bf 18}  emission   lines:  ${\rm H}\alpha,  N2$;  {\bf 19}~emission  line:  ${\rm H}\alpha$;   {\bf 20}  emission  lines:  ${\rm H}\beta$,
2O\textsc{iii}, ${\rm H}\alpha, N1, N2, S1, S2$.}
\end{table}