\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}