\begin{table}%t1 \caption{\label{table:prop}The WINGS-SPE cluster sample: global properties.} %\centerline {\small \begin{tabular}{lccrccrcllcc} \noalign{\smallskip}\hline \hline\noalign{\smallskip} Cluster & RA & Dec & $N_{\rm gal}$ & $z$ & $N_{z}$ & $\sigma_W$ & $\sigma_L$ & Refs. & $\log(L_X)$ & $R_{200}$ & $A$p\\ \noalign{\smallskip} &$(J2000)$ & $(J2000)$ & & & & km~s$^{-1}$ & km~s$^{-1}$ & & $10^{44}~{\rm erg~s}^{-1}$ & Mpc & $R_{200}$\\ \noalign{\smallskip}\hline\noalign{\smallskip} A0119 & 00:56:21.37 & --01:15:46.5 & 248 & 0.0444 & 158 & 866 $^{\pm55}$ & 740 & st99 & 44.51 & 2.10 & 0.6 \\ A0151 & 01:08:52.35 & --15:25:00.9 & 269 & 0.0532 & 92 & 762 $^{\pm57}$ & 669 & st99 & 44.00 & 1.84 & 0.9 \\ A0160 & 01:12:51.40 & +15:30:53.8 & 80 & 0.0438 & 40 & 784 $^{\pm111}$ & 572 & st99 & 43.58 & 1.90 & 0.6 \\ A0193 & 01:25:07.35 & +08:41:35.9 & 62 & 0.0485 & 40 & 761 $^{\pm86}$ & 756 & st99 & 44.19 & 1.84 & 0.6 \\ A0376 & 02:45:48.53 & +36:51:35.5 & 88 & 0.0476 & 66 & 949 $^{\pm90}$ & 519 & st99 & 44.14 & 2.29 & 0.6 \\ A0500 & 04:38:54.97 & --22:05:55.3 & 140 & 0.0678 & 89 & 729 $^{\pm55}$ & $\ldots$ & $\ldots$ & 44.15 & 1.75 & 0.9 \\ A0671 & 08:28:29.28 & +30:25:00.6 & 35 & 0.0507 & 20 & 956 $^{\pm130}$ & 1043 & st99 & 43.95 & 2.31 & 0.5 \\ A0754 & 09:08:50.08 & --09:38:11.8 & 158 & 0.0547 & 132 & 961 $^{\pm57}$ & 931 & st99 & 44.90 & 2.32 & 0.6 \\ A0957x & 10:13:57.33 & --00:54:54.4 & 128 & 0.0451 & 65 & 704 $^{\pm52}$ & 659 & st99 & 43.89 & 1.70 & 0.7 \\ A0970 & 10:17:34.30 & --10:42:01.5 & 185 & 0.0591 & 117 & 771 $^{\pm42}$ & $\ldots$ & $\ldots$ & 44.18 & 1.85 & 0.8 \\ A1069 & 10:39:54.29 & -08:36:39.8 & 112 & 0.0653 & 40 & 690 $^{\pm68}$ & 1120 & st99 & 43.98 & 1.65 & 0.9 \\ A1291 & 11:32:04.46 & +56:01:26.2 & 85 & 0.0509 & 27 & 413 $^{\pm65}$ & 720 & ag07 & 43.64 & 1.0 & 1.3 \\ A1631a & 12:52:49.84 & --15:26:17.1 & 227 & 0.0461 & 126 & 717 $^{\pm38}$ & 702 & st99 & 43.86 & 1.73 & 0.9 \\ A1644 & 12:57:14.77 & --17:21:12.6 & 266 & 0.0467 & 176 & 1051 $^{\pm58}$ & 945 & st99 & 44.55 & 2.54 & 0.5 \\ A1795 & 13:49:00.52 & +26:35:06.8 & 91 & 0.0633 & 53 & 658 $^{\pm81}$ & 887 & g96 & 45.05 & 1.58 & 1.0 \\ A1831 & 13:59:10.19 & +27:59:27.9 & 66 & 0.0634 & 17 & 444 $^{\pm68}$ & 316 & st94 & 44.28 & 1.07 & 1.5 \\ A1983 & 14:52:44.00 & +16:44:45.8 & 94 & 0.0447 & 45 & 522 $^{\pm36}$ & 498 & st94 & 43.67 & 1.26 & 0.9 \\ A1991 & 14:54:30.22 & +18:37:51.2 & 50 & 0.0584 & 35 & 625 $^{\pm73}$ & 721 & st99 & 44.13 & 1.50 & 0.9 \\ A2107 & 15:39:47.91 & +21:46:20.6 & 41 & 0.0410 & 36 & 626 $^{\pm83}$ & 625 & g96 & 44.04 & 1.52 & 0.6 \\ A2124 & 15:44:59.33 & +36:03:39.9 & 46 & 0.0666 & 30 & 596 $^{\pm58}$ & 826 & ag07 & 44.13 & 1.43 & 1.0 \\ A2169 & 16:14:06.63 & +49:07:30.6 & 63 & 0.0578 & 37 & 524 $^{\pm60}$ & 521 & ag07 & 43.65 & 1.26 & 1.1 \\ A2382 & 21:52:01.87 & --15:38:53.1 & 247 & 0.0641 & 152 & 835 $^{\pm58}$ & $\ldots$ & $\ldots$ & 43.96 & 2.00 & 0.8 \\ A2399 & 21:57:32.55 & --07:47:40.4 & 242 & 0.0578 & 125 & 716 $^{\pm46}$ & 530 & st99 & 44.00 & 1.72 & 0.9 \\ A2415 & 22:05:25.01 & --05:35:23.1 & 199 & 0.0575 & 98 & 698 $^{\pm52}$ & $\ldots$ & $\ldots$ & 44.23 & 1.68 & 1.1 \\ A2457 & 22:35:45.20 & +01:28:33.3 & 81 & 0.0584 & 56 & 648 $^{\pm51}$ & 316 & st99 & 44.16 & 1.56 & 1.0 \\ A2572a & 23:18:23.58 & +18:44:24.7 & 26 & 0.0390 & 21 & 546 $^{\pm103}$ & 676 & st99 & 44.01 & 1.33 & 0.8 \\ A2589 & 23:24:00.52 & +16:49:29.0 & 47 & 0.0419 & 35 & 830 $^{\pm98}$ & 819 & st99 & 44.27 & 2.01 & 0.4 \\ A2593 & 23:24:31.01 & +14:38:29.3 & 86 & 0.0417 & 53 & 627 $^{\pm67}$ & 763 & st99 & 44.06 & 1.52 & 0.7 \\ A2622 & 23:34:53.81 & +27:25:35.5 & 71 & 0.0610 & 38 & 732 $^{\pm68}$ & 942 & st99 & 44.03 & 1.76 & 0.6 \\ A2626 & 23:36:31.00 & +21:09:36.3 & 70 & 0.0548 & 36 & 679 $^{\pm60}$ & 696 & st99 & 44.29 & 1.64 & 0.7 \\ A3128 & 03:30:34.63 & --52:33:12.2 & 297 & 0.0600 & 207 & 900 $^{\pm38}$ & 802 & st99 & 44.33 & 2.16 & 0.8 \\ A3158 & 03:42:39.64 & --53:37:50.1 & 278 & 0.0593 & 177 & 1090 $^{\pm53}$ & 976 & st99 & 44.73 & 2.62 & 0.6 \\ A3266 & 04:31:11.92 & --61:24:22.7 & 264 & 0.0593 & 225 & 1389 $^{\pm66}$ & 1085 & st99 & 44.79 & 3.34 & 0.4 \\ A3376 & 06:00:43.57 & --40:02:59.5 & 144 & 0.0461 & 92 & 814 $^{\pm56}$ & 641 & st99 & 44.39 & 1.97 & 0.6 \\ A3395 & 06:27:31.09 & --54:23:57.8 & 191 & 0.0500 & 125 & 755 $^{\pm49}$ & 1090 & st99 & 44.45 & 1.82 & 0.7 \\ A3490 & 11:45:18.58 & --34:26:40.0 & 218 & 0.0688 & 83 & 660 $^{\pm47}$ & $\ldots$ & $\ldots$ & 44.24 & 1.58 & 1.1 \\ A3497 & 12:00:03.53 & --31:23:42.4 & 165 & 0.0680 & 82 & 724 $^{\pm48}$ & $\ldots$ & $\ldots$ & 44.16 & 1.73 & 1.3 \\ A3556 & 13:24:06.23 & --31:39:37.8 & 175 & 0.0479 & 114 & 584 $^{\pm45}$ & 643 & st99 & 43.97 & 1.41 & 0.8 \\ A3560 & 13:31:50.50 & --33:13:25.4 & 191 & 0.0489 & 118 & 717 $^{\pm43}$ & 1123 & st99 & 44.12 & 1.73 & 0.9 \\ A3809 & 21:46:51.76 & --43:52:54.7 & 195 & 0.0627 & 104 & 561 $^{\pm40}$ & 499 & st99 & 44.35 & 1.35 & 1.1 \\ IIZW108 & 21:13:56.00 & +02:33:56.0 & 32 & 0.0483 & 27 & 549 $^{\pm42}$ & $\ldots$ & $\ldots$ & 44.34 & 1.33 & 0.6 \\ MKW3s & 15:21:50.00 & +07:42:32.0 & 66 & 0.0444 & 32 & 539 $^{\pm37}$ & 612 & g96 & 44.43 & 1.31 & 0.7 \\ RX0058 & 00:58:22.30 & +26:52:03.7 & 31 & 0.0484 & 22 & 696 $^{\pm119}$ & $\ldots$ & $\ldots$ & 43.64 & 1.68 & 0.7 \\ RX1022 & 10:22:07.30 & +38:30:55.0 & 44 & 0.0548 & 25 & 582 $^{\pm91}$ & 591 & ag07 & 43.54 & 1.40 & 1.0 \\ RX1740 & 17:40:32.30 & +35:38:57.0 & 32 & 0.0441 & 20 & 540 $^{\pm66}$ & $\ldots$ & $\ldots$ & 43.70 & 1.31 & 0.8 \\ Z2844 & 10:02:37.09 & +32:41:16.7 & 54 & 0.0503 & 33 & 529 $^{\pm84}$ & $\ldots$ & $\ldots$ & 43.76 & 1.28 & 0.7 \\ Z8338 & 18:11:26.75 & +49:49:47.4 & 86 & 0.0494 & 53 & 686 $^{\pm71}$ & $\ldots$ & $\ldots$ & 43.90 & 1.66 & 0.7 \\ Z8852 & 23:10:31.85 & +07:34:17.7 & 71 & 0.0408 & 53 & 696 $^{\pm67}$ & $\ldots$ & $\ldots$ & 43.97 & 1.69 & 0.5 \\ \noalign{\smallskip}\hline\noalign{\smallskip} \end{tabular}} \medskip Refs: (st94) Struble \& Ftaclas (1994); (g96) Girardi et~al. (1996); (maz96) Mazure et~al. (1996); (wu98) Wu et~al. (1998); (st99) Struble \& Rood (1999); (FPS04) Smith et~al. (2004); (ag07) Aguerri et~al. (2007). Columns: (1) cluster name, (2--3) coordinates of the image field center at epoch $2000$ (right ascension (2) in hours, minutes and seconds and declination (3) in degrees, arcminutes, arcseconds ), (4) number of redshift determinations which is equal to the number of entries in the spectroscopic catalog for that cluster, (5) cluster mean redshift, (6) number of member galaxies (used to compute mean redshift and velocity dispersion as explained in the text), (7) cluster velocity dispersion computed from WINGS data, (8)~cluster velocity dispersion from literature, (9) reference for the literature velocity dispersion, (10)~logarithm of the \mbox{X-ray} luminosity in the 0.1--2.4~keV ROSAT RASS bandpass (from \cite{ebeling96}), (11) virial radius in~Mpc, (12) aperture in units of $R_{200}$. \end{table}