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Home All issues Volume 495 / No 3 (March I 2009) A&A, 495 3 (2009) 707-719 Full HTML
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Table 1:

The WINGS-SPE cluster sample: global properties.
Cluster RA Dec $N_{\rm gal}$ z Nz $\sigma_W$ $\sigma_L$ Refs. $\log(L_X)$ R200 Ap
  (J2000) (J2000)       km s-1 km s-1   $10^{44}~{\rm erg~s}^{-1}$ Mpc R200

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
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 X-ray luminosity in the 0.1-2.4 keV ROSAT RASS bandpass (from Ebeling et al. 1996), (11) virial radius in Mpc, (12) aperture in units of R200.

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