As published in Postman & Lauer 1995, ApJ, 440, 28. Table 1 The BCG Sample ============================================================= BCG Coordinates BCG Cluster Abell R.A. (J2000) Dec cz cz Notes ------------------------------------------------------------- 76 00 39 26.32 +06 44 02.5 11162 11162 I1565 119 00 56 16.13 -01 15 22.1 13320 13354 147 01 08 37.90 +02 16 06.1 13138 13022 Note 1 160 01 12 59.76 +15 29 29.3 13095 13095 168 01 14 57.70 +00 25 52.1 13439 13446 Note 1 189 01 23 26.33 +01 42 17.8 10236 9925 193 01 25 07.54 +08 41 57.0 14825 14553 I1695 194 01 25 58.84 -01 20 21.8 5321 5357 N 545 195 01 26 54.75 +19 12 50.1 12796 12796 I 115 260 01 50 42.96 +33 04 54.8 10699 10998 261 01 51 26.48 -02 15 11.5 13965 13965 262 01 52 46.28 +36 09 05.3 4831 4913 N 705 295 02 02 17.24 -01 07 40.6 12818 12890 347 02 25 26.47 +41 49 27.1 5257 5604 N 910 376 02 46 04.04 +36 54 16.7 14700 14700 397 02 56 28.91 +15 54 58.9 10286 9975 407 03 01 51.60 +35 50 27.4 14059 14130 419 03 08 28.73 -23 36 53.2 12240 12240 Note 2 496 04 33 37.68 -13 15 39.7 9893 9893 533 05 01 08.25 -22 34 58.1 14365 14149 539 05 16 55.12 +06 33 09.5 9682 8754 548 05 49 21.74 -25 20 47.0 11848 11949 569 07 09 07.76 +48 36 55.3 5724 5749 N2329 576 07 22 06.83 +55 52 29.3 12072 11542 634 08 15 44.90 +58 19 15.8 8135 8135 671 08 28 31.92 +30 25 48.0 14970 15219 I2378 779 09 19 46.80 +33 44 58.7 6867 6796 N2832 912 10 01 09.41 -00 04 46.5 13572 13572 957 10 13 38.27 -00 55 31.3 13438 13433 999 10 23 23.85 +12 50 05.8 9749 9603 1016 10 27 07.91 +11 00 36.9 9705 9669 I 613 1060 10 36 42.56 -27 31 42.9 3704 3719 N3311 1100 10 48 45.73 +22 13 03.4 13990 13990 1139 10 58 11.02 +01 36 15.4 11460 11788 U6057, Note 3 1142 11 00 45.39 +10 33 11.6 10118 10501 I 664 1177 11 09 44.52 +21 45 31.5 9561 9561 1185 11 10 38.32 +28 46 03.0 10521 9917 N3550 1213 11 16 22.87 +29 15 08.1 13535 14045 Note 1 1228 11 21 23.19 +34 21 24.4 10674 10973 1257 11 25 31.10 +35 30 15.3 10220 10297 Note 1 1267 11 28 36.40 +26 54 19.4 9798 9830 1308 11 33 05.09 -04 00 49.8 15508 15508 1314 11 34 49.42 +49 04 38.3 9977 9838 I 712 1367 11 44 02.17 +19 56 58.7 6237 6469 N3842 1631 12 53 18.20 -15 31 58.0 14275 14030 Note 4 1644 12 57 11.76 -17 24 35.0 14237 14220 1656 13 00 08.04 +27 58 36.3 6497 6961 N4889 1736 13 27 28.04 -27 19 27.6 13605 13583 I4252 1836 14 01 41.84 -11 36 22.7 10999 11036 1983 14 52 43.25 +16 54 12.9 13756 13617 Note 1 2040 15 12 47.74 +07 26 02.0 13680 13698 2052 15 16 44.55 +07 01 16.8 10331 10575 2063 15 23 05.46 +08 36 33.2 10626 10633 2107 15 39 39.05 +21 46 55.7 12613 12496 U9958 2147 16 02 17.04 +15 58 27.6 10384 10511 2151 16 04 35.76 +17 43 18.0 11248 11115 N6041 2152 16 05 29.28 +16 26 11.0 13598 13598 2162 16 12 35.73 +29 29 03.5 9547 9629 N6086 2197 16 29 45.04 +40 48 42.5 8800 9042 N6173, Note 1 2199 16 28 38.45 +39 33 03.0 9348 9034 N6166 2247 16 52 48.08 +81 37 57.9 12016 11641 2572 23 17 13.54 +18 42 28.2 13009 12420 2589 23 23 57.55 +16 46 35.8 12144 12397 2593 23 24 20.15 +14 38 50.4 12514 12489 N7649 2634 23 38 29.44 +27 01 49.7 9141 9153 N7720 2657 23 44 30.49 +09 15 51.6 12454 12100 Note 1 2666 23 50 58.66 +27 08 47.6 8123 8057 2717 00 03 12.77 -35 56 16.7 14936 14753 2731 00 09 59.04 -57 01 17.7 9457 9457 N 25 2806 00 40 48.47 -56 12 53.4 8229 8252 N 215 2870 01 07 41.84 -46 54 31.2 6714 7233 I1625 2877 01 09 54.82 -45 55 57.3 7261 7309 I1633 2881 01 11 14.14 -17 04 14.5 13363 13324 2896 01 18 18.60 -37 06 17.0 9555 9555 2911 01 25 12.19 -38 05 38.0 5992 6056 N 544 3144 03 37 04.88 -55 01 20.8 13120 13546 3193 03 58 13.54 -52 19 44.4 10009 10350 3367 05 49 41.71 -24 32 43.7 13461 13461 3374 05 56 42.97 -21 15 12.4 14201 14307 3376 06 00 41.01 -40 02 46.6 13814 13907 3381 06 09 53.76 -33 35 34.1 11488 11467 3389 06 22 21.30 -64 56 04.6 8294 8114 3395 06 27 36.42 -54 27 01.7 14520 14712 3526 12 48 48.94 -41 18 42.0 3045 3454 N4696 3528 12 54 22.31 -29 00 45.9 16425 16317 Note 5 3530 12 55 36.10 -30 20 49.3 16162 16206 Note 5 3532 12 57 22.15 -30 21 47.5 16633 16646 Note 5 3537 13 01 00.71 -32 26 28.9 5104 5053 3542 13 08 41.52 -34 34 31.3 10389 10387 3553 13 19 15.08 -37 10 46.5 14446 14446 3554 13 19 31.53 -33 29 19.7 14333 14333 3556 13 24 06.76 -31 40 15.0 14459 14500 3558 13 27 56.53 -31 29 46.8 14110 14312 3559 13 29 51.02 -29 30 53.1 14105 14213 3560 13 31 53.33 -33 14 04.4 3644 3734 N5193 3562 13 33 34.74 -31 40 20.3 14708 14708 3564 13 34 55.37 -35 05 57.8 14496 14721 3565 13 36 39.06 -33 57 56.7 3762 3834 I4296 3566 13 39 38.22 -35 36 32.6 14529 14529 3570 13 46 24.00 -37 58 15.5 11377 11156 3571 13 47 28.42 -32 51 51.8 11679 11913 3572 13 48 14.26 -33 22 57.8 12134 12141 3574 13 49 05.29 -30 17 44.9 4523 4657 I4329 3575 13 52 38.36 -32 53 17.3 11188 11188 3581 14 07 29.51 -27 01 07.0 6618 6682 I4374 3656 20 00 49.97 -38 34 35.9 5965 5768 I4931 3676 20 24 24.50 -40 21 59.5 12108 12108 3677 20 26 23.56 -33 21 03.5 13787 13789 3698 20 35 56.21 -25 16 45.3 5799 6040 N6936 3716 20 51 56.82 -52 37 47.9 13900 13426 3733 21 01 59.07 -28 03 34.5 10943 11039 3736 21 05 04.49 -43 25 09.2 14604 14604 3742 21 07 52.28 -47 10 43.4 4764 4842 N7014 3744 21 07 16.19 -25 28 08.4 11041 11153 3747 21 08 38.93 -43 29 11.1 9174 9170 3869 22 20 31.05 -55 07 29.9 12005 12005 N7249 4038 23 47 28.30 -28 06 34.6 8218 8501 I5353 4049 23 51 36.65 -28 21 55.7 8137 8512 I5362 4059 23 57 00.37 -34 45 32.4 14696 14730 ------------------------------------------------------------- All velocities are heliocentric and are given in km/s. Note 1: The present BCG choice differs from the galaxy selected by Hoessel, Gunn, & Thuan (1980). Note 2: A0419 appears to consist of two overlapping clusters at z=0.041 and z=0.068. We have selected the lower redshift component. Note 3: The redshift for the BCG in A1139 (obtained from ZCAT) had a relatively large measurement error of 170 km/s (see Table 6). However, a remeasurement of its redshift by us in 1992 gives a heliocentric velocity of 11495 (+/-29) km/s, within 35 km/s of the less precise value. Note 4: A1631 appears to consist of two overlapping clusters at z=0.014 and z=0.046. We have selected the higher redshift component. Note 5: This cluster was included to test for inhomogeneous velocity bias at the sample edge (see Paper I).