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Table 1

Observed galaxy counts, solid angle ratios, and cluster masses.

ID RA Dec obsn(<1.43) obsgaltot obsgalbkg Cgal n200 lgM200 Other IDs
(J2000)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)

1 125.171 31.953 29.3 25 61 9.95 14.28 ± 0.29
2 139.148 63.803 50.6 60 29 2.52 14.50 ± 0.28
3 145.511 8.959 83.8 115 73 3.78 14.67 ± 0.29 Abell 854 (1.3′)
4* 152.199 11.799 70.1 95 142 6.22 14.60 ± 0.28 MS1006+1202
6 154.152 24.801 60.2 68 29 4.00 14.55 ± 0.28 Abell 964 (0.2′)
7 156.988 10.579 57.4 68 18 1.70 14.54 ± 0.28
9 177.532 57.151 6.7 4 19 20.33 13.86 ± 0.37
10 177.950 37.258 55.1 72 62 3.85 14.55 ± 0.28
11 183.997 35.717 7.2 7 39 34.20 14.01 ± 0.33
12 184.066 35.520 16.4 13 120 28.95 14.10 ± 0.32
13 184.117 35.639 38.7 41 104 12.52 14.41 ± 0.28 Abell 1738 (0.6′)
16 201.297 57.600 63.2 81 29 1.75 14.57 ± 0.28 Abell 1744 (1.4′)
17 201.457 59.330 58.0 64 22 3.62 14.56 ± 0.28
19 211.869 27.821 49.7 53 45 4.73 14.48 ± 0.29 Abell 1861 (0.6′)
20 217.778 25.634 45.9 48 11 2.01 14.47 ± 0.28
21* 224.313 22.342 51.1 60 86 9.07 14.52 ± 0.29 MS1455.0+232
23 228.214 14.318 69.9 89 46 3.60 14.61 ± 0.29 Abell 2044 (0.3′)
24 229.075 0.089 58.0 67 21 2.31 14.55 ± 0.28 Abell 2050 (1.1′)
25 233.265 –0.771 61.5 76 32 3.48 14.59 ± 0.28
26 233.840 37.396 83.6 114 33 2.01 14.68 ± 0.29
27 245.254 25.772 43.9 48 65 7.41 14.45 ± 0.29
28 250.661 27.444 36.6 46 38 3.36 14.42 ± 0.28
29 253.061 44.823 74.3 95 41 3.10 14.63 ± 0.28
30 27.115 14.038 29.3 27 18 5.24 14.33 ± 0.30
31 328.925 12.525 52.1 59 39 5.51 14.52 ± 0.28
32 140.964 59.512 41.5 47 50 7.04 14.46 ± 0.29
33 141.833 30.232 23.5 23 172 28.64 14.26 ± 0.30
34 168.213 53.856 41.3 45 43 8.30 14.46 ± 0.28
35 179.130 54.361 19.3 15 80 38.45 14.19 ± 0.29
36 180.201 –1.188 16.4 8 10 8.05 14.03 ± 0.32
37 203.754 58.719 29.6 32 27 7.13 14.37 ± 0.28
38* 210.258 2.878 127.6 238 115 3.28 14.85 ± 0.31 Abell 1835
39 211.664 27.600 24.9 21 101 19.48 14.23 ± 0.29
40 217.705 28.153 20.8 17 39 11.73 14.20 ± 0.29
42 319.704 0.560 81.7 104 87 5.50 14.65 ± 0.29
43 354.416 0.271 89.5 139 124 5.37 14.73 ± 0.30 Abell 2631 (1.4′)

Notes. Objects with an ID with an asterisc are not part of the statistical sample, because they are X-ray selected.

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