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N | XID |
(1) | (2) | (3) | (4) | (5) |
0.126 | 906 | 0.119-0.133 | 73 | - |
0.215 | 443 | 0.211-0.218 | 61 | - |
0.338 | 1724 | 0.322-0.353 | 76 | - |
0.530 | 2190 | 0.508-0.552 | 193 | - |
0.672 | 1758 | 0.653-0.692 | 306 | 645 |
0.735 | 565 | 0.728-0.742 | 257 | 566, 594 |
0.973 | 2936 | 0.935-1.012 | 181 | 249 |
1.039 | 859 | 1.028-1.051 | 110 | - |
1.095 | 1536 | 1.074-1.117 | 129 | - |
1.221 | 391 | 1.215-1.227 | 65 | - |
1.296 | 261 | 1.292-1.300 | 35 | - |
1.611 | 497 | 1.602-1.620 | 36 | - |
2.318 | 2102 | 2.272-2.365 | 108 | - |
2.566 | 1435 | 2.532-2.601 | 72 | - |
2.811 | 575 | 2.796-2.825 | 23 | - |
3.471 | 984 | 3.442-3.501 | 29 | - |
3.702 | 360 | 3.691-3.714 | 11 | - |
Notes. The columns list: (1) the average
of each peak; (2) the velocity dispersion
;
(3) the redshift range corresponding
to
,
selected for the analysis of the spatial distribution
(see Figs. B.1, B.2, and B.3); (4) the number of galaxies in the selected redshift
interval; and (5) the identification numbers of extended X-ray sources
(from Giacconi et al. 2002) associated with the peak.
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