Table 9.
Supercluster membership as a function of the lower X-ray luminosity limit, .
Scheme | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 8 |
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0.01 | 0.02 | 0.03 | 0.04 | 0.05 | 0.06 | 0.07 | 0.1 | 0.1 |
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19.0 | 23.59 | 26.84 | 29.40 | 31.59 | 33.52 | 35.26 | 39.72 | 39.72 |
NCL | 146 | 121 | 105 | 87 | 69 | 55 | 49 | 41 | – |
Perseus-Pisces SC | 20 | −4 | – | −4 | −3, +4 | −2 | – | −1 | 10 |
A400 SC | 7 | −1 | lost | – | |||||
Local Superlcuster | 5 | lost | – | ||||||
Centaurus SC | 10 | −5, +5 | −2 +1 | – | −2, +1 | −3 | – | −1, +2 | 6 |
Coma SC | 11 | −3 | +2 | −1, +1 | − | −4 | – | −2 | 4 |
Hercules SC | 10 | −3 | −2 | lost | – | ||||
Sagittarius SC | 6 | – | – | lost | – | ||||
Lacerta SC | 6 | −1 | – | −1 | lost | – |
Notes. The table provides also the minimum linking length, , and the number of clusters in the study volume, NCL, as a function of the lower luminosity limit. For each SC we show in the second column the number of clusters linked in the first linking step and in subsequent columns the number of members lost and gained by the next linking step. If less than five members are found in steps 1 to 4 and less than four members in steps 5 to 8, the structure is no longer considered and marked as lost.
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