Table 3.
Complementarity of the final CFC detection algorithm with respect to the AMICO results.
| Finder | z = [0, 1], M > 1014 M⊙ | z = [1, 2], M > 1014 M⊙ |
|---|---|---|
| – | (common fraction, fraction of extra detections) | |
| AMASCFI | (71.2, 2.7)% | (60.7, 4.6)% |
| HCFA | (59.0, 2.2)% | (53.6, 4.5)% |
| PZWav | (89.3, 3.2)% | (81.6, 5.8)% |
| sFoF | (60.3, 2.0)% | (59.5, 3.4)% |
| WaZP | (90.1, 4.2)% | (78.9, 5.5)% |
Notes. Two redshift ranges are considered, [0, 1], and [1, 2], both for masses larger than 1014 M⊙. The two numbers correspond to the common fraction of clusters, with respect to AMICO, and the fraction of extra detections, with respect to the total. For example, adding PZWAV to AMICO, in the second redshift bin, would add 5.8% extra clusters, while they have already 81.6% clusters in common.
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