Table 2.
vz, kSZ − vz, halo relations for telescopes with different sizes under different PWV conditions.
| Diameter | PWV | 0.25R500 | 0.50R500 | R500 | R200 | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (m) | (mm) | Slope | σrms | fdetect | Slope | σrms | fdetect | Slope | σrms | fdetect | Slope | σrms | fdetect |
| 10 | 0.5 | 0.89 ± 0.12 | 154.6 | 32% | 0.85 ± 0.16 | 119.5 | 25% | 0.92 ± 0.42 | 119.6 | 13% | – | – | 3% |
| 1.0 | 0.87 ± 0.16 | 156.9 | 25% | 0.91 ± 0.26 | 154.4 | 19% | – | – | 5% | – | – | 1% | |
| 1.5 | 0.87 ± 0.26 | 226.7 | 15% | 0.88 ± 0.46 | 125.6 | 11% | – | – | 3% | – | – | 0% | |
| 2.0 | 0.78 ± 0.43 | 169.2 | 12% | 1.24 ± 0.98 | 141.9 | 7% | – | – | 1% | – | – | 0% | |
| 30 | 0.5 | 0.93 ± 0.06 | 129.6 | 82% | 0.94 ± 0.05 | 92.1 | 78% | 0.91 ± 0.05 | 75.8 | 62% | 0.98 ± 0.08 | 62.2 | 46% |
| 1.0 | 0.92 ± 0.06 | 139.3 | 75% | 0.90 ± 0.05 | 102.9 | 67% | 0.91 ± 0.07 | 63.4 | 48% | 1.01 ± 0.12 | 96.3 | 36% | |
| 1.5 | 0.90 ± 0.07 | 142.1 | 65% | 0.85 ± 0.06 | 99.3 | 56% | 0.92 ± 0.09 | 72.6 | 45% | 1.00 ± 0.18 | 98.1 | 28% | |
| 2.0 | 0.85 ± 0.07 | 145.2 | 59% | 0.81 ± 0.07 | 106.5 | 51% | 0.94 ± 0.11 | 89.0 | 40% | 1.01 ± 0.24 | 100.2 | 21% | |
| 100 | 0.5 | 0.87 ± 0.06 | 138.1 | 98% | 1.00 ± 0.04 | 89.8 | 94% | 1.05 ± 0.03 | 62.4 | 90% | 1.01 ± 0.03 | 51.0 | 86% |
| 1.0 | 0.89 ± 0.06 | 139.8 | 90% | 0.98 ± 0.04 | 90.7 | 88% | 1.01 ± 0.03 | 59.3 | 85% | 0.97 ± 0.03 | 50.6 | 78% | |
| 1.5 | 0.88 ± 0.06 | 137.7 | 88% | 0.98 ± 0.04 | 90.0 | 86% | 0.98 ± 0.03 | 57.4 | 82% | 0.95 ± 0.03 | 53.8 | 72% | |
| 2.0 | 0.89 ± 0.06 | 137.5 | 86% | 0.96 ± 0.04 | 89.6 | 85% | 0.96 ± 0.04 | 57.9 | 75% | 0.94 ± 0.04 | 54.9 | 65% | |
Notes. For cases for which too few sources were detected for at least three frequencies, we cannot fit the relation between vz, kSZ and vz, halo. These cases are labeled with a minus. The rms scatters, σrms, are in km/s. The fdetect is the detection rate of galaxy clusters that have measurements with an S/N greater than 2 for at least three frequencies.
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