Table 5.
σ68(δzi) for shift parameters δzi.
Configuration | σ68(δz1) | σ68(δz2) | σ68(δz3) | σ68(δz4) | σ68(δz5) |
---|---|---|---|---|---|
×102 | ×102 | ×102 | ×102 | ×102 | |
Stage III | |||||
γγ:coh. | 3.28 | 1.98 | 2.25 | 1.71 | 1.45 |
γγ:incoh. | 3.18 | 1.94 | 2.20 | 1.71 | 1.39 |
3 × 2 pt:coh. | 3.44 | 2.13 | 2.47 | 1.88 | 1.58 |
3 × 2 pt:incoh. | 3.42 | 2.17 | 2.53 | 1.86 | 1.57 |
3ph × 2 pt:coh. | 1.59 | 1.16 | 1.10 | 1.00 | 1.14 |
3ph × 2 pt:incoh. | 1.58 | 1.28 | 1.23 | 1.14 | 1.11 |
6 × 2 pt:coh. | 0.78 | 0.60 | 0.58 | 0.63 | 0.87 |
6 × 2 pt:incoh. | 0.88 | 0.60 | 0.61 | 0.63 | 0.85 |
Stage IV | |||||
γγ: shift. | 1.21 | 1.67 | 2.34 | 3.08 | 5.14 |
3 × 2 pt:shift. | 0.91 | 0.83 | 0.89 | 1.01 | 1.67 |
3ph × 2 pt:shift. | 0.47 | 0.56 | 0.62 | 0.65 | 0.99 |
6 × 2 pt:shift. | 0.25 | 0.19 | 0.16 | 0.16 | 0.40 |
Notes. The sizes of intervals σ68(δzi) for shift parameters δzi, as constrained by each of our redshift-biased forecast configurations (left-most column), each multiplied by 102 for clarity. One sees dramatic gains in precision coming purely from including spectroscopic-photometric cross-clustering in the 6 × 2 pt.
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