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Table 1.
Dark Energy Figure of Merit for all three probes when considering the Gaussian covariance or the full Gaussian+SSC covariance in fsky and psky.
| Probe | Survey area [deg2] | Gaussian | Gaussian + fsky SSC | Gaussian + psky SSC | fsky/psky − 1 [%] |
|---|---|---|---|---|---|
| WL | 5 | 0.014 | 0.009 | 0.012 | −30.87 |
| 15 000 | 43.120 | 26.329 | 26.335 | −0.02 | |
| GCph | 5 | 0.035 | 0.029 | 0.029 | −1.56 |
| 15 000 | 103.714 | 88.636 | 88.455 | 0.20 | |
| GCph+WL+XC | 5 | 0.346 | 0.150 | 0.166 | −9.58 |
| 15 000 | 1038.132 | 454.590 | 460.510 | 1.30 | |
Notes. We show the results for the lowest and largest survey area.
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