Table 8.
Increasing and decreasing multiplicative changes required in the matter bispectrum, across all configurations and all ℓ-modes, to significantly affect the biases from each relevant correction term.
| Correction | Min. change | Bispec. mult. | Bispec. mult. |
|---|---|---|---|
| param | increase | decrease | |
| RS | Ωm | −2.16 | −4.16 |
| SLC | Ωm | 1.20 | 0.80 |
| MB | wa | 0.58 | 1.41 |
| SO-SLC | Ωm | 100.63 | −99.67 |
| SO-MB | wa | 47.00 | −47.00 |
Notes. A significant change is when any one of the biases on the cosmological parameters changes by ±0.25σ. These values encapsulate the fractional change for a fixed cosmology, in this case the w0waCDM cosmology of Table 3, with ΩK = 0. It should be noted that these values are not exhaustive thresholds, as sufficiently significant changes to the model at a particular sub-range of scales may also be problematic.
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