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Table 5.
CPL model.
| BINGO | Planck | BINGO + Planck | ||
|---|---|---|---|---|
| Parameter | ±1σ ( ) |
±1σ ( ) |
±1σ ( ) |
100%×|σtotal − σref|/σref |
| Ωbh2 | 0.015 (68%) | 0.00016 (0.7%) | 0.00014 (0.6%) | 6.9% |
| Ωch2 | 0.052 (43%) | 0.0013 (1.1%) | 0.0011 (0.9%) | 19% |
| h | 0.14 (20%) | 0.088 (13%) | 0.019 (2.9%) | 78% |
| ln(1010As) | 0.92 (30%) | 0.016 (0.5%) | 0.016 (0.5%) | 0.6% |
| ns | 0.11 (11%) | 0.0044 (0.5%) | 0.0041 (0.4%) | 8.0% |
| w0 | 0.55 (55%) | 0.46 (46%) | 0.30 (30%) | 34% |
| wa | 2.8 | 1.8 | 1.3 | 31% |
| bH I | 0.081 (8.1%) | 0.023 (2.3%) | 72% | |
Notes. Expected 1σ constraints on the CPL cosmological parameters from BINGO, Planck, and BINGO + Planck. The last column shows the improvement in combining BINGO + Planck with respect to the case with Planck only, except for bH I, which is compared with BINGO only.
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