Table 1.
Instrumental characteristics of LiteBIRD used in this study (adapted from Hazumi et al. 2020, see Sect. 3.2.3).
| Telescope | Frequency | Sensitivity  |
θFWHM |
|---|---|---|---|
| [GHz] | [μK arcmin] | [arcmin] | |
| LFT | 40.0 | 37.42 | 70.5 |
| LFT | 50.0 | 33.46 | 58.5 |
| LFT | 60.0 | 21.31 | 51.1 |
| LFT | 68.0 | 19.91/31.77 | 41.6/47.1 |
| LFT | 78.0 | 15.55/19.13 | 36.9/43.8 |
| LFT | 89.0 | 12.28/28.77 | 33.0/41.5 |
| LFT/MFT | 100.0 | 10.34/8.48 | 30.2/37.8 |
| LFT/MFT | 119.0 | 7.69/5.70 | 26.3/33.6 |
| LFT/MFT | 140.0 | 7.25/6.38 | 23.7/30.8 |
| MFT | 166.0 | 5.57 | 28.9 |
| MFT/HFT | 195.0 | 7.05/10.50 | 28.0/28.6 |
| HFT | 235.0 | 10.79 | 24.7 |
| HFT | 280.0 | 13.8 | 22.5 |
| HFT | 337.0 | 21.95 | 20.9 |
| HFT | 402.0 | 47.45 | 17.9 |
Notes. Some frequency bands are shared by two different telescopes or detector arrays. If so, the two values of polarization sensitivities 
and instrumental beam full width at half maximum θFWHM are displayed on the same line.
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