Table 7.
A posteriori photometric calibration test using the best Solar dipole estimation (see values in Sect. 4.2) for single detectors within a frequency, and frequency averages.
| Data | Single fiducial simulation |
100 simulations |
||||
|---|---|---|---|---|---|---|
| Absolute frequency bias |
||||||
| Detector rms |
SRoll gain | |||||
| Frequency | uncertainty | Average | rms | |||
| [GHz] | (A) | (B) | (C) | (D) | (E) | (F) |
| 100......... | 5 × 10−6 | 1.1 × 10−5 | 5.8 × 10−6 | −5.9 × 10−5 | 8.0 × 10−5 | 1.5 × 10−4 |
| 143......... | 8 × 10−6 | 3.7 × 10−6 | 2.7 × 10−6 | 3.1 × 10−4 | 2.1 × 10−4 | 1.1 × 10−4 |
| 217......... | 2 × 10−5 | 1.3 × 10−5 | 3.1 × 10−6 | 2.3 × 10−4 | 2.8 × 10−4 | 1.4 × 10−4 |
| 353......... | 2 × 10−4 | 1.0 × 10−4 | 2.8 × 10−5 | 6.0 × 10−4 | 2.4 × 10−4 | 3.9 × 10−4 |
Notes. Column A refers to data, Cols. B–D refer to the single fiducial simulation, and Cols. E and F refer to 100 E2E simulations where the best Solar dipole was used as input.
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