Table 2
Statistical and systematic uncertainties on the dipole calibration, for single detectors from the lower-frequency HFI channels.
| Frequency | Statistical error | Systematic | Systematic |
| [GHz] | [%] | (worst case) [%] | [%] |
|
|
|||
| 100 | 0.004 | 0.64 | 0.37 |
| 143 | 0.002 | 0.53 | 0.29 |
| 217 | 0.002 | 0.69 | 0.41 |
| 353 | 0.010 | 2.53 | 1.81 |
Notes. The “worst case” column corresponds to a situation with a poorly matched sky template, whereas the third column is for the best case. In addition to each of these values, one has to take into account the WMAP solar dipole amplitude uncertainty, 0.24%, as this measurement is our primary calibrator.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.