Table 2
Fitted values for D and 6.
| D [10-3] | δ [°] | |
|---|---|---|
| Values from fit: | ||
| M3 | –6.14 ±4.7 | 170.0 ± 0.9 |
| M4-M8 | 2.58 ± 2.7 | 144.4 ± 0.3 |
| M10-M18 | 87.35 ± 1.9 | 142.3 ± 1.2 |
| Values from model: | ||
| M3 | –7.7 | 176.4 |
| M4-M8 | 24.7 | 147.5 |
| M9 (dichroic) | 57.47 | 165.0 |
| M10-M18 | 43.0 | 123.9 |
Notes. The given uncertainty is derived by bootstrapping the full dataset, fitting the data of the four telescopes individually, and calculating the standard deviation over the four values. For the final uncertainty, the larger value of the two methods is chosen. The values for M9 are not fitted and, therefore, have no uncertainty. For comparison, the lower part of the table shows the values expected from the model without a fit.
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