Table 3
Overall uncertainty depending on the configuration of the observation for the stars in CU6GB-cal.
| FoV-row | Md(Δ ) |
mean(Δ ) |
σ(Δ ) |
|---|---|---|---|
| km s−1 | km s−1 | km s−1 | |
| All | −0.01 | −0.04 | 0.42 |
| FoV1-All | 0.15 | 0.15 | 0.37 |
| FoV1-row4 | 0.18 | 0.20 | 0.37 |
| FoV1-row5 | 0.10 | 0.13 | 0.39 |
| FoV1-row6 | 0.13 | 0.12 | 0.36 |
| FoV1-row7 | 0.17 | 0.14 | 0.35 |
| FoV2-All | −0.19 | −0.23 | 0.40 |
| FoV2-row4 | −0.08 | −0.15 | 0.43 |
| FoV2-row5 | −0.15 | −0.22 | 0.45 |
| FoV2-row6 | −0.20 | −0.17 | 0.33 |
| FoV2-row7 | −0.31 | −0.41 | 0.36 |
Notes. The units are km s−1. Median, mean, and standard deviation of the residuals
Δ 
= 
−
(km s −1) over the time covered by the DR2. FoV-row are the possible configurations of a star transit (FoV1 and FoV2 are the FoVs of the two telescopes, and rows 1–4 are the CCD rows, see Fig. 1).
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