Table 5.
Extracted astrometry and photometry for each planet (same Id than in Table 3) using the model of planet image technique (Sect. 3.2) and the negative planet technique (Sect. 3.3) on the final image provided by PCA 10 modes.
| Extraction | Id | Band | ΔRA (pixel) | E | ΔDec (pixel) | E | C × 1e6 | E |
|---|---|---|---|---|---|---|---|---|
| Model of planet image | 1 | H2 | 52.87 ± 0.21 | 0.14 | 2.51 ± 0.15 | 1.27 | 2.108 ± 0.148 | 6.03 |
| H3 | 52.92 ± 0.23 | 0.09 | 2.56 ± 0.16 | 0.88 | 1.650 ± 0.118 | 6.36 | ||
| 2 | H2 | −25.77 ± 0.19 | 0.16 | 8.35 ± 0.14 | 0.36 | 4.634 ± 0.290 | 4.71 | |
| H3 | −26.00 ± 0.33 | 0.61 | 8.34 ± 0.21 | 0.29 | 2.182 ± 0.204 | 4.01 | ||
| 3 | H2 | −72.07 ± 0.23 | 0.30 | −71.03 ± 0.23 | 0.74 | 0.787 ± 0.070 | 3.04 | |
| H3 | −71.93 ± 0.15 | 0.47 | −71.15 ± 0.15 | 0.33 | 2.365 ± 0.143 | 4.44 | ||
| Negative planet | 1 | H2 | 52.90 ± 0.10 | 0.00 | 2.58 ± 0.07 | 1.71 | 2.781 ± 0.146 | 1.50 |
| H3 | 52.84 ± 0.12 | 0.50 | 2.56 ± 0.08 | 1.75 | 2.298 ± 0.126 | 0.81 | ||
| 2 | H2 | −25.74 ± 0.10 | 0.60 | 8.47 ± 0.08 | 0.88 | 6.338 ± 0.321 | 1.05 | |
| H3 | −25.93 ± 0.18 | 0.72 | 8.56 ± 0.13 | 1.23 | 3.116 ± 0.190 | 0.61 | ||
| 3 | H2 | −72.06 ± 0.28 | 0.21 | −71.28 ± 0.19 | 0.42 | 0.915 ± 0.086 | 0.99 | |
| H3 | −71.91 ± 0.09 | 1.00 | −71.13 ± 0.09 | 0.78 | 2.919 ± 0.162 | 0.50 |
Notes. For each measurement, we compare it to the true value using the E criteria that is given in Eq. (17).
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