Table A.1
Relative astrometry of HD 206893 B from the literature.
| MJD | Sep. | PA | Inst. | Band | Source |
|---|---|---|---|---|---|
| (days) | (mas) | (deg) | |||
| 57 300 | 270.0 ± 2.6 | 69.95 ± 0.55 | SPHERE | H | M17 |
| 57 608 | 269.53 ± 12.15 | 62.76 ± 2.16 | NACO | L’ | S20 |
| 57 647 | 265 ± 2 | 62.25 ± 0.11 | SPHERE | K1/K2 | D17 |
| 57 653 | 267.6 ± 2.9 | 62.72 ± 0.62 | GPI | H | W21 |
| 57 682 | 265.0 ± 2.7 | 61.33 ± 0.64 | GPI | K1 | W21 |
| 57 948 | 260.3 ± 2.0 | 54.2 ± 0.4 | SPHERE | H | G19 |
| 58 066 | 256.9 ± 1.1 | 51.01 ± 0.35 | GPI | K2 | W21 |
| 58 277 | 246.51 ± 21.34 | 42.80 ± 2.24 | NACO | NB4.05 | S20 |
| 58 289 | 249.11 ± 1.60 | 45.50 ± 0.37 | SPHERE | H2/H3 | G19 |
| 58 385 | 251.7 ± 5.4 | 42.6 ± 1.6 | GPI | J | W21 |
| 58 415 | 239.12 ± 17.55 | 42.53 ± 2.17 | NACO | M’ | S20 |
Notes. “Sep.” and “PA” denote the angular separation and the position angle, respectively, and “Inst.” denotes the instrument with which the data were acquired. M17 = Milli et al. (2017), D17 = Delorme et al. (2017), G19 = Grandjean et al. (2019), S20 = Stolker et al. (2020), W21 = Ward-Duong et al. (2021).
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