Table 2
Astrometry on HD 142527 B.
Epoch | MJD | Separation(*) (mas) | Position angle(*)(deg) | ∆RA(mas) | ∆Dec (mas) | ρ(**) – | Instrument | Reference(***) |
---|---|---|---|---|---|---|---|---|
2012-03-11 | 55 997 | 89.70 ± 2.60 | 133.10 ± 1.90 | 65.50 ± 10.79 | −61.29 ± 11.48 | 0.92 | NACO | Bl12 |
2013-03-17 | 56 368 | 82.00 ± 2.10 | 126.30 ± 1.60 | 66.09 ± 2.16 | −48.55 ± 2.22 | 0.08 | NACO | L16 |
2013-04-11 | 56 393 | 82.50 ± 1.01 | 127.98 ± 0.46 | 65.03 ± 0.89 | −50.77 ± 0.81 | −0.39 | VisAO | Ba22 |
2013-07-14 | 56 487 | 82.50 ± 1.10 | 123.80 ± 1.20 | 68.56 ± 1.32 | −45.89 ± 1.56 | 0.40 | NACO | L16 |
2014-04-08 | 56 755 | 77.73 ± 1.63 | 117.87 ± 0.96 | 68.71 ± 1.56 | −36.34 ± 1.39 | −0.18 | VisAO | Ba22 |
2014-04-25 | 56 772 | 88.25 ± 10.10 | 123.00 ± 9.20 | 74.01 ± 11.44 | −48.06 ± 13.03 | 0.30 | GPI | R14 |
2014-05-10 | 56 787 | 78.00 ± 1.80 | 119.10 ± 1.00 | 68.15 ± 1.71 | −37.93 ± 1.48 | −0.23 | SINFONI | Ch18 |
2014-05-12 | 56 789 | 77.20 ± 0.60 | 116.60 ± 0.50 | 69.03 ± 0.62 | −34.57 ± 0.66 | 0.09 | GPI | L16 |
2015-05-13 | 57 155 | – | – | 65.00 ± 2.00 | −24.00 ± 2.00 | – | SPHERE | C118 |
2015-05-15 | 57 157 | 70.16 ± 1.19 | 110.56 ± 0.80 | 65.69 ± 1.17 | −24.64 ± 1.01 | −0.12 | VisAO | Ba22 |
2015-05-16 | 57 158 | 72.19 ± 2.02 | 107.84 ± 0.97 | 68.72 ± 1.95 | −22.12 ± 1.32 | −0.29 | VisAO | Ba22 |
2015-05-18 | 57 160 | 70.00 ± 1.35 | 110.12 ± 0.72 | 65.73 ± 1.30 | −24.08 ± 0.95 | −0.28 | VisAO | Ba22 |
2015-07-03 | 57 206 | – | – | 62.90 ± 0.40 | −18.30 ± 0.50 | – | SPHERE/SAM | C118 |
2016-03-26 | 57 473 | – | – | 60.00 ± 2.00 | −7.00 ± 2.00 | – | SPHERE | Cl18 |
2016-03-31 | 57 478 | 62.80 ± 2.70 | 98.70 ± 1.80 | 62.08 ± 2.69 | −9.50 ± 2.00 | −0.10 | ZIMPOL | Cu19 |
2016-06-13 | 57 552 | – | – | 61.00 ± 2.00 | −7.00 ± 2.00 | – | SPHERE | Cl18 |
2017-05-03 | 57 876 | – | – | 49.67 ± 0.04 | 11.33 ± 0.08 | 0.50 | GRAVITY | This work |
2017-05-16 | 57 889 | – | – | 47.40 ± 0.50 | 10.30 ± 0.20 | – | SPHERE/SAM | Cl18 |
2018-02-17 | 58 166 | – | – | 38.07 ± 0.50 | 23.49 ± 0.28 | −0.79 | GRAVITY | This work |
2018-04-14 | 58 222 | – | – | 36.00 ± 1.00 | 25.00 ± 1.00 | – | SPHERE | Cl18 |
2018-04-27 | 58 235 | 43.69 ± 2.01 | 58.28 ± 1.76 | 37.16 ± 1.85 | 22.97 ± 1.55 | 0.35 | VisAO | Ba22 |
2018-07-25 | 58 324 | – | – | 29.70 ± 0.04 | 29.65 ± 0.08 | −0.43 | GRAVITY | This work |
2018-07-28 | 58 327 | – | – | 29.48 ± 0.02 | 29.51 ± 0.08 | −0.30 | GRAVITY | This work |
2019-04-28 | 58 601 | – | – | 12.59 ± 0.16 | 36.44 ± 0.10 | −0.93 | GRAVITY | This work |
2019-05-01 | 58 604 | – | – | 12.48 ± 0.15 | 36.53 ± 0.09 | −0.90 | GRAVITY | This work |
2021-01-08 | 59 222 | – | – | −27.77 ± 0.22 | 23.98 ± 0.05 | −0.49 | GRAVITY | This work |
Notes.(*) Different measurements made with different techniques and instruments are reported on two different bases: separation and position angle, or right-ascension (RA) and declination (Dec). For convenience, we have converted all values reported in separation/position angle to RA/Dec using an MCMC approach, but these values are treated on their original bases during our orbit fits.(**) When available, the correlation coefficient ρ is reported in addition to the error along the RA and Dec axes.(***) Sources: Ba22: Balmer et al. (2022) ; L16: Lacour et al. (2016); B112: Biller et al. (2012); R14: Rodigas et al. (2014); Ch18: Christiaens et al. (2018); Cl19: Claudi et al. (2019); Cu19: Cugno et al. (2019).
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