Table 3
Relative astrometry and photometry of the star and planet b for NaCo, GPI, and SPHERE at 68% confidence level.
UT Date | Ins.-Filter | Algo.(a) | ∆α (mas) | ∆δ (mas) | Sep. (mas) | PA (°) | Contrast (mag) | True North (deg) | Plate scale (mas) | Ref. |
---|---|---|---|---|---|---|---|---|---|---|
12-01-2012 | NaCo-L′ | sADI | 294 ± 8 | −550 ± 8 | 624 ± 8 | 151.9 ± 0.8 | 9.8 ± 0.4 | −0.57 ± 0.10 | 27.11 ± 0.06 | 1 |
12-01-2012 | NaCo-L′ | sADI | – | – | – | – | 9.5 ± 0.2 | – | – | 3 |
14-03-2013 | NaCo-L′ | sADI | 305 ± 13 | −546 ± 13 | 626 ± 13 | 150.8 ± 1.3 | 9.7 ± 0.6 | −0.58 ± 0.10 | 27.10 ± 0.03 | 1 |
27-06-2013 | NaCo-L′ | sADI | 291 ± 8 | −525 ± 8 | 600 ± 11 | 151.0 ± 1.2 | 9.2 ± 0.8 | −0.65 ± 0.10 | 27.10 ± 0.04 | 1 |
10-12-2013 | GPI-K1 | LOCI | 301 ± 5 | −541 ± 5 | 619 ± 5 | 150.9 ± 0.5 | 12.1 ± 0.5 | −0.10 ± 0.13 | 14.17 ± 0.01 | 2, 3, 7 |
11-12-2013 | GPI-H | LOCI | 306 ± 11 | −537± 11 | 618 ± 11 | 150.3 ± 1.1 | 13.1 ± 0.9 | −0.10 ± 0.13 | 14.17 ± 0.01 | 2, 3, 7 |
13-05-2014 | GPI-K1 | LOCI | 307 ± 8 | −536 ± 8 | 618 ± 8 | 150.2 ± 0.7 | – | −0.10 ± 0.13 | 14.17 ± 0.01 | 3, 7 |
06-04-2015 | GPI-K1 | LOCI | 322 ± 7 | −532 ± 7 | 622 ± 7 | 148.8 ± 0.6 | – | −0.10 ± 0.13 | 14.17 ± 0.01 | 3, 7 |
08-04-2015 | GPI-K1 | LOCI | 320 ± 4 | −533 ± 4 | 622 ± 4 | 149.0 ± 0.4 | 12.2 ± 0.2 | −0.10 ± 0.13 | 14.17 ± 0.01 | 3, 4, 7 |
29-02-2016 | GPI-H | LOCI | 330 ± 5 | −525 ± 5 | 621 ± 5 | 147.8 ± 0.5 | 13.7 ± 0.2 | −0.10 ± 0.13 | 14.17 ± 0.01 | 3, 4, 7 |
06-03-2016 | GPI-H | LOCI | 336 ± 3 | −521 ± 3 | 620 ± 5 | 147.2 ± 0.5 | – | −0.10 ± 0.13 | 12.17 ± 0.01 | 3, 7 |
03-02-2015 | IRDIS-K1 | TLOCI | 322 ± 4 | −532 ± 4 | 621 ± 4 | 148.7 ± 0.3 | 12.2 ± 0.1 | −1.72 ± 0.06 | 12.25 ± 0.03 | 5 |
03-02-2015 | IRDIS-K1 | ANDR | – | – | 620 ± 4 | 148.9 ± 0.4 | 12.6 ± 0.5 | −1.72 ± 0.06 | 12.25 ± 0.03 | 6 |
05-05-2015 | IRDIS-K1 | TLOCI | 324 ± 4 | −530 ± 6 | 621 ± 5 | 148.5 ± 0.4 | 12.4 ± 0.2 | −1.71 ± 0.06 | 12.25 ± 0.06 | 5 |
05-05-2015 | IRDIS-K1 | ANDR | – | – | 619 ± 7 | 148.6 ± 0.5 | 12.0 ± 0.5 | −1.71 ± 0.06 | 12.25 ± 0.06 | 6 |
18-01-2016 | IRDIS-K1 | TLOCI | 326 ± 4 | −532 ± 4 | 625 ± 4 | 148.4 ± 0.3 | 12.3 ± 0.2 | −1.74 ± 0.07 | 12.27 ± 0.03 | 5, 7 |
18-01-2016 | IRDIS-K1 | ANDR | – | – | 623 ± 4 | 148.7 ± 0.4 | 11.6 ± 0.9 | −1.74 ± 0.07 | 12.27 ± 0.03 | 6 |
31-05-2016 | IRDIS-K1 | TLOCI | 333 ± 2 | −519 ± 2 | 618 ± 2 | 147.3 ± 0.2 | 12.2 ± 0.2 | −1.81 ± 0.05 | 12.26 ± 0.01 | 5 |
31-05-2016 | IRDIS-K1 | ANDR | – | – | 621 ± 3 | 147.4 ± 0.3 | 12.2 ± 0.3 | −1.81 ± 0.05 | 12.26 ± 0.01 | 6 |
10-05-2017 | IRDIS-K1 | TLOCI | 341 ± 2 | −517 ± 3 | 620 ± 3 | 146.6 ± 0.2 | 12.3 ± 0.2 | −1.78 ± 0.06 | 12.25 ± 0.02 | 5 |
10-05-2017 | IRDIS-K1 | ANDR | – | – | 624 ± 3 | 146.7 ± 0.3 | 12.2 ± 0.2 | −1.78 ± 0.06 | 12.25 ± 0.02 | 6 |
06-01-2018 | IRDIS-K1 | TLOCI | 351 ± 2 | −514 ± 2 | 622 ± 2 | 145.6 ± 0.2 | 12.3 ± 0.1 | −1.83 ± 0.05 | 12.26 ± 0.01 | 5 |
06-01-2018 | IRDIS-K1 | ANDR | – | – | 625 ± 4 | 145.6 ± 0.3 | 12.2 ± 0.1 | −1.83 ± 0.05 | 12.26 ± 0.01 | 6 |
24-02-2018 | IRDIS-K1 | TLOCI | 353 ± 3 | −517 ± 3 | 627 ± 3 | 145.6 ± 0.3 | 12.2 ± 0.1 | −1.75 ± 0.06 | 12.25 ± 0.01 | 5, 7 |
24-02-2018 | IRDIS-K1 | ANDR | – | – | 625 ± 4 | 145.7 ± 0.4 | 12.1 ± 0.1 | −1.75 ± 0.06 | 12.25 ± 0.01 | 6, 7 |
28-03-2018 | IRDIS-K1 | TLOCI | 357 ± 4 | −521 ± 4 | 632 ± 4 | 145.5 ± 0.3 | 12.3 ± 0.1 | −1.73 ± 0.07 | 12.26 ± 0.02 | 5, 7 |
28-03-2018 | IRDIS-K1 | ANDR | – | – | 631 ± 4 | 145.6 ± 0.4 | 12.3 ± 0.1 | −1.73 ± 0.07 | 12.26 ± 0.02 | 6, 7 |
13-04-2019 | IRDIS-K1 | TLOCI | 368 ± 3 | −508 ± 3 | 623 ± 3 | 144.1 ± 0.2 | 12.3 ± 0.2 | −1.78 ± 0.07 | 12.25 ± 0.02 | 5 |
13-04-2019 | IRDIS-K1 | ANDR | – | – | 627 ± 3 | 144.1 ± 0.3 | 12.2 ± 0.2 | −1.78 ± 0.07 | 12.25 ± 0.02 | 6 |
18-05-2019 | IRDIS-K1 | TLOCI | 368 ± 4 | −509 ± 4 | 630 ± 4 | 144.1 ± 0.3 | 12.2 ± 0.1 | −1.78 ± 0.07 | 12.26 ± 0.01 | 5, 7 |
18-05-2019 | IRDIS-K1 | ANDR | – | – | 628 ± 4 | 144.3 ± 0.4 | 12.1 ± 0.1 | −1.77 ± 0.07 | 12.26 ± 0.01 | 6 |
Notes. (a) Algo. refers to the algorithms used for the reduction: smart ADI (sADI; Rameau et al. 2013b), TLOCI (Lafrenière et al. 2007), and ANDROMEDA (ANDR; Mugnier et al. 2009).
References. (1) Astrometric and photometric results from Rameau et al. (2013a); (2, 3) Astrometric results processed by Rameau et al. (2016) and photometric results from Galicher et al. (2014); (4) Photometric results reported by De Rosa et al. (2016); (5,6) This work: astrometric and photometric results done automatically with pipeline (5) SpeCal-TLOCI or (6) ANDROMEDA. The 2018 and 2019 data have not been reported and exploited yet. The 2015, 2016, and 2017 data are reported by Chauvin et al. (2018), but they reduced the data with the IPAG-ADI pipeline; (7) These epochs are not used for the orbital fit of the HD 95086 b exoplanet (see Sect. 3.3).
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