Table A.1
Brown dwarfs and planets physical parameters.
| Name | Obs date | Observing mode | Tot rotation angle | Seeing | Reference |
|---|---|---|---|---|---|
| 51 Eri | 2017-09-27 | IRDIFS_EXT | 46.4° | 0.49″ | a |
| AB Pic | 2015-02-06 | IRDIFS | 28.3° | 1.10″ | b |
| β Pic | 2015-02-05 | IRDIFS | 76.6° | 0.77″ | c |
| CT Cha | 2017-03-19 | IRDIFS | 25.0° | 0.77″ | d |
| DH Tau | 2015-10-26 | IRDIFS | 20.0° | 1.27″ | |
| *2015-12-19 | IRDIFS | 24.5° | 0.63″ | ||
| 2018-12-16 | IRDIFS | 33.7° | 0.48″ | ||
| 2019-09-19 | LMIRCam | 37.0° | 0.65″ | ||
| 2020-01-05 | IRDIFS_EXT | 17.4° | 0.55″ | ||
| η Tel | 2015-05-04 | IRDIFS | 41.5° | 1.11″ | b |
| GJ 504 | *2015-06-03 | IRDIFS | 28.9° | 1.46″ | e |
| 2016-03-29 | IRDIFS | 27.5° | 0.98″ | e | |
| GQ Lup | 2015-05-04 | IRDIFS | 25.1° | 1.05″ | |
| *2016-06-26 | IRDIFS | 90.9° | 0.61″ | ||
| HD 1160 | 2015-07-01 | IRDIFS | 30.8° | 0.53″ | |
| HD 4747 | 2016-12-11 | IRDIFS_EXT | 7.1° | 2.11″ | f |
| HD 19467 | 2017-11-03 | IRDIFS_EXT | 63.3° | 0.52″ | g |
| HD 95086 | 2018-01-05 | IRDIFS_EXT | 41.0° | 0.30″ | |
| HIP 64892 | 2016-04-01 | IRDIFS | 44.7° | 0.83″ | h |
| *2017-02-08 | IRDIFS_EXT | 54.8° | 0.80″ | h | |
| HIP 65426 | 2016-06-26 | IRDIFS | 42.2° | 0.73″ | i |
| *2017-02-06 | IRDIFS | 44.3° | 0.60″ | i | |
| 2018-05-12 | IRDIFS_EXT | 31.6° | 0.81″ | j | |
| HIP 78530 | 2015-05-04 | IRDIFS | 36.3° | 0.66″ | b |
| HIP 107412 | 2016-09-16 | IRDIFS_EXT | 75.9° | 0.68″ | k |
| HR 2562 | *2017-02-06 | BROAD BAND H | 34.9° | 0.54″ | l |
| 2017-09-28 | IRDIFS_EXT | 27.6° | 0.78″ | m | |
| HR 3549 | 2015-12-19 | IRDIFS | 32.5° | 0.91″ | n |
| HR 8799 | 2015-07-04 | IRDIFS_EXT | 19.1° | 1.05” | o |
| PDS 70 | 2018-02-04 | IRDIFS_EXT | 95.7° | 0.41″ | p |
| PZ Tel | *2015-05-06 | IRDIFS | 11.4° | 1.24″ | b |
| 2015-05-31 | IRDIFS | 9.3° | 1.30″ | b | |
| TYC 7084-794-1 | 2015-11-29 | IRDIFS | 38.9° | 1.01″ | b |
| *2016-01-19 | IRDIFS_EXT | 70.6° | 1.17″ | b | |
| TYC 8047- 232-1 | *2015-09-25 | IRDIFS | 81.5° | 0.99″ | b |
| 2016-01-17 | IRDIFS | 14.3° | 1.58″ | b | |
| HIP 87836 | 2018-05-09 | IRDIFS | 50.4° | ||
Notes. The asterisks indicate the datasets used to derive the flux of the companions and the contrast curves when multiple observations were available for a single system.
References. a: Maire et al. (2019); b: Langlois et al. (in prep.); c: Lagrange et al. (2019); d: Schmidt et al. (in prep.); e: Bonnefoy et al. (2018); f: Peretti et al. (2019); g: Maire et al. (in prep.); h: Cheetham et al. (2018); i: Chauvin et al. (2017b); j: Cheetham et al. (2019); k: Delorme et al. (2017b); l: Mesa et al. (2018); m: (Maire et al. 2018); n: Mesa et al. (2016); o: Zurlo et al. (in prep.); p: Müller et al. (2018).
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