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Table A.2

General information about the SINFONI Library sample.

Name RA, Dec Association Parallax (mas) Distance (pc) Age (Myr) AvGaia(mag)$A_{\rm{v}}^{Gaia}\left( {{\rm{mag}}} \right)$
2M 0103 AB b 01 03 35.66 -55 15 56.24 Tucana-Ho. 21.18±1.37 47.21 ±3.00 30 ± 1 <0.004
AB Pic b 06 19 12.91 -58 03 15.52 Carina 19.95±0.01 50.14±0.03 13.3 ± 1.1 <0.004
CAHA Tau 1 04 36 09.00 +24 08 21.20 Taurus 140±50 3 ± 2 0.23±0.28
CD-35 2722 b 06 09 19.21 -35 49 31.06 AB Doradus 44.72±0.01 22.36±0.01 133 ± 20 <0.003
DH Tau b 04 29 41.66 +26 32 56.50 Taurus 7.49±0.03 133.45±0.53 3 ± 2 0.18±0.01
FU Tau b 04 23 35.75 +25 02 59.64 Taurus 7.48±1.12 133.78±17.4 3 ± 2 0.18±0.15
HIP 78530 b 16 01 55.65 -21 58 53.01 Upper Sco. 7.42±0.03 134.70±0.54 10 ± 1 0.23±0.01
HR 7329 b 19 22 51.36 -54 25 31.56 β Pictoris 20.60±0.10 48.54±0.23 20 ± 4 <0.006
KPNO Tau 1 04 15 14.72 +28 00 09.38 Taurus 7.77±0.61 128.72±9.37 5 ± 4 0.13±0.07
KPNO Tau 4 04 27 27.99 +26 12 05.08 Taurus 7.49±1.02 133.43±16.0 5 ± 4 0.18±0.14
KPNO Tau 6 04 30 07.24 +26 08 20.71 Taurus 8.15±0.38 122.72±5.47 5 ± 4 0.09±0.05
USco 1606-2219 16 06 03.76 -22 19 29.95 Upper Sco. 10.16 ± 2.41 98.39±19.0 8 ± 1 0.06±0.09
USco 1606-2230 16 06 48.18 -22 30 40.02 Upper Sco. 6.49±0.49 154.17±11.0 11 ± 1 0.30±0.03
USco 1606-2335 16 06 06.29 -23 35 13.36 Upper Sco. 145±50 11 ± 1 0.27±0.12
USco 1607-2239 16 07 27.82 -22 39 04.06 Upper Sco. 145±50 11 ± 1 0.28±0.12
USco 1608-2232 16 08 18.43 -22 32 24.82 Upper Sco. 145±50 11 ± 1 0.28±0.12
USco 1608-2335 16 08 30.49 -23 35 10.98 Upper Sco. 7.14±0.42 104.04±7.78 11 ± 1 0.26±0.03
USco 1610-2239 16 10 47.13 -22 39 49.32 Upper Sco. 8.08±0.59 123.81 ±8.42 11 ± 1 0.19±0.05
USco 1612-2156 16 12 27.64 -21 56 40.71 Upper Sco. 145±50 11 ± 1 0.30±0.13
USco 1613-2124 16 13 02.32 -21 24 28.37 Upper Sco. 145±50 11 ± 1 0.31±0.14
USco CTIO 108 A 16 05 54.07 -18 18 44.37 Upper Sco. 6.85±0.13 146.02±2.72 11 ± 1 0.31 ±0.01

Notes: The right ascension (RA) and declination (Dec) are provided in ICRS J2000 format, queried from SIMBAD (Wenger et al. 2000) for each target. Parallaxes, in milliarcseconds, were obtained from the Gaia DR3 data release and converted to distances in parsecs. For targets without reported parallaxes, we used the median distance of their associated group, with a conservative uncertainty of 50 parsecs. The expected interstellar extinction in the visible (Av) was measured and kindly provided by Carine Babusiaux using the 3D extinction map from Lallement et al. (2022) and is rounded to two decimal places or listed as an upper limit in this table.

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