Table A.3
Second part of the general information for the SINFONI Library.
| Name | Spectral type | mK (mag) | MK (mag) | Flux (Wm−2 μm−1) | References |
|---|---|---|---|---|---|
| 2M 0103 AB b | L0 ± 0.5 | 13.690 ± 0.022 | 10.32 ± 0.07 | 1.4361 × 10−15 | 1,2,3,4,11,24 |
| AB Pic b | L0.5 ± 0.5 | 14.090 ± 0.08 | 10.59 ± 0.08 | 9.8374 × 10−16 | 1,4,5,6,7,8,9,10,11 |
| CAHA Tau 1 | M6 ± 5 | 15.110 ± 0.09 | 9.38 ± 0.11 | 3.9881 × 10−16 | 1,11,12,13 |
| CD-35 2722 b | L4.5 ± 5 | 12.01 ± 0.16 | 10.26 ± 0.30 | 6.5393 × 10−15 | 1,4,11,14,25 |
| DH Tau b | M9.25 ± 0.25 | 14.19 ± 0.02 | 8.56 ± 0.04 | 9.0759 × 10−16 | 1,7,9,11,15 |
| FU Tau b | L0.25 ± 0.25 | 13.329 ± 0.098 | 7.70 ± 0.11 | 2.0223 × 10−15 | 1,11,12,15 |
| HIP 78530 b | M7 ± 1 | 13.491 ± 0.003 | 7.84 ± 0.02 | 1.7653 × 10−15 | 1,11,17,19 |
| HR 7329 b | M7 ± 1 | 11.6 ± 0.1 | 8.17 ± 0.17 | 1.0106 × 10−14 | 1,7,11,20 |
| KPNO Tau 1 | M8.5 ± 0.5 | 13.772 ± 0.035 | 8.22 ± 0.05 | 1.3410 × 10−15 | 1,11,21 |
| KPNO Tau 4 | M9.5 ± 0.5 | 13.28 ± 0.03 | 7.65 ± 0.05 | 2.0882 × 10−15 | 1,7,11,12,21 |
| KPNO Tau 6 | M8.5 ± 0.5 | 13.689 ± 0.037 | 8.25 ± 0.06 | 1.4592 × 10−15 | 1,11,21,22 |
| USco 1606-2219 | L2 ± 1 | 14.550 ± 0.086 | 9.59 ± 0.45 | 6.5125 × 10−16 | 1,11,23 |
| USco 1606-2230 | M8 ± 0.5 | 13.806 ± 0.042 | 7.87 ± 0.26 | 1.3052 × 10−15 | 1,11,23 |
| USco 1606-2335 | M9 ± 0.5 | 15.052 ± 0.161 | 9.25 ± 0.40 | 4.1317 × 10−16 | 1,11,23 |
| USco 1607-2239 | L0 ± 0.5 | 15.436 ± 0.019 | 9.63 ± 0.26 | 2.8820 × 10−16 | 1,11,23 |
| USco 1608-2232 | M9 ± 0.5 | 14.775 ± 0.113 | 8.97 ± 0.35 | 5.3114 × 10−16 | 1,11,23 |
| USco 1608-2335 | M8.5 ± 0.5 | 13.814 ± 0.054 | 8.73 ± 0.39 | 1.3102 × 10−15 | 1,11,23 |
| USco 1610-2239 | M8.5 ± 0.5 | 14.025 ± 0.058 | 8.56 ± 0.34 | 1.0767 × 10−15 | 1,11,23 |
| USco 1612-2156 | L0 ± 1 | 15.395 ± 0.166 | 9.59 ± 0.40 | 3.0080 × 10−16 | 1,11,23 |
| USco 1613-2124 | L0 ± 1 | 15.652 ± 0.022 | 9.85 ± 0.26 | 2.3869 × 10−16 | 1,11,23 |
| USco CTIO 108 A | M7 ± 0.5 | 12.51 ± 0.03 | 6.69 ± 0.27 | 4.4330 × 10−15 | 1,7,11 |
Notes: Here we list the previously reported spectral types of our objects, along with their K-band apparent and absolute magnitudes, and the flux scaling factor. The corresponding references are found in the right-hand column.
References: (1) Wenger et al. (2000); (2) Liu et al. (2013); (3) Kraus et al. (2014); (4) Stone et al. (2016); (5) Chauvin et al. (2005); (6) Bonnefoy et al. (2010); (7) Bonnefoy et al. (2014); (8) Patience et al. (2012); (9) Martinez & Kraus (2022); (10) Booth et al. (2021); (11) Gaia Collaboration (2021); (12) Quanz et al. (2010); (13) Luhman & Mamajek (2010); (14) Wahhaj et al. (2011); (15) Wu et al. (2020); (16) Cheetham et al. (2015); (17) Lachapelle et al. (2015); (18) Ireland et al. (2011); (19) Petrus et al. (2020); (20) Lowrance et al. (2000); (21) Briceno et al. (2002); (22) Akeson et al. (2019); (23) Lodieu et al. (2011); (24) Delorme et al. (2013); (25) Gagné et al. (2018).
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