Table A.1.
Clusters and groups
| Ident | l,b | distance | log(age) | ref. |
|---|---|---|---|---|
| deg. | pc | Myr | ||
| Open Clusters and star cluster candidates | ||||
| FSR 1521 | 280.435, -1.625 | 6535±1330 | 9.10 | (1) |
| LP 0780 | 280.730, -2.458 | 2136±163 | 6.60, 8.01 | (1),(7) |
| Gulliver 35 | 282.048, -2.389 | 2127±108 | 7.83 | (1) |
| BH 84 | 282.059, -2.413 | 2404±247 | 9.05 | (1) |
| Loden 28 | 282.213, -2.214 | 3950 | 7.3 | (2) |
| FSR 1530 | 282.339, -1.066 | 6600 | 6.8 | (4) |
| BH 92 | 282.989, 0.431 | 2254±115 | 7.46 | (1) |
| BH 90 | 283.139, -1.451 | 2294±59 | 8.04, 8.31 | (1),(7) |
| LP 1009 | 283.653, -1.369 | 4098 * |
8.98 | (7) |
| LP 1007 | 283.747, -1.120 | 3752 * |
7.93 | (7) |
| LP 0782 | 284.074, -1.978 | 2509±244 | 7.99, 8.56 | (1),(7) |
| LP 1006 | 284.151, -0.741 | 3640 * |
8.82 | (7) |
| LP 1002 | 284.223, 0.308 | 2770 * |
7.79 | (7) |
| LP 1004 | 284.254, -0.682 | 4318 * |
8.77 | (7) |
| Westerlund 2 | 284.272, -0.328 | 4208±79 | 7.21 | (2),(5) |
| LP 1003 | 284.290, -0.883 | 4003 * |
7.93 | (7) |
| LP 1008 | 284.305, -0.318 | 3134 * |
8.69 | (7) |
| LP 1005 | 284.313, -0.320 | 3967 * |
8.80 | (7) |
| Collinder 220 | 284.552, -0.352 | 2231±112 | 7.79, 8.19 | (1),(7) |
| IC 2581 | 284.588, 0.025 | 2449±153 | 6.60, 7.10 | (1),(7) |
| LP 2150 | 284.796, 0.879 | 1935±220 | 8.88 | (7) |
| LP 1020 | 284.912, -0.875 | 4397±361 | 8.76 | (7) |
| Ruprecht 89 | 284.969, -0.345 | 750 | 8.98 | (3) |
| LP 1025 | 285.140, -1.249 | 3990 * |
8.84 | (7) |
| LP 1011 | 285.190, -1.16 | 4146 * |
6.60 | (7) |
| LP 227 | 285.238, -0.839 | 4011 * |
9.22 | (7) |
| LP 1490 | 285.303, -0.287 | 2449±112 | 7.24, 8.67 | (1),(7) |
| LP 1024 | 285.313, -0.268 | 4066 * |
7.83 | (7) |
| UBC 258 | 285.507, 0.594 | 2406±56 | 7.40 | (1) |
| Loden 153 | 285.672, 0.083 | 2670 | 6.74 | (2) |
| NGC 3293 | 285.856, 0.076 | 2334±52 | 7.13 | (1) |
| IR clusters/groups | ||||
| [DBS2003]125 | 281.170, -1.646 | 2817 | 8.38 | (6) |
| [DBS2003]40 | 281.761, -2.016 | 1358 | 7.98 | (6) |
| [DBS2003]41 | 281.777, -2.016 | |||
| [DBS2003]126 | 282.031, -1.182 | |||
| [DBS2003]42 | 282.331, -1.395 | |||
| [DBS2003]44 | 283.153, -0.622 | |||
| [DBS2003]45 | 283.881, -0.913 | 3492 | 7.7 | (6) |
| [DBS2003]46 | 284.728, +0.325 | 2565 | 7.3 | (6) |
| [DBS2003]48 | 285.259, -0.046 | 6057 | 8.2 | (6) |
Notes. References: (1) Dias et al. (2021), (2) Kharchenko et al. (2005), (3) Dib et al. (2018), (4) Buckner & Froebrich (2014) (5) Cantat-Gaudin et al. (2018), (6)Kharchenko et al. (2013), (7) Liu & Pang (2019). *: distance calculated with the TOPCAT functions which gives from the parallax the best estimate of distance and the 5th and 95th percentile confidence intervals using the Exponentially Decreasing Space Density prior (adopting a length scale of 1500 parsec).
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