Table A.1.
Identifiers, positions (epoch = 2000), proper motions, trigonometric parallaxes, and radial velocities for the 519 stars in our initial sample.
| 2MASS identifier | Gaia-DR2 identifier | Other identifier | α | δ | μα cos δ | μδ | ϖ | Source | Vr | Ref. | Cluster | Member | Table | ||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (h:m:s) | (° ′ ″) | (mas yr−1) | (mas yr−1) | (mas) | (km s−1) | (literature) | |||||||||
| 2MASS J04034930+2610520 | Gaia DR2 162535413750345856 | HBC358A+B+C | 04 03 49.32 | 26 10 52.0 | 0 | 0 | 1 | 0 | 0 | ||||||
| 2MASS J04034997+2620382 | Gaia DR2 162541942104406784 | XEST06-006 | 04 03 49.99 | 26 20 38.4 | 14.212 ± 0.311 | −19.389 ± 0.221 | 6.866 ± 0.208 | Gaia DR2 | 0 | 0 | 1 | 1 | 0 | ||
| 2MASS J04035084+2610531 | Gaia DR2 162535345034688768 | HBC359 | 04 03 50.83 | 26 10 53.0 | 18.855 ± 0.159 | −29.927 ± 0.123 | 7.781 ± 0.129 | Gaia DR2 | 14.2 ± 2.0 | 4 | 0 | 0 | 1 | 0 | 0 |
| 2MASS J04043936+2158186 | Gaia DR2 53092775104124288 | HBC360 | 04 04 39.36 | 21 58 18.5 | 3.399 ± 0.405 | −15.695 ± 0.226 | 8.220 ± 0.237 | Gaia DR2 | 0 | 0 | 1 | 0 | 0 | ||
| 2MASS J04043984+2158215 | Gaia DR2 53092775104123776 | HBC361 | 04 04 39.84 | 21 58 21.4 | 5.102 ± 0.394 | −15.118 ± 0.221 | 8.183 ± 0.252 | Gaia DR2 | 16.2 ± 2.0 | 4 | 0 | 0 | 1 | 0 | 0 |
| 2MASS J04044307+2618563 | IRAS 04016+2610 | 04 04 43.08 | 26 18 56.5 | 0 | 0 | 1 | 1 | 0 | |||||||
| 2MASS J04053087+2151106 | Gaia DR2 53098994216894208 | HBC362 | 04 05 30.89 | 21 51 10.8 | 4.271 ± 0.189 | −14.224 ± 0.126 | 7.969 ± 0.128 | Gaia DR2 | 14.8 ± 2.0 | 4 | 0 | 0 | 1 | 0 | 0 |
| 2MASS J04053214+2733139 | Gaia DR2 163511608280866816 | 04 05 32.16 | 27 33 13.5 | 11.426 ± 0.196 | −25.316 ± 0.135 | 7.606 ± 0.149 | Gaia DR2 | 0 | 0 | 0 | 0 | 1 | |||
| 2MASS J04064263+2902014 | Gaia DR2 164265220422661760 | 04 06 42.65 | 29 02 01.2 | 11.027 ± 0.320 | −17.797 ± 0.162 | 6.004 ± 0.168 | Gaia DR2 | 0 | 0 | 0 | 0 | 1 | |||
| 2MASS J04064443+2540182 | Gaia DR2 162259814291151616 | 04 06 44.45 | 25 40 18.0 | 14.009 ± 0.261 | −18.784 ± 0.159 | 6.536 ± 0.159 | Gaia DR2 | 0 | 0 | 0 | 1 | 0 | |||
| 2MASS J04065134+2541282 | Gaia DR2 162260226608005120 | V1195Tau | 04 06 51.37 | 25 41 28.6 | 12.368 ± 0.272 | −18.119 ± 0.133 | 6.415 ± 0.138 | Gaia DR2 | 16.01 ± 0.20 | 15 | 0 | 0 | 0 | 1 | 0 |
| 2MASS J04065364+2540368 | Gaia DR2 162259951730099968 | 04 06 53.66 | 25 40 36.6 | 14.318 ± 0.263 | −18.857 ± 0.157 | 6.666 ± 0.157 | Gaia DR2 | 0 | 0 | 0 | 0 | 1 | |||
| 2MASS J04080782+2807280 | Gaia DR2 163926914439144320 | 04 08 07.82 | 28 07 28.2 | −0.118 ± 0.252 | −10.310 ± 0.157 | 4.435 ± 0.146 | Gaia DR2 | 0 | 0 | 1 | 0 | 0 | |||
| 2MASS J04105425+2501266 | 04 10 54.25 | 25 01 26.6 | 0 | 0 | 0 | 1 | 0 | ||||||||
| 2MASS J04110081+2717163 | 04 11 00.81 | 27 17 16.3 | 0 | 0 | 0 | 1 | 0 | ||||||||
| 2MASS J04124068+2438157 | Gaia DR2 150073682105601408 | 04 12 40.71 | 24 38 15.4 | 14.258 ± 0.180 | −18.838 ± 0.151 | 6.869 ± 0.131 | Gaia DR2 | 0 | 0 | 0 | 1 | 0 | |||
| 2MASS J04131414+2819108 | Gaia DR2 163246832135164544 | LkCa1 | 04 13 14.14 | 28 19 10.9 | 8.371 ± 0.171 | −24.403 ± 0.137 | 7.791 ± 0.115 | Gaia DR2 | 9.57 ± 0.12 | 15 | 7 | 1 | 1 | 1 | 0 |
| 2MASS J04132722+2816247 | Gaia DR2 163233981593016064 | Anon1 | 04 13 27.24 | 28 16 25.0 | 7.440 ± 0.185 | −23.835 ± 0.145 | 7.367 ± 0.121 | Gaia DR2 | 21.91 ± 0.28 | 17 | 7 | 1 | 1 | 1 | 0 |
| 2MASS J04135328+2811233 | Gaia DR2 163229544890946944 | IRAS 04108+2803A | 04 13 53.28 | 28 11 23.3 | 11.323 ± 2.530 | −22.677 ± 1.889 | 6.936 ± 1.013 | Gaia DR2 | 15.32 ± 0.27 | 17 | 0 | 0 | 1 | 1 | 0 |
| 2MASS J04135471+2811328 | IRAS 04108+2803B | 04 13 54.72 | 28 11 33.0 | 0 | 0 | 1 | 1 | 0 | |||||||
Notes. The columns “Cluster” and “Member” provide the cluster membership from the analysis presented in Sect. 4.2 (zeros denote the outliers in the sample) and the final membership status (0 = probable outlier, 1 = confirmed member) of each star in the corresponding cluster (see Sect. 4.3). The last three columns indicate whether the star is included in one of the original tables from the literature used to construct our initial sample of stars (1 = included, 0 = not included). They refer to the samples of Joncour et al. (2017) and Tables 1 (members) and 6 (candidate members) of Luhman (2018), respectively. This table is available in its entirety in machine-readable form at the CDS.
References. For radial velocities: (1) Wilson (1953), (2) Hartmann et al. (1986), (3) Hartmann et al. (1987), (4) Herbig & Bell (1988), (5) Reipurth et al. (1990), (6) Duflot et al. (1995), (7) Mathieu et al. (1997), (8) Wichmann et al. (2000), (9) White & Basri (2003), (10) Muzerolle et al. (2003), (11) Gontcharov (2006), (12) Torres et al. (2006), (13) Kharchenko et al. (2007), (14) Scelsi et al. (2008), (15) Nguyen et al. (2012), (16) Kraus et al. (2017), (17) Kounkel et al. (2019) and (18) Gaia Collaboration (2018a).
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