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Table 1.

Triangulum stream member stars.

No. αJ2000 δJ2000 μδ σμδ Vr σVr [Fe/H] σ[Fe/H] G GBP GRP Survey
(°) (°) (mas yr−1) (mas yr−1) (mas yr−1) (mas yr−1) (km s−1) (km s−1) (dex) (dex) (mag) (mag) (mag)
1 23.8285 22.8031 1.0098 0.0986 −0.1037 0.0784 −16.84 3.11 −1.913 0.068 16.759 17.222 16.106 SEGUE
2× 24.1829 22.9364 1.0127 0.1831 −0.9748 0.1339 2.78 7.84 −2.545 0.048 17.617 18.049 16.997 SEGUE
3 24.2157 22.9598 0.8790 0.3456 0.2562 0.2288 −17.60 8.73 −1.867 0.104 18.530 19.005 17.998 SEGUE
4 (BHB) 23.2433 23.1934 0.6858 0.1844 −0.2179 0.1546 −32.59 6.76 −2.121 0.078 17.967 18.031 17.815 SEGUE
5 24.1515 23.3639 1.2849 0.1128 0.2147 0.0938 −23.76 4.55 −2.348 0.114 17.335 17.803 16.718 SEGUE
6 23.9200 23.3903 0.5511 0.2549 0.4586 0.1641 −26.84 7.61 −2.128 0.114 18.251 18.672 17.667 SEGUE
7 23.8055 23.4783 1.1128 0.2314 0.0493 0.1889 −16.15 8.19 −2.371 0.056 18.457 18.891 17.927 SEGUE
8 (BHB) 24.5968 23.6575 1.1237 0.1755 0.1393 0.1465 −28.03 4.77 −2.278 0.152 17.834 17.903 17.692 SEGUE
9 23.7817 23.8800 1.0403 0.2248 0.2268 0.1843 −36.43 5.51 −2.383 0.095 18.256 18.669 17.716 SEGUE
10 23.9193 24.1185 0.8721 0.2242 −0.1813 0.1614 −31.52 5.94 −1.953 0.128 18.220 18.705 17.689 SEGUE
11 24.0593 24.1634 1.0918 0.0460 0.1548 0.0351 −27.93 8.18 −2.249 0.061 15.279 15.832 14.573 LAMOST
12 23.4145 24.3451 1.5329 0.3380 0.0838 0.1762 −22.60 9.99 −2.072 0.072 18.648 18.981 18.075 SEGUE
13 23.5792 24.3911 1.1712 0.2725 0.3187 0.1921 −13.69 9.70 −2.653 0.147 18.648 19.030 18.073 SEGUE
14 23.5445 24.5692 1.0955 0.0584 0.1400 0.0363 −32.73 9.18 −1.962 0.135 16.025 16.537 15.347 LAMOST
15 23.8850 24.7038 0.9478 0.1592 0.0680 0.1383 −24.41 6.23 −1.830 0.140 17.839 18.239 17.246 SEGUE
16 22.3385 28.4684 0.9975 0.0801 0.3481 0.0569 −41.53 12.97 −2.311 0.111 16.581 17.045 15.961 LAMOST
17 22.4622 30.0863 0.9254 0.1081 0.0873 0.0825 −34.82 9.93 −1.716 0.272 17.156 17.596 16.563 LAMOST
18 22.3181 31.2075 0.9126 0.0968 0.0614 0.0716 −57.01 16.48 −2.143 0.241 17.152 17.616 16.521 LAMOST
19 21.4457 34.2315 0.8154 0.0552 0.2357 0.0419 −68.02 13.15 −2.439 0.161 15.964 16.453 15.313 LAMOST
20 20.8085 34.9178 0.7522 0.0638 0.4043 0.0443 −75.26 12.41 −2.056 0.136 16.213 16.680 15.569 LAMOST
21 21.2461 35.1423 0.9246 0.1032 0.4356 0.0884 −74.81 12.45 −2.322 0.204 17.493 17.885 16.919 LAMOST
22 21.3470 35.2527 0.8679 0.0563 0.2653 0.0435 −74.42 11.61 −2.141 0.211 16.273 16.759 15.613 LAMOST
23 20.6703 37.3033 0.5967 0.2600 0.3732 0.2044 −76.24 12.45 −2.145 0.038 19.007 19.514 18.485 SEGUE
24 (BHB) 20.4665 37.9600 0.7622 0.1674 0.3160 0.1455 −90.22 5.21 −1.740 0.055 18.101 18.157 18.010 SEGUE
25 20.6305 38.4133 0.9838 0.1966 0.2130 0.1741 −87.51 7.20 −2.042 0.089 18.524 18.966 17.931 SEGUE
26 (BHB) 20.7368 38.4931 1.0037 0.1538 0.2964 0.1236 −105.28 7.22 −1.378 0.040 17.908 18.044 17.637 SEGUE
27 20.1517 38.6458 0.8931 0.1369 0.2047 0.0976 −101.34 5.60 −2.036 0.041 17.676 18.130 17.124 SEGUE

Notes. Identified member stars of Triangulum stream, sorted by δ. Common stars of Martin et al. (2013) are marked with “⋆.” An outlier identified in μδ panel of Fig. 3 is further labeled in “×.” Columns 12–14 are Gaia magnitudes that have been extinction-corrected (see text). The last column indicates which survey the radial velocity and metallicity come from.

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