Table B.1.
Main Gaia data of the stars studied in the frame of the LP First stars.
Turnoff stars | Err | Err | Err(π) | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Gaia | Gaia | Gaia | Gaia | UVES | UVES | Gaia | / | |||||||
[Fe/H] | [Ba/Fe] | Ra | Dec | pmRA | pmDec | RVel | RVel | RVel | RVel | π | err(π) | π | d | |
BS16023-046 | −2.97 | <−0.61 | 210.22678 | 22.77818 | −42.36 | −40.68 | − | − | −7.5 | 0.5 | 0.972 | 0.023 | 0.02 | 1.03 |
BS16076-006 | −3.81 | <−1.20 | 192.09468 | 20.94551 | −26.33 | −13.06 | − | − | 206 | 0.5 | 0.592 | 0.037 | 0.06 | 1.69 |
BS16968-061 | −3.05 | <−1.03 | 225.27528 | 3.71246 | −46.28 | −45.91 | − | − | −80.7 | 0.5 | 1.045 | 0.041 | 0.04 | 0.96 |
BS17570-063 | −2.92 | −0.31 | 5.15105 | 23.79362 | 52.27 | −37.18 | − | − | −184.4 | 0.5 | 0.934 | 0.039 | 0.04 | 1.07 |
CS22177-009 | −3.10 | <−0.48 | 61.91948 | −25.04581 | 22.24 | −61.67 | − | − | −208.4 | 0.5 | 1.219 | 0.022 | 0.02 | 0.82 |
CS22888-031 | −3.30 | <−0.08 | 347.88562 | −35.44536 | 56.62 | −27.42 | − | − | −125.1 | 0.5 | 1.103 | 0.034 | 0.03 | 0.91 |
CS22948-093 | −3.30 | 0.22 | 327.63123 | −41.13045 | −18.22 | −16.99 | − | − | 364.3 | 0.5 | 0.502 | 0.039 | 0.08 | 1.99 |
CS22953-037 | −2.89 | <−0.79 | 21.27828 | −59.26672 | 67.87 | 35.62 | − | − | −163.3 | 0.5 | 1.217 | 0.017 | 0.01 | 0.82 |
CS22965-054 | −3.04 | <−0.84 | 331.62634 | −2.54289 | 27.32 | 0.95 | − | − | −281.6 | 0.5 | 0.680 | 0.056 | 0.08 | 1.47 |
CS22966-011 | −3.07 | −0.06 | 353.77954 | −30.38193 | 32.58 | −41.92 | − | − | −13.5 | 0.5 | 1.150 | 0.059 | 0.05 | 0.87 |
CS29506-007 | −2.91 | 0.18 | 320.11935 | −20.77313 | −7.88 | −20.30 | − | − | 56.4 | 0.5 | 0.869 | 0.043 | 0.05 | 1.15 |
CS29506-090 | −2.83 | −0.35 | 322.62024 | −22.17839 | −12.43 | −40.73 | − | − | −21.3 | 0.5 | 0.892 | 0.041 | 0.05 | 1.12 |
CS29518-020 | −2.77 | – | 18.05528 | −31.00153 | 42.03 | −8.65 | − | − | −22.2 | 0.5 | 0.960 | 0.025 | 0.03 | 1.04 |
CS29518-043 | −3.20 | <−0.78 | 19.65977 | −30.68414 | 36.39 | −3.31 | − | − | 144.8 | 0.5 | 0.734 | 0.030 | 0.04 | 1.36 |
CS30301-024 | −2.75 | −0.28 | 227.12340 | −0.59987 | −40.40 | −17.35 | − | − | −67.7 | 0.5 | 1.762 | 0.045 | 0.03 | 0.57 |
CS31061-032 | −2.58 | <−0.45 | 39.68045 | 3.31729 | 5.64 | −20.28 | − | − | 21 | 0.5 | 1.071 | 0.027 | 0.03 | 0.93 |
Giant stars | Err | Err | Err(π) | |||||||||||
Gaia | Gaia | Gaia | Gaia | UVES | UVES | Gaia | / | |||||||
[Fe/H] | [Ba/Fe] | Ra | Dec | pmRA | pmDec | RVel | RVel | RVel | RVel | err π | π | d | ||
HD2796 | −2.47 | −0.21 | 7.82047 | −16.79488 | −1.38 | −51.05 | −60.7 | 0.1 | −61 | 0.3 | 1.516 | 0.063 | 0.04 | 0.66 |
HD122563 | −2.82 | −0.85 | 210.63186 | 9.68579 | −189.68 | −70.32 | −26.2 | 0.2 | −26.2 | 0.3 | 3.474 | 0.063 | 0.02 | 0.29 |
HD186478 | −2.59 | −0.08 | 296.30882 | −17.49122 | −22.22 | −85.05 | 32 | 1.7 | 31.6 | 0.3 | 1.044 | 0.041 | 0.04 | 0.96 |
BD+17d3248 | −2.07 | 0.33 | 262.06007 | 17.50986 | −47.75 | −22.41 | −146 | 0.2 | −146.5 | 0.3 | 1.251 | 0.036 | 0.03 | 0.80 |
BD-18d5550 | −3.06 | −0.61 | 299.70729 | −18.20349 | 11.47 | −91.15 | −125.1 | 0.3 | −124.9 | 0.3 | 2.008 | 0.041 | 0.02 | 0.50 |
CD-38d245 | −4.19 | −0.53 | 11.65090 | −37.65935 | 15.23 | −7.53 | 48.3 | 2.5 | 46.5 | 0.3 | 0.245 | 0.034 | 0.14 | 4.08 |
BS16467-062 | −3.77 | <−0.71 | 205.50255 | 17.81136 | −18.16 | 4.02 | − | − | −90.6 | 0.3 | 0.230 | 0.028 | 0.12 | 4.34 |
CS22169-035 | −3.04 | −1.13 | 63.05787 | −12.08476 | 7.99 | −4.90 | 15.9 | 0.9 | 14.4 | 0.3 | 0.223 | 0.039 | 0.17 | 4.49 |
CS22186-025 | −3.00 | −0.06 | 66.13667 | −37.15071 | 2.70 | −3.49 | − | − | −122.3 | 0.3 | 0.126 | 0.015 | 0.12 | 7.93 |
CS22189-009 | −3.49 | −1.13 | 40.42657 | −13.46963 | 3.35 | −4.59 | − | − | −20.2 | 0.3 | 0.165 | 0.031 | 0.19 | 6.08 |
CS22873-166 | −2.97 | −0.57 | 304.84168 | −61.50425 | −15.42 | −12.52 | − | − | −16.9 | 0.3 | 0.199 | 0.034 | 0.17 | 5.03 |
CS22878-101 | −3.25 | −0.32 | 251.38102 | 8.24597 | −7.06 | 1.23 | − | − | −129.2 | 0.3 | 0.126 | 0.025 | 0.20 | 7.91 |
CS22885-096 | −3.78 | −0.94 | 305.21320 | −39.89176 | −4.43 | −6.91 | − | − | −250.1 | 0.3 | 0.201 | 0.025 | 0.12 | 4.98 |
CS22896-154 | −2.69 | 0.34 | 295.61198 | −56.97624 | −9.75 | −24.97 | − | − | 138 | 0.3 | 0.337 | 0.018 | 0.05 | 2.96 |
CS22897-008 | −3.41 | −0.96 | 315.79938 | −65.08582 | −1.68 | −6.28 | − | − | 266.6 | 0.3 | 0.186 | 0.020 | 0.11 | 5.39 |
CS22948-066 | −3.14 | −0.83 | 326.21319 | −37.46531 | −0.17 | −6.51 | − | − | −170.6 | 0.3 | 0.153 | 0.029 | 0.19 | 6.52 |
CS22953-003 | −2.84 | 0.39 | 15.56610 | −61.72947 | −3.82 | −15.77 | − | − | 208.5 | 0.3 | 0.240 | 0.014 | 0.06 | 4.16 |
CS22956-050 | −3.33 | −0.62 | 329.52429 | −65.22424 | −1.39 | −6.07 | − | − | −0.4 | 0.3 | 0.152 | 0.023 | 0.15 | 6.58 |
CS22966-057 | −2.62 | −0.33 | 357.24066 | −29.65650 | 4.35 | −36.52 | − | − | 102.2 | 0.3 | 0.536 | 0.027 | 0.05 | 1.87 |
CS22968-014 | −3.56 | <−1.37 | 46.62292 | −54.50905 | −0.50 | −5.19 | − | − | 159.1 | 0.3 | 0.144 | 0.017 | 0.12 | 6.95 |
CS29495-041 | −2.82 | −0.46 | 324.13870 | −28.31351 | −1.70 | −12.85 | − | − | 79.6 | 0.3 | 0.218 | 0.031 | 0.14 | 4.58 |
CS29502-042 | −3.19 | −1.43 | 335.45341 | 2.47910 | −6.59 | −7.28 | −139.3 | 4.9 | −138.2 | 0.3 | 0.543 | 0.097 | 0.18 | 1.84 |
CS29516-024 | −3.06 | −0.61 | 336.56399 | 2.86270 | 1.00 | −38.71 | − | − | −84.3 | 0.3 | 0.314 | 0.031 | 0.10 | 3.18 |
CS29518-051 | −2.69 | −0.13 | 21.04172 | −28.25593 | 7.14 | −15.66 | − | − | 96.4 | 0.3 | 0.517 | 0.036 | 0.07 | 1.93 |
CS30325-094 | −3.30 | <−1.68 | 223.66348 | 4.36050 | −33.26 | −18.52 | −155.1 | 1.6 | −157.7 | 0.3 | 0.457 | 0.042 | 0.09 | 2.19 |
CS31082-001 | −2.91 | 0.74 | 22.37977 | −16.01282 | 11.74 | −42.71 | 139.1 | 0.9 | 139.1 | 0.3 | 0.511 | 0.046 | 0.09 | 1.96 |
Notes. In this table, we state the [Fe/H], the metallicity of the star, [Ba/Fe] (a proxy for [Eu/Fe]), the Gaia equatorial coordinates ra and dec (epoch 2015.5), the proper motions pmra and pmdec (in mas), the line-of-sight velocity (in km s−1) measured by Gaia and measured on the UVES spectra (Gaia RVel and UVES RVel) with the corresponding errors, the Gaia DR2 parallax corrected by the zero-point offset, the error σπ and σπ/π, and finally the distances of the stars d (in kpc) deduced from the parallax. The stars were kept only when σπ/π < 0.20.
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