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Table B.3.

Main Gaia data of the stars selected in the sample of Sestito et al. (2019).

Sestito’s sample Err Err Err(π)
Gaia Gaia Gaia Gaia Spec Spec Gaia
[Fe/H] [Ba/Fe] Ra Dec pmRA pmDec RVel RVel RVel RVel π Err(π) π d
HE 0233-0343 −4.70 39.12435 −3.50172 49.96 −10.61 64.0 1.0 0.822 0.054 0.07 1.22
HE 1327−2326 −5.96 202.5245 −23.69694 −52.52 45.5 64.4 1.3 0.918 0.024 0.03 1.09
SDSS J081554.26+472947.5 <−5.80 123.97602 47.49645 −14.15 −24.23 −95.0 23.0 0.474 0.084 0.18 2.11
SDSS J102915+172927 −4.99 157.31307 17.49107 −10.86 −4.06 −35.0 4.0 0.764 0.078 0.1 1.31
SMSS J031300.36−670839.3 <−6.53 48.25164 −67.14426 7.03 1.09 298.5 0.5 0.128 0.016 0.13 7.81
BD+44 493 −4.30 36.70797 44.96279 118.36 −32.23 −147.9 0.9 −150.14 0.63 4.79 0.066 0.01 0.21
CS 22885−0096 −4.21 305.2132 −39.89176 −4.43 −6.91 −248.0 10.0 0.201 0.025 0.12 4.98
CS 22963−0004 −4.09 44.19414 −4.85485 21.71 −2.67 292.4 0.2 0.252 0.036 0.14 3.97
HE 0044−3755 −4.19 11.6509 −37.65935 15.23 −7.53 48.3 2.5 0.245 0.034 0.14 4.08
HE 0057−5959 −4.08 14.97496 −59.72497 2.39 −10.52 375.64 1.0 0.228 0.025 0.11 4.38
HE 0134−1519 −4.00 24.27252 −15.07304 24.96 −10.9 244.0 1.0 0.375 0.03 0.08 2.66
HE 1012−1540 −4.17 153.72236 −15.93132 −102.32 28.13 225.8 0.5 2.572 0.028 0.01 0.39
LAMOST J125346.09+075343.1 −4.02 193.44198 7.89501 21.04 −58.73 78.0 0.4 1.435 0.038 0.03 0.7
SDSS J014036.21+234458.1 −4.00 25.15092 23.74941 1.02 −21.47 −197.0 1.0 1.078 0.056 0.05 0.93
2MASS J18082002−5104378 −4.07 272.08343 −51.07724 −5.63 −12.64 16.54 0.12 1.708 0.04 0.02 0.59

Notes. Five of these stars are ultra iron-poor stars with [Fe/H] <  −4.5. The other stars have metallicities close to the metallicity of the LP First stars sample, but many of them are C rich. The columns are the same as in Table B.1.

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