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Table 1

Atmospheric parameters and iron, lithium, and carbon abundances for the target stars.

ID Teff log g ξ [Fe/H] A(Li) [C/Fe] S/N CEMP Bin
(K) (cgs) (km s−1) (dex) (dex) (dex) (@6708)
BD+233130 5304 2.81 1.3 −2.55 ± 0.08 1.17 ± 0.09 0.26 ± 0.10 310
BD-012582 5224 2.82 1.2 −2.28 ± 0.07 0.97 ± 0.08 0.80 ± 0.10 400
BS 16467-062 5348 2 78 1.6 −3.70 ± 0.08 1.06 ± 0.09 0.39 ± 0.11 180
BS 16477-003 5017 2.00 1.9 −3.26 ± 0.08 1.12 ± 0.09 0.51 ± 0.09 150 ?
CD-241782 5285 2.80 1.0 −2.66 ± 0.07 1.12 ± 0.08 0.24 ± 0.10 280
CD-30298 5274 2.71 0.6 −3.29 ± 0.08 1.07 ± 0.08 0.41 ± 0.08 700
CS 22183-031 5271 2.76 1.0 −3.03 ± 0.08 1.18 ± 0.08 0.45 ± 0.10 160 ?
CS 22186-023 5178 2.30 1.4 −2.64 ± 0.07 <0.65 0.33 ± 0.10 200
CS 22877-001 5061 2.25 1.2 −3.00 ± 0.09 0.99 ± 0.09 0.93 ± 0.10 240
CS 22880-086 5324 2.69 1.5 −2.91 ± 0.07 1.16 ± 0.08 0.72 ± 0.13 120
CS 22885-096 5099 2.22 2.1 −3.77 ± 0.09 0.98 ± 0.09 0.46 ± 0.10 230
CS 22896-154 5285 2.64 1.5 −2.68 ± 0.09 1.14 ± 0.08 0.43 ± 0.12 320 ?
CS 22897-008 4986 2.07 2.1 −3.33 ± 0.07 1.10 ± 0.08 0.55 ± 0.10 200
CS 22953-003 5150 2.39 1.6 −2.80 ± 0.08 1.23 ± 0.09 0.38 ± 0.11 220
CS 22957-022 5258 2.53 1.1 −2.81 ± 0.07 <0.84 0.19 ± 0.10 200
CS 29491-069 5270 2.68 1.2 −2.61 ± 0.07 1.17 ± 0.08 0.15 ± 0.10 130
CS 29495-042 5373 2.45 1.0 −1.94 ± 0.08 <0.73 1.07 ± 0.12 140 high **
CS 29502-042 5348 2.88 1.7 −2.98 ± 0.08 1.16 ± 0.09 0.37 ± 0.10 360
CS 30312-100 5186 2.79 1.1 −2.51 ± 0.08 1.10 ± 0.09 0.29 ± 0.12 140 **
CS 31082-001 5015 2.10 1.8 −2.73 ± 0.09 1.10 ± 0.07 0.25 ± 0.10 350
HD 002665 5059 2.28 1.6 −2.04 ± 0.08 1.14 ± 0.10 −0.07 ± 0.11 310
HD 004306 5080 2.31 1.0 −2.88 ± 0.08 1.10 ± 0.08 0.46 ± 0.10 450
HD 006755 5176 2.84 1.4 −1.53 ± 0.08 1.17 ± 0.10 −0.03 ± 0.09 160 *
HD 021581 5018 2.46 1.4 −1.65 ± 0.07 1.04 ± 0.08 0.11 ± 0.08 140
HD 026169 5100 2.45 1.3 −2.43 ± 0.08 1.07 ± 0.09 0.32 ± 0.10 700 *
HD 027928 5131 2.48 1.3 −2.34 ± 0.06 1.09 ± 0.09 0.12 ± 0.12 450
HD 045282 5283 3.25 1.1 −1.50 ± 0.08 1.17 ± 0.09 −0.02 ± 0.11 250
HD 087140 5167 2.72 1.4 −1.74 ± 0.08 1.15 ± 0.10 0.17 ± 0.10 160
HD 108317 5326 2.85 1.2 −2.30 ± 0.08 <0.42 0.08 ± 0.10 500
HD 111721 5020 2.69 1.2 −1.34 ± 0.07 1.07 ± 0.10 −0.05 ± 0.11 400
HD 126238 4990 2.21 1.7 −1.80 ± 0.08 1.16 ± 0.09 −0.09 ± 0.12 150
HD 128279 5244 3.15 1.0 −2.28 ± 0.07 1.03 ± 0.09 −0.04 ± 0.11 330
HD 175305 5079 2.60 1.5 −1.40 ± 0.08 1.13 ± 0.11 −0.06 ± 0.10 340
HD 200654 5303 2.94 0.8 −2.89 ± 0.08 1.06 ± 0.07 0.54 ± 0.11 550
HD 211998 5255 3.39 0.9 −1.52 ± 0.08 1.11 ± 0.09 0.12 ± 0.09 540
HD 218857 5149 2.62 1.4 −1.96 ± 0.07 1.13 ± 0.09 0.04 ± 0.10 320
HD 220127 5249 3.09 1.3 −1.54 ± 0.07 1.04 ± 0.08 −0.08 ± 0.10 170
HD 274939 5125 2.58 1.4 −1.67 ± 0.08 1.08 ± 0.10 0.08 ± 0.08 330
HE 0037-2657 5147 2.28 0.9 −3.08 ± 0.07 1.18 ± 0.09 0.36 ± 0.10 180 **
HE 0044-2459 5349 2.95 0.8 −3.21 ± 0.07 1.15 ± 0.08 0.35 ± 0.10 140
HE 0107-5240 5214 2.52 1.5 <−5.00 <0.66 4.48 ± 0.13 130 high *
HE 0132-2439 5321 2.83 1.7 −3.73 ± 0.08 1.00 ± 0.08 0.72 ± 0.10 200 *
HE 0207-1423 5186 3.11 1.3 −2.98 ± 0.08 <0.63 2.18 ± 0.15 170 high
HE 0243-5238 5295 2.74 1.1 −2.87 ± 0.07 1.09 ± 0.13 0.45 ± 0.10 130
HE 0323-4529 5237 2.53 1.0 −2.98 ± 0.09 1.08 ± 0.09 0.49 ± 0.11 230
HE 0401-0138 5078 2.11 0.9 −3.18 ± 0.08 1.05 ± 0.09 0.30 ± 0.10 270 **
HE 0547-4539 5291 2.67 1.0 −2.90 ± 0.08 1.18 ± 0.07 0.58 ± 0.10 140
HE 0557-4840 5120 2.31 1.3 −4.44 ± 0.13 <0.60 1.77 ± 0.15 70 low
HE 0926-0546 5193 2.23 1.7 −3.71 ± 0.09 <0.70 0.31 ± 0.10 190
HE 1005-1439 5201 2.59 1.5 −3.15 ± 0.09 <0.64 2.45 ± 0.14 230 high ?
HE 1150-0428 5080 2.48 1.4 −3.68 ± 0.08 <0.55 2.76 ± 0.16 140 high *
HE 1219-0312 5200 2.77 1.1 −2.84 ± 0.08 1.06 ± 0.09 0.03 ± 0.10 170
HE 1347-1025 5217 2.62 1.8 −3.74 ± 0.08 <0.55 1.06 ± 0.10 190 low
HE 1506-0113 5186 2.46 1.5 −3.38 ± 0.08 1.01 ± 0.09 1.46 ± 0.13 150 low *
HE 2228-3806 5276 2.89 1.0 −2.90 ± 0.09 1.00 ± 0.10 0.28 ± 0.10 150
HE 2314-1554 5161 2.47 1.1 −3.22 ± 0.09 1.02 ± 0.10 0.60 ± 0.10 130
HE 2327-5642 5100 2.33 1.1 −2.99 ± 0.08 1.05 ± 0.10 0.47 ± 0.10 250 **
SMSS J031300.36-670839.3 5194 2.29 1.5 <−7.00 0.87 ± 0.05 4.48 ± 0.15 350 low

Notes. The S/N around the Li line is listed. The last two columns indicate whether the target star is classified as a CEMP (‘high’ indicates it is a high-C band CEMP star and ‘low’ a low-C band CEMP star; otherwise, it is a carbon-normal star) and as a binary (a single asterisk indicates the binary had already been identified, two asterisks means it is a binary from this work, and a question mark indicates that there is one only RV measurement; otherwise, it is a single star).

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