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Table A.1

Surface gravities, temperatures and chemical properties observed in the 67 CEMP-s stars of our sample.

ID log 10(g/ cm s-2) Teff/ K Porb/ days Number of [Fe/H] [C/Fe] [s/ Fe] [Eu/Fe]
observed elements

CEMP-s/nr stars

CS22880074 3.9 ± 0.13 5917 21 −1.9 1.5 1.3 0.6
CS22942019 2.2 ± 0.4 4967 2800 18 −2.7 2.2 1.8 0.8
CS22964161A 3.7 ± 0.2 6050 252.481 21 −2.4 1.6 1.4 0.7
CS22964161B 4.1 ± 0.4 5850 252.481 22 −2.4 1.4 1.3 0.7
CS30301015 0.8 ± 0.1 4750 17 −2.7 1.7 1.5 0.3
HD 196944 1.8 ± 0.1 5234 27 −2.4 1.4 1.2 0.3
HD 198269 1.3 ± 0.25 4800 1295 11 −2.2 1.7 1.7 0.9
HE02022204 1.6 ± 0.1 5280 21 −2.0 1.2 1.4 0.5
HE1135+0139 1.8 ± 0.1 5487 20 −2.4 1.1 1.1 0.4
HE21580348 2.5 ± 0.1 5215 18 −2.8 2.1 1.6 0.9

CEMP-s/r stars

BS16080175 3.7 ± 0.2 6240 6 −1.9 1.8 1.6 1.1
BS17436058 2.7 ± 0.2 5690 7 −1.8 1.6 1.7 1.2
CS22881036 4.0 ± 0.1 6200 14 −2.1 2.1 1.9 1.0
CS22898027 3.7 ± 0.28 6110 22 −2.3 2.0 2.3 2.0
CS22948027 1.8 ± 0.4 4800 426.5 21 −2.5 2.4 2.4 1.9
CS29497030 4.0 ± 0.5 6966 344 33 −2.5 2.4 2.3 1.7
CS29526110 3.2 ± 0.1 6500 18 −2.4 2.3 2.1 1.8
CS31062012 4.2 ± 0.38 6099 24 −2.8 2.3 2.1 1.6
CS31062050 2.9 ± 0.24 5489 37 −2.5 1.9 2.4 2.0
HD 187861 2.0 ± 0.35 4960 14 −2.4 2.0 1.9 1.3
HD 224959 1.9 ± 0.25 5050 1273 14 −2.1 1.8 2.2 1.7
HE01313953 3.8 ± 0.1 5928 16 −2.7 2.5 2.2 1.7
HE01430441 4.0 ± 0.35 6305 22 −2.4 2.0 2.4 1.7
HE03383945 4.1 ± 0.33 6161 32 −2.5 2.1 2.4 2.0
HE1105+0027 3.5 ± 0.1 6132 16 −2.5 2.0 2.4 1.9
HE1305+0007 1.5 ± 0.5 4655 21 −2.2 2.1 2.6 2.2
HE21481247 3.9 ± 0.1 6380 25 −2.4 2.0 2.4 2.0
HE22586358 1.6 ± 0.1 4900 31 −2.7 2.4 2.3 1.7
LP62544 2.6 ± 0.3 5500 >4383 31 −2.8 2.3 2.8 1.9
SDSSJ0912+0216 4.5 ± 0.1 6500 28 −2.6 2.3 1.6 1.3

CEMP-s/ur stars

BD+04°2466 1.8 ± 0.2 5032 4592.7 20 −2.1 1.3 1.6
CS22945017 3.8 ± 0.2 6400 6 −2.5 2.3 0.6
CS22956028 3.9 ± 0.1 6900 1290 11 −2.1 1.9 0.4
CS29509027 4.2 ± 0.1 7050 196 5 −2.1 1.5 1.3
CS30338089 2.1 ± 0.1 5000 10 −2.5 2.1 2.3
HD 13826 0.1 ± 0.35 3540 9 −2.5 1.6 1.4
HD 187216 0.4 ± 0.4 3500 14 −2.5 1.4 2.3
HD 201626 2.2 ± 0.25 5190 407 11 −2.1 2.1 2.0
HD 5223 1.0 ± 0.25 4500 18 −2.1 1.6 1.9
HE00121441 3.5 ± 0.1 5730 7 −2.7 1.9 1.3
HE00242523 4.3 ± 0.1 6625 3.14 17 −2.7 2.1 1.6
HE02061916 2.7 ± 0.1 5200 8 −2.2 2.1 2.0
HE02120557 2.1 ± 0.4 5075 15 −2.3 1.9 2.2
HE02314016 3.6 ± 0.1 5972 17 −2.1 1.3 1.5
HE03221504 0.8 ± 0.1 4460 5 −2.0 2.4 2.8
HE04304404 4.3 ± 0.1 6214 15 −2.1 1.3 1.6
HE04410652 1.4 ± 0.1 4900 11 −2.6 1.4 1.2
HE05071430 0.8 ± 0.1 4560 446 5 −2.4 2.7 1.3
HE05344548 1.5 ± 0.3 4250 4 −1.8 1.5 0.6
HE10451434 1.8 ± 0.1 4950 5 −2.5 3.3 3.0
HE11570518 2.0 ± 0.1 4900 8 −2.4 2.2 2.2
HE14290551 1.5 ± 0.1 4700 7 −2.6 2.3 1.7
HE14301123 3.8 ± 0.1 5915 15 −2.7 1.8 1.8
HE14341442 3.1 ± 0.4 5420 15 −2.5 2.1 1.3
HE1443+0113 1.9 ± 0.1 4945 5 −2.2 2.0 1.4
HE1447+0102 1.7 ± 0.1 5100 7 −2.5 2.5 2.8
HE15231155 1.6 ± 0.1 4800 6 −2.2 1.9 1.8
HE15280409 1.8 ± 0.1 5000 6 −2.7 2.4 2.4
HE21500825 3.7 ± 0.1 5960 18 −2.0 1.4 1.7
HE22210453 0.4 ± 0.1 4400 7 −2.3 1.8 1.8
HE22274044 3.9 ± 0.1 5811 14 −2.4 1.7 1.4
HE22280706 2.6 ± 0.1 5100 8 −2.5 2.3 2.6
HE22320603 3.5 ± 0.1 5750 17 −2.1 1.6 1.6
HE22400412 4.3 ± 0.1 5852 13 −2.2 1.4 1.4
SDSS0924+40 4.0 ± 0.3 6200 12 −2.6 2.7 1.9
SDSS1707+58 4.2 ± 0.3 6700 8 −2.6 2.1 3.5
SDSS2047+00 4.5 ± 0.3 6600 12 −2.1 2.0 1.6

Notes. Barium abundance is used as indicator of s-elements. In HD 198269, HD 13826 and HD 201626 lanthanum is used because barium is not observed.

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