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Table 1

Properties of the stellar sample.

Name Sp. type Ref. [Fe/H] N obs Δt V σ σ / ϵ SB/ORB
(d) (km s-1) (km s-1)

HD 26 CH 10 –1.3 110 11999 –213.14 1.36 25 ORB:
HD 76396 CH 6 68 13217 –61.73 1.67 30 ORB+jitter?
HD 145777 CH 3 32 2215 18.43 0.83 15 SB
HD 187216 CH 8 –2.5 41 12373 –115.08 4.49 82 SB
HIP 53522 CH(-like) 6, 9, 11 –0.5 57 1816 32.49 5.54 100 ORB
HIP 53832 CH(-like) 6, 7, 11 –0.8 38 1151 –2.28 7.36 134 ORB
HE 0017+0055 CEMP-rs 1, 5, 12 –2.4 25 1581 –79.84 0.52 9.5 SB+jitter?
HE 0111-1346 CEMP-s 1, 5 –1.9 52 1542 44.71 6.45 117 ORB
HE 0457-1805 CEMP-s 1, 5 –1.5 29 1894 66.76 4.24 77 ORB
HE 0507-1653 CEMP-s 2, 5 –1.8 30 1495 348.41 4.90 89 ORB
HE 1120-2122 CEMP-s 4 40 1948 108.6 3.79 69 ORB+jitter?
HE 1429-0551 CEMP-s 1, 2 –2.5 39 1930 –44.51 0.19 3.4 SB?
HE 2144-1832 CEMP-s 1 22 2170 141.79 0.60 11 SB

Notes. Nobs is the number of radial-velocity observations (including older measurements from McClure & Woodsworth 1990), Δt is their time span, V is the average velocity and σ its standard deviation, σ/ϵ is the ratio between the standard deviation and measurement error (estimated to be 55 m s-1). In column SB/ORB, the systems with close to 1 yr variations superimposed on the long-term orbit are flagged with the label “jitter?”.

Reference. (1) Goswami (2005); (2) Masseron et al. (2010); (3) Bidelman (1956); (4) Goswami et al. (2010); (5) Kennedy et al. (2011); (6) Hartwick & Cowley (1985); (7) Zamora et al. (2009); (8) Kipper & Jorgensen (1994); (9) this work; (10) Van Eck et al. (2003); (11) Sperauskas et al. (2015); (12) Jorissen et al. (2016).

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