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Table 4

Results for the stellar parameters, for the DMA (upper portion) and SAT (lower portion) subsamples.

Tex (K) log g [FeI/H] [FeII/H] ξ (km s-1) BC(V) M V M bol L/L R/R M/M D (pc) [Ba/Eu] Class Var.

DMA subsample

BS 15621-047
4750 1.48 –2.29 –2.35 1.05 –0.384 –1.38 –1.76 02.85 29.73 0.96 9700 –0.49 r B
70 0.09 0.07 0.09 0.05 0.025 0.21 0.20 76.37 2.97 0.09 1188

BS 16033-081
5020 1.84 –2.20 –2.07 1.2 –0.297 –0.61 –0.91 82.92 17.94 0.80 5620 –1.31 r B
50 0.07 0.05 0.07 0.1 0.014 0.13 0.12 21.33 1.12 0.00 542

BS 16077-077
5900 3.19 –2.05 –2.00 1.00 –0.164 1.76 1.59 18.29 4.11 0.95 2344 0.76 s
50 0.08 0.05 0.09 0.20 0.007 0.20 0.20 3.45 0.41 0.09 279

BS 16082-129
5080 1.98 –2.65 –2.59 1.30 –0.298 –0.26 –0.56 32.80 14.92 0.77 5200 ... no?r?
50 0.11 0.06 0.08 0.05 0.014 0.27 0.27 33.05 1.89 0.13 773

BS 16543-097
5220 2.54 –2.48 –2.36 1.85 –0.264 1.00 0.73 40.41 7.80 0.77 1970 –0.49 r
50 0.10 0.06 0.08 0.10 0.012 0.16 0.16 6.10 0.61 0.05 225

BS 16929-005
5250 3.10 –3.15 –3.02 0.90 –0.288 2.40 2.11 11.39 4.09 0.77 1670 –0.74 r
50 0.09 0.06 0.09 0.10 0.010 0.22 0.22 2.29 0.42 0.10 207

CS 22949-008
6000 3.74 –2.45 –2.61 1.5 –0.181 3.32 3.14 4.40 1.95 0.76 1430 ... s?rs?
50 0.07 0.03 0.09 0.1 0.002 0.15 0.15 0.61 0.14 0.05 143

CS 29503-010
6050 3.66 –1.69 –1.70 1.6 –0.135 2.91 2.77 6.17 2.27 0.86 1400 0.12 rs
50 0.08 0.02 0.06 0.1 0.003 0.15 0.15 0.87 0.17 0.05 146

CS 29512-073
5560 3.44 –2.06 –1.88 1.1 –0.195 2.78 2.58 7.35 2.93 0.86 1730 1.05 s
50 0.07 0.02 0.04 0.1 0.006 0.12 0.12 0.85 0.18 0.02 160

CS 29526-110
6650 3.79 –2.19 –2.29 1.6 –0.152 2.85 2.70 6.62 1.95 0.85 1170 0.01 rs B
50 0.07 0.04 0.10 0.1 0.002 0.12 0.12 0.76 0.12 0.02 108

CS 29528-028
7100 4.27 –2.12 –2.17 1.2 –0.155 3.81 3.65 2.75 1.10 0.81 1320 0.33 rs
50 0.07 0.06 0.18 0.3 0.003 0.12 0.12 0.31 0.07 0.02 121

CS 31070-073
6190 3.86 –2.55 –2.64 1.5 –0.181 3.43 3.25 3.99 1.74 0.80 1630 –0.41 r
50 0.07 0.03 0.08 0.1 0.001 0.12 0.12 0.46 0.11 0.02 150

SAT subsample

Tex (K) log g [Fe/H] ξ (km s-1) [Ba/Eu] Class Var.

BS 16080-175
6240  ±  100 3.70  ±  0.1 –1.86  ±  0.2 1.05  ±  0.1 0.5 rs

BS 17436-058
5340  ±  100 2.20  ±  0.1 –1.90  ±  0.2 2.70  ±  0.1 0.44 rs

CS 22183-015
5470  ±  100 2.85  ±  0.1 –2.85  ±  0.2 1.45  ±  0.1 0.52 s?rs?

CS 22887-048
6500  ±  100 3.35  ±  0.1 –1.70  ±  0.2 2.05  ±  0.1 0.51 s?rs? B

CS 22898-027
6240  ±  100 3.72  ±  0.1 –2.30  ±  0.2 1.40  ±  0.1 0.35 rs

CS 29502-092
4970  ±  100 1.70  ±  0.1 –3.05  ±  0.2 1.85  ±  0.1 –1.58 r

Notes. For the DMA subsample, Tex is the excitation temperature, Mbol is the bolometric magnitude, L is the luminosity, R is the radii, M the mass, π the parallax. Uncertainties are shown in the second line. For [Fe/H], the uncertainties are the standard error of the mean abundance, excluding the effects of errors on atmosphere parameters. SAT did not use isochrones, so did not determine values for BC(V), MV, Mbol, L, R, M or D. The last column indicates whether the star is binary or not, according to Tsangarides (2005).

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