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Table 5

Relative abundances.

HIP Δ[C/H] σ Δ[O/H] σ Δ[Na/H] σ ...

wm: late F-dwarfs

522 −0.059 0.036 −0.066 0.011 −0.183 0.011 ...
3119 −0.106 0.033 −0.031 0.002 −0.192 0.011 ...
3236 −0.213 0.044 −0.117 0.003 −0.242 0.003 ...
3540 −0.146 0.080 −0.164 0.005 −0.288 0.003 ...
5862 −0.041 0.011 −0.032 0.005 −0.097 0.004 ...
5985 −0.157 0.060 −0.136 0.005 −0.228 0.008 ...
7978 −0.260 0.076 −0.230 0.020 −0.440 0.008 ...
8548 −0.089 0.059 −0.142 0.006 −0.236 0.026 ...
12653 −0.106 0.036 −0.032 0.012 −0.179 0.030 ...
12764 −0.076 0.041 −0.069 0.010 −0.229 0.011 ...
. . . . . . . . . . . . . . . . . . . . . . . .
mr: metal-rich solar analogs

1499 −0.103 0.023 −0.099 0.015 −0.134 0.011 ...
1803 −0.215 0.031 −0.086 0.021 −0.206 0.015 ...
5176 −0.130 0.030 −0.121 0.015 −0.148 0.004 ...
12048 −0.229 0.049 −0.141 0.012 −0.340 0.014 ...
12186 −0.253 0.029 −0.155 0.008 −0.298 0.031 ...
17054 0.156 0.034 0.108 0.022 0.234 0.013 ...
17960 −0.126 0.036 −0.080 0.009 −0.183 0.007 ...
20723 −0.027 0.020 −0.031 0.023 −0.059 0.026 ...
20741 −0.244 0.032 −0.102 0.028 −0.263 0.008 ...
21923 −0.153 0.032 −0.065 0.009 −0.177 0.011 ...
. . . . . . . . . . . . . . . . . . . . . . . .

Notes. The Δ values listed here are relative to the reference stars HIP 14954 for the wm sample and HIP 74500 for the mr sample. The σ columns correspond to a simple line-by-line scatter and are not necessarily representative of the true error of our relative, strict differential abundance measurements, which we estimate to be around 0.01 dex.

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