Individual abundances for μ Leonis derived from spectrum at different resolution and S/N.
|Species||λ||ESPaDOnS||UVES,∞||UVES, low||UVES, high|
|Ba ii||6496||–0.02||0.06||0.15 ± 0.09||0.10 ± 0.08|
|La ii||6390||–0.36||–0.36||–0.33 ± 0.06||–0.37 ± 0.03|
|Nd ii||6740||–0.70||–0.66||–0.56 ± 0.08||–0.65 ± 0.04|
|Ce ii||6043||–0.14||0.02||0.10 ± 0.07||0.02 ± 0.04|
|Eu ii||6645||–0.18||–0.14||–0.10 ± 0.05||–0.14 ± 0.03|
Notes. The column ESPaDOnS lists the abundances derived using the original ESPaDOnS spectrum. The column UVES, ∞ lists the abundances derived using the spectrum degraded to the UVES resolution, with the original S/N. The last two columns give the mean abundances and their standard deviation, obtained from the 101 Monte Carlo simulations for the low and high signal-to-noise hypothesis.
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