Colours and magnitudes of our program stars before dereddening.
Temperatures derived from photometric data by using the final metallicity found for each star.
Results for the stellar parameters, for the DMA (upper portion) and SAT (lower portion) subsamples.
Average of abundances for the DMA subsample of CEMP stars, and solar abundances used as reference, as well as their sources.
Average of abundances for the SAT subsample of CEMP stars.
Comparison between results from this work and from the literature.
Diference between the output value of the synthesis program (log Ap) and the output value with 1σ of diference in temperature (ΔT), log g (Δlg), metallicity (Δfeh), velocity of microturbulent (Δξ), observational (ΔObs), and macroturbulence Δmu.
© ESO, 2012