Discovery and classification of HE 1153-0518 as a new high-A(C) CEMP-no star among three EMP stars based on abundance patterns from high-resolution spectra.
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2 Pith papers cite this work, alongside 36 external citations. Polarity classification is still indexing.
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Pith papers citing it
36
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2026 2verdicts
UNVERDICTED 2representative citing papers
Derives homogeneous n-capture element abundances for GBSv3 sample via iSpec spectral analysis and clustering for line selection, yielding measurements in agreement with literature.
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Three Extremely Metal-Poor stars: discovery of a new CEMP-no star
Discovery and classification of HE 1153-0518 as a new high-A(C) CEMP-no star among three EMP stars based on abundance patterns from high-resolution spectra.
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Gaia FGK benchmark stars: abundances of \textit{n}-capture elements of the third version
Derives homogeneous n-capture element abundances for GBSv3 sample via iSpec spectral analysis and clustering for line selection, yielding measurements in agreement with literature.