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Published in Springer Link (Chiba Institute of Technology) • Jun 29, 2021
NobleIDNI0P97W88R66S55
Authors:,,
R. E. Giribaldi
A. R. da Silva
R. Smiljanic
Abstract
\nContext. Several large stellar spectroscopic surveys are producing enormous amounts of data that can be used to determine stellar atmospheric parameters and chemical abundances. Nonetheless, the accuracy achieved in the derived astrophysical parameters is still insufficient, mainly because of the ...