An international team, with the participation of researchers from the Instituto de Astrofísica de Canarias (IAC), has developed a new generation of calibrations that make it possible to estimate the chemical composition (metallicity) of both nearby galaxies and the most distant and early galaxies in the Universe observed by the James Webb Space Telescope. The study is based on the analysis of the largest collection of high-quality spectroscopic observations gathered to date, the result of more than a decade of compilation and analysis work. To understand the origin and evolution of galaxies
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