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Chemical abundances in high-redshift galaxies: a powerful new emission line diagnostic
, 2016This Letter presents a new, remarkably simple diagnostic specifically designed to derive chemical abundances for high redshift galaxies. It uses only the Hα$\mathrm{H}\alpha$, [N ii] and [S ii] emission lines, which can usually be observed in a single ...
M. Dopita +3 more
semanticscholar +1 more source
Tracking chemical alteration in magmatic zircon using rare earth element abundances
Chemical Geology, 2019Elizabeth A. Bell +3 more
semanticscholar +1 more source