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Measuring Dwarf Galaxy Intrinsic Abundance Scatter with Mid-resolution Spectroscopic Surveys: Calibrating APOGEE Abundance Errors
Jennifer Mead et al 2024 The Astrophysical Journal 974 .
Caption: Figure 2.
Same as Figure 1 with the best-fit line subtracted to remove scatter dependence on [Fe/H]. [X/Fe]* = [X/Fe]−〈[X/Fe]〉.
© 2024. The Author(s). Published by the American Astronomical Society.
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