Image Details
Caption: Figure 5.
Comparison of metallicities derived from different models. The x-axis shows results from the BC03 method, while the y-axis displays results from ULYSS using either the Vazdekis (V10) or PEGASE-HR (PEG) models. The dashed line indicates a 1:1 relation. Error bars represent the 1σ uncertainties from each method.
© 2026. The Author(s). Published by the American Astronomical Society.