HR-PYPOPSTAR - II. High-spectral-resolution evolutionary synthesis models, low-metallicity expansion, and the properties of the stellar populations of dwarf galaxies

Open Access

Fig. A.1.

Comparison between the old version of HR-PYPOPSTAR using the stellar library of C14 (MI21), in blue line, and the present models using MUN05 PHOENIX+ new PoWR stellar library, in red line, for Z = 0.004 and CHA IMF. The bottom part of every sub-figure shows $Δ L_{M I 21 - n e w} = \frac{L_{M I 21} - L_{new}}{L_{M I 21}}$ $\Delta L_{MI21-new}= \frac{L_{MI21}-L_{new}}{L_{MI21}}$ .

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