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Semiempirical versus Theoretical Stellar Population Models: A Comparison with Star Clusters

  • Authors: Randa Asa'd, Paula R. T. Coelho, Johina M. John, Igor V. Chilingarian, Gustavo Bruzual, Stephane Charlot

Randa Asa’d et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 3.

Comparison of results for adev, χ2, log(LWA), light-weighted [Fe/H], and Av obtained from multipopulation fits. Left column: difference in derived values between MILES and SynCoMiL SPS models. Right column: difference in derived values between Coelho14ext and SynCoMiL SPS models. Dots are color-coded according to the goodness of fit: blue and green dots represent fits with χ2 ≤ 3 and χ2 > 3 for both SPS models, respectively. The black dots correspond to fits with χ2 ≤ 3 for one SPS model and >3 for the other.

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