Recovering stellar population parameters via two full-spectrum fitting algorithms in the absence of model uncertainties
Using mock spectra based on Vazdekis/MILES library fitted within the wavelength region 3600-7350\AA, we analyze the bias and scatter on the resulting physical parameters induced by the choice of fitting algorithms and observational uncertainties, but avoid effects of those model uncertainties. We co...
| Hoofdauteurs: | , , , , , |
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| Formaat: | Journal article |
| Gepubliceerd in: |
Oxford University Press
2018
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