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...
Үндсэн зохиолчид: | Ge, J, Yan, R, Cappellari, M, Mao, S, Li, H, Lu, Y |
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Формат: | Journal article |
Хэвлэсэн: |
Oxford University Press
2018
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