Recovering stellar population parameters via two full-spectrum fitting algorithms in the absence of model uncertainties

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...

書誌詳細
主要な著者:	Ge, J, Yan, R, Cappellari, M, Mao, S, Li, H, Lu, Y
フォーマット:	Journal article
出版事項:	Oxford University Press 2018

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