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...

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Príomhchruthaitheoirí:	Ge, J, Yan, R, Cappellari, M, Mao, S, Li, H, Lu, Y
Formáid:	Journal article
Foilsithe / Cruthaithe:	Oxford University Press 2018

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