Abstract
For 18 well-observed gravitationally lensed QSOs, we compare new non-parametric mass profiles for the lensing galaxies with stellar-population models derived from published HST photometry. The large volume of parameter space searched -- with respect to the possible star formation histories -- allows us to infer robust estimates and uncertainties for the stellar masses. The most interesting results are: (1) the transition from little or no dark matter in the inner regions (
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CITATION STYLE
Ferreras, I., Saha, P., & Williams, L. L. R. (2005). Stellar and Total Mass in Early-Type Lensing Galaxies. The Astrophysical Journal, 623(1), L5–L8. https://doi.org/10.1086/429995
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