In my talk i will summarize some results obtained from strong lensing, weak lensing, and dynamical analyses of galaxies in clusters and the field. What can we conclude on their dark matter haloes and are conclusions on the IMF of their stars robust?
In my talk i will summarize some results obtained from strong lensing, weak lensing, and dynamical analyses of galaxies in clusters and the field. What can we conclude on their dark matter haloes and are conclusions on the IMF of their stars robust?
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