Dynamical modeling of 109 cluster members in two strong-lensing clusters recovers sigma0 reliably and rt for galaxies with extended kinematic coverage, producing better profile fits and higher-normalization Faber-Jackson relations than prior strong-lensing or kinematic work.
arXiv preprint arXiv:2510.23863 , year=
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Dynamical models of cluster members to probe the total mass properties of cluster subhalos. I. A comparison with parametric strong lensing models
Dynamical modeling of 109 cluster members in two strong-lensing clusters recovers sigma0 reliably and rt for galaxies with extended kinematic coverage, producing better profile fits and higher-normalization Faber-Jackson relations than prior strong-lensing or kinematic work.