A dense dark matter core of the subhalo in the strong lensing system JVAS B1938+666
This study presents a non-parametric reconstruction of the dark subhalo in the strong-lensing system JVAS B1938+666, revealing a dense kiloparsec-scale core that is better explained by self-interacting dark matter (SIDM) and fuzzy dark matter models than by standard NFW profiles, with SIDM being the favored framework.