While astrophysical and cosmological probes provide a remarkably precise and consistent
picture of the quantity and general properties of dark matter, its fundamental nature remains …

Context. Previous studies have revealed that the estimated probability of galaxy-galaxy
strong lensing in observed galaxy clusters exceeds the expectations from the Λ cold dark …

Ultra-light dark matter (ULDM) refers to a class of theories, including ultra-light axions, in
which particles with mass comprise a significant fraction of the dark matter. A galactic scale …

Context. An excess of galaxy–galaxy strong lensing (GGSL) in galaxy clusters compared to
expectations from the Λ cold-dark-matter (CDM) cosmological model has recently been …

We introduce a machine learning method for estimating the sensitivity of strong lens
observations to dark matter subhaloes in the lens. Our training data include elliptical power …

Modeling the mass distribution of galaxy-scale strong gravitational lenses is a task of
increasing difficulty. The high-resolution and depth of imaging data now available render …

We devise a method to constrain self-interacting dark matter (SIDM) from observations of
quadruply imaged quasars, and apply it to five self-interaction potentials with a long-range …

Strong gravitational lensing can be used to find otherwise invisible dark matter subhaloes. In
such an analysis, the lens galaxy mass model is a significant source of systematic …

Strong gravitational lensing provides a purely gravitational means to infer properties of dark
matter haloes and thereby constrain the particle nature of dark matter. Strong lenses …

We present the first strong-gravitational-lensing analysis of the galaxy cluster RX J0437. 1+
0043 (RXJ0437; z= 0.285). Newly obtained, deep MUSE observations, Keck/MOSFIRE near …