The extreme astrophysical processes and conditions that characterize the early Universe
are expected to result in young galaxies that are dynamically different from those observed …

There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …

Using a single gravitational lens system observed at≲ 5 mas resolution with very long
baseline interferometry, we place a lower bound on the mass of the fuzzy dark matter (FDM) …

We investigate the mass structure of a strong gravitational lens galaxy at z= 0.350, taking
advantage of the milliarcsecond (mas) angular resolution of very long baseline …

Strong gravitational lensing, which can make a background source galaxy appears multiple
times due to its light rays being deflected by the mass of one or more foreground lens …

ABSTRACT A defining prediction of the cold dark matter cosmological model is the
existence of a very large population of low-mass haloes. This population is absent in models …

The large-scale mass distributions of galaxy-scale strong lenses have long been assumed
to be well described by a singular ellipsoidal power-law density profile with external shear …

The vast quantity of strong galaxy–galaxy gravitational lenses expected by future large-scale
surveys necessitates the development of automated methods to efficiently model their mass …

Strong gravitational lensing provides a wealth of astrophysical information on the baryonic
and dark matter content of galaxies. It also serves as a valuable cosmological probe by …

We present modelling of∼ 0.1 arcsec resolution Atacama Large Millimetre/submillimetre
Array imaging of seven strong gravitationally lensed galaxies detected by the Herschel …