Gravitational wave cosmology with EMRIs
  We show that the loudest extreme mass-ratio inspirals (EMRIs) detected by the
future space-based gravitational wave detector LISA can be used as dark
standard sirens, statistically matching their sky localisation region with mock
galaxy catalogs. In these Proceedings we focus on a realistic EMRI population
scenario and report accuracy predictions for the measure of cosmological
parameters, anticipating the potential of EMRIs to simultaneously constrain the
Hubble constant, the dark matter, and the dark energy density parameters.
