Dark Sirens to Resolve the Hubble-Lema\^itre Tension
  The planned sensitivity upgrades to the LIGO and Virgo facilities could
uniquely identify host galaxies of dark sirens-compact binary coalescences
without any electromagnetic counterparts-within a redshift of z = 0.1. This is
aided by the higher order spherical harmonic modes present in the
gravitational-wave signal, which also improve distance estimation. In
conjunction, sensitivity upgrades and higher modes will facilitate an accurate,
independent measurement of the host galaxy's redshift in addition to the
luminosity distance from the gravitational wave observation to infer the
Hubble-Lema\^itre constant H0 to better than a few percent in five years. A
possible Voyager upgrade or third generation facilities would further solidify
the role of dark sirens for precision cosmology in the future.
