  In 2013, the IceCube Collaboration reported the first observation of an
astrophysical neutrino flux, with energies extending up to the PeV-scale. Over
the last decade, this flux has been characterized by measurements in multiple
detection channels that are complementary with respect to the sensitive energy
range, flavor composition, sky coverage, and backgrounds. The origin of these
neutrinos remains largely unknown. However, evidence has been found for
neutrino emission from the directions of the blazar TXS 0506+056, Seyfert
galaxy NGC 1068. and the Galactic Plane. IceCube also has an active program of
indirect dark matter searches with competitive constraints on dark matter
models. In this talk, we will present recent results of the IceCube experiment,
highlighting the latest diffuse flux measurements, point source searches, and
dark matter analyses.
