The past few years have witnessed exciting discoveries in particle astrophysics. Astrophysical neutrinos, with the highest energy ever observed, have been detected by the IceCube telescope, launching the high-energy neutrino astronomy era. LIGO has spotted, for the first time, gravitational waves from compact star merging. Our knowledge of the gamma-ray sky has dramatically improved thanks to the Fermi telescope. By combining information coming from such a pletora of data, we are now starting to learn about of thermal and non-thermal astrophysical sources and their properties. We here present a concise summary of the status of the art in the field as reported in the ``Multimessenger astrophysics'' parallel session of Neutrino Oscillation Workshop 2016.