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J. 870(2)</i>: 134. <a href=\"https://doi.org/10.3847/1538-4357/aaf21d\" target=\"_blank\">https://doi.org/10.3847/1538-4357/aaf21d</a>","DocTypID":8,"DocType":"Journal article","MarineFlag":0,"FreshFlag":0,"BrackishFlag":0,"TerrestrialFlag":0,"Authorstring":"ANTARES Collaboration; IceCube Collaboration; LIGO Scientific Collaboration; VIRGO Collaboration; van Haren, H.","OrigTitleTranslFlag":0,"Authorstringtrunc":"ANTARES Collaboration <i>et al.</i>","Englishabstract":"Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. 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