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dc.contributor.authorAlbert, A.
dc.contributor.authorBesson, David Zeke
dc.date.accessioned2020-12-23T21:41:36Z
dc.date.available2020-12-23T21:41:36Z
dc.date.issued2019-01-16
dc.identifier.citationA. Albert et al 2019 ApJ 870 134en_US
dc.identifier.urihttp://hdl.handle.net/1808/31013
dc.descriptionOriginal content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.en_US
dc.description.abstractAstrophysical 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. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.en_US
dc.publisherAmerican Astronomical Societyen_US
dc.rights© 2019. The American Astronomical Society.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/en_US
dc.subjectGravitational wavesen_US
dc.subjectNeutrinosen_US
dc.titleSearch for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCubeen_US
dc.typeArticleen_US
kusw.kuauthorBesson, David Zeke
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.3847/1538-4357/aaf21den_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


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© 2019. The American Astronomical Society.
Except where otherwise noted, this item's license is described as: © 2019. The American Astronomical Society.