Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

TY - JOUR

T1 - Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube

AU - Albert, Andreas

AU - André, M.

AU - Ardid, M.

AU - Aubert, J.J.

AU - Aublin, J.

AU - Avgitas, T.

AU - Baret, B.

AU - Barrios-Marti, J.

AU - Basa, S.

AU - Belhorma, B.

AU - Bertin, V.

AU - Biagi, S.

AU - Bormuth, R.

AU - Boumaaza, J.

AU - Bourret, S.

AU - Bouwhuis, Marna

AU - Brânzaş, H.

AU - Bruijn, R.

AU - Brunner, Jurgen

AU - Busto, Jesús H.

AU - Capone, A.

AU - Caramete, L.

AU - Carr, J.

AU - Celli, S.

AU - Chabab, M.

AU - Cherkaoui El Moursli, R.

AU - Chiarusi, T.

AU - Antares, and Icecube

AU - Ahlers, Markus Tobias

AU - Bourbeau, Etienne

AU - Koskinen, D. Jason

AU - Larson, Michael James

AU - Medici, Morten Ankersen

AU - Sarkar, Subir

AU - Stuttard, Thomas Simon

AU - Rameez, M

PY - 2019/1/10

Y1 - 2019/1/10

N2 - 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. 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.

AB - 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. 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.

U2 - 10.3847/1538-4357/aaf21d

DO - 10.3847/1538-4357/aaf21d

M3 - Journal article

SN - 0004-637X

VL - 870

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 134

ER -